<rss version="2.0" xmlns:media="http://search.yahoo.com/mrss/" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Docstoc feed for: Education-&gt;Graduate-&gt;Physics</title><link>http://www.docstoc.com/documents/education//graduate//physics/most-recent/</link><description>The following documents are the recent documents shared by the docstoc community in the Education-&gt;Graduate-&gt;Physics category</description><image><url>http://i.docstoccdn.com/logo.gif</url><title>Docstoc.com</title><link>http://www.docstoc.com</link></image><atom:icon>http://i.docstoccdn.com/logo.gif</atom:icon><ttl>10</ttl><pubDate>Tue, 01 Dec 2009 01:07:33 GMT</pubDate><lastBuildDate>Tue, 01 Dec 2009 01:07:33 GMT</lastBuildDate><item><title>Adaptations for Children with Disabilities</title><link>http://www.docstoc.com/docs/14378962/Adaptations-for-Children-with-Disabilities</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/14378962/Adaptations-for-Children-with-Disabilities title="Adaptations for Children with Disabilities"&lt;img src="http://img.docstoc.com/thumb/100/14378962.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/susanaudi"&gt;susanaudi&lt;/a&gt; on: Saturday, October 31, 2009&lt;p&gt;ADAPTATIONS FOR A DISABILITYWRITE A BEHAVIORAL OBJECTIVE FOR A YOUNG CHILD. The student will be able to wash his/her hands after eating each meal or after going to the bathroom with 4-6 trials daily for 12 weeks. DESCRIBE POSSIBLE ACTIVITIES TO GO WITH THE OBJECTIVE. HAND WASHING * One activity will be stand behind the child and physically prom&lt;/p&gt;&lt;/div&gt;</description><author>susanaudi</author><pubDate>Sat, 31 Oct 2009 13:15:47 GMT</pubDate><guid>http://www.docstoc.com/docs/14378962/Adaptations-for-Children-with-Disabilities</guid></item><item><title>Anomali cuaca dan iklim</title><link>http://www.docstoc.com/docs/13823420/Anomali-cuaca-dan-iklim</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/13823420/Anomali-cuaca-dan-iklim title="Anomali cuaca dan iklim"&lt;img src="http://img.docstoc.com/thumb/100/13823420.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/jokowiratmo"&gt;jokowiratmo&lt;/a&gt; on: Sunday, October 25, 2009&lt;p&gt;Anomali cuaca dan iklim hampir selalu berkaitan dengan bencana. Untuk Indonesia bencana yang sering terjadi akibat anomali cuaca dan iklim ini adalah banjir dan kekeringan. Bencana yang timbul mungkin juga tidak hanya disebabkan oleh faktor lokal, tetapi bisa regional bahkan global. El Nino, La Nina, pemanasan global merupakan contoh dari faktor-faktor global yang mempengaruhi iklim. &lt;/p&gt;&lt;/div&gt;</description><author>jokowiratmo</author><pubDate>Sun, 25 Oct 2009 22:33:06 GMT</pubDate><guid>http://www.docstoc.com/docs/13823420/Anomali-cuaca-dan-iklim</guid></item><item><title>A Course in Fluid Mechanics with Vector Field Theory by Dennis C. Prieve</title><link>http://www.docstoc.com/docs/13553457/A-Course-in-Fluid-Mechanics-with-Vector-Field-Theory-by-Dennis-C-Prieve</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/13553457/A-Course-in-Fluid-Mechanics-with-Vector-Field-Theory-by-Dennis-C-Prieve title="A Course in Fluid Mechanics with Vector Field Theory by Dennis C. Prieve"&lt;img src="http://img.docstoc.com/thumb/100/13553457.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/twaha"&gt;twaha&lt;/a&gt; on: Thursday, October 22, 2009&lt;p&gt;This book clearly describes the advanced topics of fluid mechanics, starting from algebra of vector fields and tensors to electrodynamics. Should be a great book for understanding the concepts of fluid mechanics.&lt;/p&gt;&lt;/div&gt;</description><author>twaha</author><pubDate>Thu, 22 Oct 2009 09:27:08 GMT</pubDate><guid>http://www.docstoc.com/docs/13553457/A-Course-in-Fluid-Mechanics-with-Vector-Field-Theory-by-Dennis-C-Prieve</guid></item><item><title>Classical Mechanics 5th ed by Tom W.B. Kibble and Frank H. Berkshire</title><link>http://www.docstoc.com/docs/13552987/Classical-Mechanics-5th-ed-by-Tom-WB-Kibble-and-Frank-H-Berkshire</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/13552987/Classical-Mechanics-5th-ed-by-Tom-WB-Kibble-and-Frank-H-Berkshire title="Classical Mechanics 5th ed by Tom W.B. Kibble and Frank H. Berkshire"&lt;img src="http://img.docstoc.com/thumb/100/13552987.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/twaha"&gt;twaha&lt;/a&gt; on: Thursday, October 22, 2009&lt;p&gt;An excellent book on classical mechanics published by Imperial College Press, London. This book is based on course given Physics and Applied Mathematics students. Prerequisite is knowledge of Differential and integrial calculus including partials but not differential equations.&lt;/p&gt;&lt;/div&gt;</description><author>twaha</author><pubDate>Thu, 22 Oct 2009 09:12:23 GMT</pubDate><guid>http://www.docstoc.com/docs/13552987/Classical-Mechanics-5th-ed-by-Tom-WB-Kibble-and-Frank-H-Berkshire</guid></item><item><title>El Nino dan produksi pangan di Indonesia</title><link>http://www.docstoc.com/docs/13532636/El-Nino-dan-produksi-pangan-di-Indonesia</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/13532636/El-Nino-dan-produksi-pangan-di-Indonesia title="El Nino dan produksi pangan di Indonesia"&lt;img src="http://img.docstoc.com/thumb/100/13532636.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/jokowiratmo"&gt;jokowiratmo&lt;/a&gt; on: Thursday, October 22, 2009&lt;p&gt;El Nino berdampak pada cuaca dan iklim di Indonesia. Ia menyebabkan curah hujan di sebagian besar wilayah Indonesia berkurang. Ini berimbas pada produksi pangan karena kebutuhan air tanaman khususnya lahan tadah hujan tidak tercukupi.&lt;/p&gt;&lt;/div&gt;</description><author>jokowiratmo</author><pubDate>Thu, 22 Oct 2009 00:58:42 GMT</pubDate><guid>http://www.docstoc.com/docs/13532636/El-Nino-dan-produksi-pangan-di-Indonesia</guid></item><item><title>Experimental Techniques in Low Temperature</title><link>http://www.docstoc.com/docs/12646828/Experimental-Techniques-in-Low-Temperature</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12646828/Experimental-Techniques-in-Low-Temperature title="Experimental Techniques in Low Temperature"&lt;img src="http://img.docstoc.com/thumb/100/12646828.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Monday, October 05, 2009&lt;p&gt;No description&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Mon, 05 Oct 2009 21:41:26 GMT</pubDate><guid>http://www.docstoc.com/docs/12646828/Experimental-Techniques-in-Low-Temperature</guid></item><item><title>Great Physicists From Galileo to Hawking</title><link>http://www.docstoc.com/docs/12398901/Great-Physicists-From-Galileo-to-Hawking</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12398901/Great-Physicists-From-Galileo-to-Hawking title="Great Physicists From Galileo to Hawking"&lt;img src="http://img.docstoc.com/thumb/100/12398901.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Great PhysicistsGreat PhysicistsThe Life and Times of Leading Physicists from Galileo to HawkingWilliam H. Cropper120011Oxford New York Athens Auckland Bangkok Bogota Buenos Aires  Cape Town Chennai Dar es Salaam Delhi Florence Hong Kong Istanbul Karachi Kolkata Kuala Lumpur Madrid Melbourne Mexico City Mumbai Nairobi Pari&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 05:39:31 GMT</pubDate><guid>http://www.docstoc.com/docs/12398901/Great-Physicists-From-Galileo-to-Hawking</guid></item><item><title>CF-INDIC</title><link>http://www.docstoc.com/docs/12393029/CF-INDIC</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12393029/CF-INDIC title="CF-INDIC"&lt;img src="http://img.docstoc.com/thumb/100/12393029.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:17:45 GMT</pubDate><guid>http://www.docstoc.com/docs/12393029/CF-INDIC</guid></item><item><title>CE-PUBLI</title><link>http://www.docstoc.com/docs/12392919/CE-PUBLI</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12392919/CE-PUBLI title="CE-PUBLI"&lt;img src="http://img.docstoc.com/thumb/100/12392919.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:15:54 GMT</pubDate><guid>http://www.docstoc.com/docs/12392919/CE-PUBLI</guid></item><item><title>CD-MATHS</title><link>http://www.docstoc.com/docs/12392847/CD-MATHS</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12392847/CD-MATHS title="CD-MATHS"&lt;img src="http://img.docstoc.com/thumb/100/12392847.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:14:39 GMT</pubDate><guid>http://www.docstoc.com/docs/12392847/CD-MATHS</guid></item><item><title>CC-PARTS</title><link>http://www.docstoc.com/docs/12392838/CC-PARTS</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12392838/CC-PARTS title="CC-PARTS"&lt;img src="http://img.docstoc.com/thumb/100/12392838.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:14:29 GMT</pubDate><guid>http://www.docstoc.com/docs/12392838/CC-PARTS</guid></item><item><title>CB-UNITS</title><link>http://www.docstoc.com/docs/12392831/CB-UNITS</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12392831/CB-UNITS title="CB-UNITS"&lt;img src="http://img.docstoc.com/thumb/100/12392831.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:14:20 GMT</pubDate><guid>http://www.docstoc.com/docs/12392831/CB-UNITS</guid></item><item><title>CA-NOTAT</title><link>http://www.docstoc.com/docs/12392828/CA-NOTAT</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12392828/CA-NOTAT title="CA-NOTAT"&lt;img src="http://img.docstoc.com/thumb/100/12392828.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:14:12 GMT</pubDate><guid>http://www.docstoc.com/docs/12392828/CA-NOTAT</guid></item><item><title>C-8-QMNU</title><link>http://www.docstoc.com/docs/12392746/C-8-QMNU</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12392746/C-8-QMNU title="C-8-QMNU"&lt;img src="http://img.docstoc.com/thumb/100/12392746.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:13:24 GMT</pubDate><guid>http://www.docstoc.com/docs/12392746/C-8-QMNU</guid></item><item><title>C-7-NUCL</title><link>http://www.docstoc.com/docs/12392724/C-7-NUCL</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12392724/C-7-NUCL title="C-7-NUCL"&lt;img src="http://img.docstoc.com/thumb/100/12392724.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:13:15 GMT</pubDate><guid>http://www.docstoc.com/docs/12392724/C-7-NUCL</guid></item><item><title>C-6-PERM</title><link>http://www.docstoc.com/docs/12392512/C-6-PERM</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12392512/C-6-PERM title="C-6-PERM"&lt;img src="http://img.docstoc.com/thumb/100/12392512.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:11:39 GMT</pubDate><guid>http://www.docstoc.com/docs/12392512/C-6-PERM</guid></item><item><title>C-5-QEDD</title><link>http://www.docstoc.com/docs/12392500/C-5-QEDD</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12392500/C-5-QEDD title="C-5-QEDD"&lt;img src="http://img.docstoc.com/thumb/100/12392500.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:11:31 GMT</pubDate><guid>http://www.docstoc.com/docs/12392500/C-5-QEDD</guid></item><item><title>C-5-QEDC</title><link>http://www.docstoc.com/docs/12392465/C-5-QEDC</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12392465/C-5-QEDC title="C-5-QEDC"&lt;img src="http://img.docstoc.com/thumb/100/12392465.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:11:13 GMT</pubDate><guid>http://www.docstoc.com/docs/12392465/C-5-QEDC</guid></item><item><title>C-5-QEDB</title><link>http://www.docstoc.com/docs/12392451/C-5-QEDB</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12392451/C-5-QEDB title="C-5-QEDB"&lt;img src="http://img.docstoc.com/thumb/100/12392451.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:11:03 GMT</pubDate><guid>http://www.docstoc.com/docs/12392451/C-5-QEDB</guid></item><item><title>C-5-QEDA</title><link>http://www.docstoc.com/docs/12392417/C-5-QEDA</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12392417/C-5-QEDA title="C-5-QEDA"&lt;img src="http://img.docstoc.com/thumb/100/12392417.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:10:51 GMT</pubDate><guid>http://www.docstoc.com/docs/12392417/C-5-QEDA</guid></item><item><title>C-4-GRVA</title><link>http://www.docstoc.com/docs/12392362/C-4-GRVA</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12392362/C-4-GRVA title="C-4-GRVA"&lt;img src="http://img.docstoc.com/thumb/100/12392362.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:10:22 GMT</pubDate><guid>http://www.docstoc.com/docs/12392362/C-4-GRVA</guid></item><item><title>C-3-PEPA</title><link>http://www.docstoc.com/docs/12392028/C-3-PEPA</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12392028/C-3-PEPA title="C-3-PEPA"&lt;img src="http://img.docstoc.com/thumb/100/12392028.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:07:32 GMT</pubDate><guid>http://www.docstoc.com/docs/12392028/C-3-PEPA</guid></item><item><title>C-2-CLSD</title><link>http://www.docstoc.com/docs/12391952/C-2-CLSD</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12391952/C-2-CLSD title="C-2-CLSD"&lt;img src="http://img.docstoc.com/thumb/100/12391952.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:06:54 GMT</pubDate><guid>http://www.docstoc.com/docs/12391952/C-2-CLSD</guid></item><item><title>C-2-CLSC</title><link>http://www.docstoc.com/docs/12391669/C-2-CLSC</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12391669/C-2-CLSC title="C-2-CLSC"&lt;img src="http://img.docstoc.com/thumb/100/12391669.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:04:26 GMT</pubDate><guid>http://www.docstoc.com/docs/12391669/C-2-CLSC</guid></item><item><title>C-2-CLSB</title><link>http://www.docstoc.com/docs/12391479/C-2-CLSB</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12391479/C-2-CLSB title="C-2-CLSB"&lt;img src="http://img.docstoc.com/thumb/100/12391479.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:02:50 GMT</pubDate><guid>http://www.docstoc.com/docs/12391479/C-2-CLSB</guid></item><item><title>C-2-CLSA</title><link>http://www.docstoc.com/docs/12391344/C-2-CLSA</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12391344/C-2-CLSA title="C-2-CLSA"&lt;img src="http://img.docstoc.com/thumb/100/12391344.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 04:01:26 GMT</pubDate><guid>http://www.docstoc.com/docs/12391344/C-2-CLSA</guid></item><item><title>C-0-INTR</title><link>http://www.docstoc.com/docs/12391113/C-0-INTR</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12391113/C-0-INTR title="C-0-INTR"&lt;img src="http://img.docstoc.com/thumb/100/12391113.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 03:58:40 GMT</pubDate><guid>http://www.docstoc.com/docs/12391113/C-0-INTR</guid></item><item><title>C15-SEXP</title><link>http://www.docstoc.com/docs/12391074/C15-SEXP</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12391074/C15-SEXP title="C15-SEXP"&lt;img src="http://img.docstoc.com/thumb/100/12391074.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 03:58:22 GMT</pubDate><guid>http://www.docstoc.com/docs/12391074/C15-SEXP</guid></item><item><title>C12-EXTD</title><link>http://www.docstoc.com/docs/12391058/C12-EXTD</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12391058/C12-EXTD title="C12-EXTD"&lt;img src="http://img.docstoc.com/thumb/100/12391058.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 03:58:16 GMT</pubDate><guid>http://www.docstoc.com/docs/12391058/C12-EXTD</guid></item><item><title>C11-LGSM</title><link>http://www.docstoc.com/docs/12391018/C11-LGSM</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12391018/C11-LGSM title="C11-LGSM"&lt;img src="http://img.docstoc.com/thumb/100/12391018.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 03:57:57 GMT</pubDate><guid>http://www.docstoc.com/docs/12391018/C11-LGSM</guid></item><item><title>C10-QMGR</title><link>http://www.docstoc.com/docs/12390978/C10-QMGR</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/12390978/C10-QMGR title="C10-QMGR"&lt;img src="http://img.docstoc.com/thumb/100/12390978.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Friday, October 02, 2009&lt;p&gt;Physics&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Fri, 02 Oct 2009 03:57:36 GMT</pubDate><guid>http://www.docstoc.com/docs/12390978/C10-QMGR</guid></item><item><title>The Bend : A Speculation on History and Science</title><link>http://www.docstoc.com/docs/11294418/The-Bend--A-Speculation-on-History-and-Science</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/11294418/The-Bend--A-Speculation-on-History-and-Science title="The Bend : A Speculation on History and Science"&lt;img src="http://img.docstoc.com/thumb/100/11294418.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/mkirsh"&gt;mkirsh&lt;/a&gt; on: Monday, September 14, 2009&lt;p&gt;The age of human civilization is given the name “the bend” based on a re-examination of the emergence of science, science theory content, and history.&lt;/p&gt;&lt;/div&gt;</description><author>mkirsh</author><pubDate>Mon, 14 Sep 2009 19:32:56 GMT</pubDate><guid>http://www.docstoc.com/docs/11294418/The-Bend--A-Speculation-on-History-and-Science</guid></item><item><title>Fisika</title><link>http://www.docstoc.com/docs/11264990/Fisika</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/11264990/Fisika title="Fisika"&lt;img src="http://img.docstoc.com/thumb/100/11264990.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Monday, September 14, 2009&lt;p&gt;Gelombang Mekanis1SUMBER-SUMBER BUNYIGETARAN BUNYI Sehelai dawai ditegangkan dengan beban variabel. Jika dawai dipetik di tengah-tengahnya, maka seluruh dawai akan bergetar membentuk setengah panjang gelombang. Gelombang yang terjadi adalah gelombang stasioner, pada bagian ujung terjadi simpul dan di bagain tengah terjadi perut. jadi panj&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Mon, 14 Sep 2009 01:18:53 GMT</pubDate><guid>http://www.docstoc.com/docs/11264990/Fisika</guid></item><item><title>Deriving drainage networks and catchment boundaries</title><link>http://www.docstoc.com/docs/11018375/Deriving-drainage-networks-and-catchment-boundaries</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/11018375/Deriving-drainage-networks-and-catchment-boundaries title="Deriving drainage networks and catchment boundaries"&lt;img src="http://img.docstoc.com/thumb/100/11018375.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/smspdev"&gt;smspdev&lt;/a&gt; on: Wednesday, September 09, 2009&lt;p&gt;sfdsdfsdfsdfdsfds&lt;/p&gt;&lt;/div&gt;</description><author>smspdev</author><pubDate>Wed, 09 Sep 2009 07:44:38 GMT</pubDate><guid>http://www.docstoc.com/docs/11018375/Deriving-drainage-networks-and-catchment-boundaries</guid></item><item><title>Teori Cahaya</title><link>http://www.docstoc.com/docs/10424893/Teori-Cahaya</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/10424893/Teori-Cahaya title="Teori Cahaya"&lt;img src="http://img.docstoc.com/thumb/100/10424893.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/roylamhot"&gt;roylamhot&lt;/a&gt; on: Wednesday, August 26, 2009&lt;p&gt;TEORI CAHAYAFakultas Teknik Elektro &amp; KomunikasiTeori Cahaya• Pendekatan optika geometris– – – – – – – Cahaya merambat lurus Kecepatan di r hampa c=1/ √(εoμo) ≈ 3 x 108 m/s Kec di medium lain v = c/n ; n adalah indeks bias medium n = c/v =√(εμ)/√(εoμo) . o : Permitivitas hampa udara = 8,85 x 10-12 C2 N-1 m-2o: Permeabilitas hampa&lt;/p&gt;&lt;/div&gt;</description><author>roylamhot</author><pubDate>Wed, 26 Aug 2009 07:18:19 GMT</pubDate><guid>http://www.docstoc.com/docs/10424893/Teori-Cahaya</guid></item><item><title>Fundamental Quantum Mechanics for Engineers</title><link>http://www.docstoc.com/docs/9120605/Fundamental-Quantum-Mechanics-for-Engineers</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/9120605/Fundamental-Quantum-Mechanics-for-Engineers title="Fundamental Quantum Mechanics for Engineers"&lt;img src="http://img.docstoc.com/thumb/100/9120605.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/jaymody"&gt;jaymody&lt;/a&gt; on: Thursday, July 30, 2009&lt;p&gt;Fundamental Quantum Mechanics for EngineersLeon van Dommelen 07/14/08 Version 3 beta 4.2CopyrightCopyright 2004 and on, Leon van Dommelen. You are allowed to copy or print out this work in unmodiﬁed work for your personal use. You are allowed to attach additional notes, corrections, and additions, as long as they are clearly identiﬁed&lt;/p&gt;&lt;/div&gt;</description><author>jaymody</author><pubDate>Thu, 30 Jul 2009 00:05:52 GMT</pubDate><guid>http://www.docstoc.com/docs/9120605/Fundamental-Quantum-Mechanics-for-Engineers</guid></item><item><title>Fields</title><link>http://www.docstoc.com/docs/9119990/Fields</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/9119990/Fields title="Fields"&lt;img src="http://img.docstoc.com/thumb/100/9119990.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/jaymody"&gt;jaymody&lt;/a&gt; on: Wednesday, July 29, 2009&lt;p&gt;FIELDSWarren SiegelC. N. Yang Institute for Theoretical Physics State University of New York at Stony Brook Stony Brook, New York 11794-3840 USA mailto:siegel@insti.physics.sunysb.edu http://insti.physics.sunysb.edu/˜siegel/plan.html2CONTENTSPreface . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23 .................. . . .&lt;/p&gt;&lt;/div&gt;</description><author>jaymody</author><pubDate>Wed, 29 Jul 2009 23:57:58 GMT</pubDate><guid>http://www.docstoc.com/docs/9119990/Fields</guid></item><item><title>Physical Foundations of Solid-State Devices</title><link>http://www.docstoc.com/docs/8979481/Physical-Foundations-of-Solid-State-Devices</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/8979481/Physical-Foundations-of-Solid-State-Devices title="Physical Foundations of Solid-State Devices"&lt;img src="http://img.docstoc.com/thumb/100/8979481.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/jaymody"&gt;jaymody&lt;/a&gt; on: Monday, July 27, 2009&lt;p&gt;Physical Foundations of Solid-State DevicesE. F. Schubert Rensselaer Polytechnic Institute Troy, New York 2007 Edition E. F. Schubert, 2007 The use of this book for non-commercial educational purposes is permitted. This book is recommended as an introductory text for graduate students in Electrical Engineering, Applied Physics, and Material &lt;/p&gt;&lt;/div&gt;</description><author>jaymody</author><pubDate>Mon, 27 Jul 2009 01:09:56 GMT</pubDate><guid>http://www.docstoc.com/docs/8979481/Physical-Foundations-of-Solid-State-Devices</guid></item><item><title>My PhD thesis</title><link>http://www.docstoc.com/docs/8846128/My-PhD-thesis</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/8846128/My-PhD-thesis title="My PhD thesis"&lt;img src="http://img.docstoc.com/thumb/100/8846128.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/edgaravalos"&gt;edgaravalos&lt;/a&gt; on: Thursday, July 23, 2009&lt;p&gt;Nonconformal Interaction Models and Thermodynamics of Polar Fluids(Def: Dec, 03, 2004. Grad.: March 2005).&lt;/p&gt;&lt;/div&gt;</description><author>edgaravalos</author><pubDate>Thu, 23 Jul 2009 22:43:01 GMT</pubDate><guid>http://www.docstoc.com/docs/8846128/My-PhD-thesis</guid></item><item><title>20 Địa  </title><link>http://www.docstoc.com/docs/8743747/20-Địa</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/8743747/20-Địa title="20 Địa  "&lt;img src="http://img.docstoc.com/thumb/100/8743747.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/trananhnguyet19451"&gt;trananhnguyet19451&lt;/a&gt; on: Tuesday, July 21, 2009&lt;p&gt;1.1 http://www.docstoc.com/docs/document-preview.aspx?doc_id=8713016 1.2 http://www.docstoc.com/docs/document-preview.aspx?doc_id=8712909 2 http://www.docstoc.com/docs/document-preview.aspx?doc_id=87126723.1 http://www.docstoc.com/docs/document-preview.aspx?doc_id=8712583 3.2 http://www.docstoc.com/docs/document-preview.aspx?doc_id=8712458 4 ht&lt;/p&gt;&lt;/div&gt;</description><author>trananhnguyet19451</author><pubDate>Tue, 21 Jul 2009 01:54:50 GMT</pubDate><guid>http://www.docstoc.com/docs/8743747/20-Địa</guid></item><item><title>Maple-Mekanika</title><link>http://www.docstoc.com/docs/8259228/Maple-Mekanika</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/8259228/Maple-Mekanika title="Maple-Mekanika"&lt;img src="http://img.docstoc.com/thumb/100/8259228.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Thursday, July 09, 2009&lt;p&gt;11. Aplikasi dalam mekanikaI. Gerak lurus berubah beraturan &gt; restart; ketinggian:=5+40*t-8*t^2; plot(ketinggian,t=0..5); kecepatan:= diff(ketinggian,t); plot(kecepatan,t=0..5); percepatan:=diff(kecepatan,t); plot(percepatan,t=0..5); II. Gerak Parabola &gt; restart; x:=vo*cos(Pi/6)*t; y:=vo*sin(Pi/6)*t-1/2*g*t^2; plot([subs(vo=20,g=9.8,x(t)),subs(vo&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Thu, 09 Jul 2009 06:58:07 GMT</pubDate><guid>http://www.docstoc.com/docs/8259228/Maple-Mekanika</guid></item><item><title>Boiler</title><link>http://www.docstoc.com/docs/8102215/Boiler</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/8102215/Boiler title="Boiler"&lt;img src="http://img.docstoc.com/thumb/100/8102215.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Sunday, July 05, 2009&lt;p&gt;DISUSUN OLEH: IR. SOERIPTO M.KEPALA PUSAT HIPERKES DEPARTEMEN TENAGA KERJA JL. JEND. A. YANI NO 69-70 JAKARTA1AIR PENGISI KETEL UAP DAN PENGOLAHANNYA (Ir. Soeripto M.)I. SUSUNAN AIR PENGISI A. Kotoran di dalam air pengisi 1. Air alam yang digunakan untuk pengisian ketel uap umumnya mengandung bahan-bahan padat dan gas-gas terlarut &lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Sun, 05 Jul 2009 04:13:17 GMT</pubDate><guid>http://www.docstoc.com/docs/8102215/Boiler</guid></item><item><title>Elektronika</title><link>http://www.docstoc.com/docs/8096080/Elektronika</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/8096080/Elektronika title="Elektronika"&lt;img src="http://img.docstoc.com/thumb/100/8096080.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Saturday, July 04, 2009&lt;p&gt;Arus Listrik &amp; Rangkaian Arus DCDede Djuhana Departemen Fisika FMIPA UIdede@fisika.ui.ac.id0-0Kuliah Fisika DasarArus Listrik &amp; Rangkaian Arus DCArus dan Gerak Muatan• Arus listrik, I dideﬁnisikan sebagai laju aliran muatan listrik ,∆Q yang melalui suatu penampang dalam waktu tertentu,∆tI=satuan arus listrik adalah ampere&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Sat, 04 Jul 2009 05:37:47 GMT</pubDate><guid>http://www.docstoc.com/docs/8096080/Elektronika</guid></item><item><title>Kristal Mineral</title><link>http://www.docstoc.com/docs/8043585/Kristal-Mineral</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/8043585/Kristal-Mineral title="Kristal Mineral"&lt;img src="http://img.docstoc.com/thumb/100/8043585.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Wednesday, July 01, 2009&lt;p&gt;PEMBENTUKAN MINERAL Mineral tanah adalah mineral yang terkandung di dalam tanah dan merupakan salah satu bahan utama penyusun tanah. Mineral dalam tanah berasal dari pelapukan fisik dan kimia dari batuan yang merupakan bahan induk tanah, rekristalisasi dari senyawa-senyawa hasil pelapukan lainnya atau pelapukan (alterasi) dari mineral primer dan se&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Wed, 01 Jul 2009 19:52:45 GMT</pubDate><guid>http://www.docstoc.com/docs/8043585/Kristal-Mineral</guid></item><item><title>Steam Turbine</title><link>http://www.docstoc.com/docs/8043319/Steam-Turbine</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/8043319/Steam-Turbine title="Steam Turbine"&lt;img src="http://img.docstoc.com/thumb/100/8043319.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Wednesday, July 01, 2009&lt;p&gt;Steam TurbineSteam turbines are devices which convert the energy stored in steam into rotational mechanical energy. These machines are widely used for the generation of electricity in a number of different cycles, such as:   Rankine cycle Reheat cycle Regenerative cycle Combined cycleThe steam turbine may consists of several stages.&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Wed, 01 Jul 2009 19:43:23 GMT</pubDate><guid>http://www.docstoc.com/docs/8043319/Steam-Turbine</guid></item><item><title>Sistem Tenaga</title><link>http://www.docstoc.com/docs/8042735/Sistem-Tenaga</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/8042735/Sistem-Tenaga title="Sistem Tenaga"&lt;img src="http://img.docstoc.com/thumb/100/8042735.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Wednesday, July 01, 2009&lt;p&gt;SISTEM TENAGAElemen Sistem TenagaSalah satu cara yang paling ekonomis, mudah dan aman untuk mengirimkan energi adalah melalui bentuk energi listrik. Pada pusat pembangkit, sumberdaya energi primer seperti bahan bakar fosil (minyak, gas alam, dan batubara), hidro, panas bumi dan nuklir diubah menjadi energi listrik. Generator sinkro mengubah ene&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Wed, 01 Jul 2009 19:29:04 GMT</pubDate><guid>http://www.docstoc.com/docs/8042735/Sistem-Tenaga</guid></item><item><title>Photovoltaic Basics</title><link>http://www.docstoc.com/docs/7982611/Photovoltaic-Basics</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/7982611/Photovoltaic-Basics title="Photovoltaic Basics"&lt;img src="http://img.docstoc.com/thumb/100/7982611.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/cord"&gt;cord&lt;/a&gt; on: Tuesday, June 30, 2009&lt;p&gt;11 Photovoltaic Basics1.1 PV array systems and PV applications1.1.1 OverviewPhotovoltaic (PV) systems can be grouped into stand-alone systems and gridconnected systems. In stand-alone systems the solar energy yield is matched to the energy demand. Since the solar energy yield often does not coincide in time with the energy demand from t&lt;/p&gt;&lt;/div&gt;</description><author>cord</author><pubDate>Tue, 30 Jun 2009 16:15:01 GMT</pubDate><guid>http://www.docstoc.com/docs/7982611/Photovoltaic-Basics</guid></item><item><title>Optical reflection and transmission formulae for thin films</title><link>http://www.docstoc.com/docs/7982432/Optical-reflection-and-transmission-formulae-for-thin-films</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/7982432/Optical-reflection-and-transmission-formulae-for-thin-films title="Optical reflection and transmission formulae for thin films"&lt;img src="http://img.docstoc.com/thumb/100/7982432.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/cord"&gt;cord&lt;/a&gt; on: Tuesday, June 30, 2009&lt;p&gt;Semiconductor Materials for Intermediate Band Solar CellsOctober 19, 2004 GCEP Solar Energy Workshop Stanford, CAW. WalukiewiczElectronic Materials Program Materials Sciences Division Lawrence Berkeley National LaboratoryThis work was supported by the Director's Innovation Initiative, National Reconnaissance Office and by the Office of &lt;/p&gt;&lt;/div&gt;</description><author>cord</author><pubDate>Tue, 30 Jun 2009 16:06:23 GMT</pubDate><guid>http://www.docstoc.com/docs/7982432/Optical-reflection-and-transmission-formulae-for-thin-films</guid></item><item><title>Optical reflection and transmission formulae for thin films</title><link>http://www.docstoc.com/docs/7982420/Optical-reflection-and-transmission-formulae-for-thin-films</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/7982420/Optical-reflection-and-transmission-formulae-for-thin-films title="Optical reflection and transmission formulae for thin films"&lt;img src="http://img.docstoc.com/thumb/100/7982420.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/cord"&gt;cord&lt;/a&gt; on: Tuesday, June 30, 2009&lt;p&gt;BRIT. J. APPL. PHYS. (J. PHYS. D , 1968, SER. )2, VOL. 1.PRINTED IN GREAT BRITAINOptical reflection and transmission formulae for thzn filmsS . G. TOMLINDepartment of Physics, University of Adelaide, AustraliaMS. received 13th May 1968Abstract. The very complicated formulae which relate the components of the complex refractive&lt;/p&gt;&lt;/div&gt;</description><author>cord</author><pubDate>Tue, 30 Jun 2009 16:05:15 GMT</pubDate><guid>http://www.docstoc.com/docs/7982420/Optical-reflection-and-transmission-formulae-for-thin-films</guid></item><item><title>Gas discharge plasmas and their applications</title><link>http://www.docstoc.com/docs/7982408/Gas-discharge-plasmas-and-their-applications</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/7982408/Gas-discharge-plasmas-and-their-applications title="Gas discharge plasmas and their applications"&lt;img src="http://img.docstoc.com/thumb/100/7982408.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/cord"&gt;cord&lt;/a&gt; on: Tuesday, June 30, 2009&lt;p&gt;Spectrochimica Acta Part B 57 (2002) 609–658ReviewGas discharge plasmas and their applicationsAnnemie Bogaertsa,*, Erik Neytsa, Renaat Gijbelsa, Joost van der MullenbbUniversity of Antwerp, Department of Chemistry, Universiteitsplein 1, B-2610 Wilrijk-Antwerp, Belgium Eindhoven University of Technology, Department of Applied Physics&lt;/p&gt;&lt;/div&gt;</description><author>cord</author><pubDate>Tue, 30 Jun 2009 16:04:15 GMT</pubDate><guid>http://www.docstoc.com/docs/7982408/Gas-discharge-plasmas-and-their-applications</guid></item><item><title>Chemical Vapor Deposition (CVD)</title><link>http://www.docstoc.com/docs/7982351/Chemical-Vapor-Deposition-(CVD)</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/7982351/Chemical-Vapor-Deposition-(CVD) title="Chemical Vapor Deposition (CVD)"&lt;img src="http://img.docstoc.com/thumb/100/7982351.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/cord"&gt;cord&lt;/a&gt; on: Tuesday, June 30, 2009&lt;p&gt;Chemical Vapor Deposition (CVD)Processes: gift of SiO2 - Expose Si to steam =&gt; uniform insulating layer… or metal film growth : … Contrast with high vacuum, single element… toxic, corrosive gas flowing through valves,CVD:T up to 1000C, multiple simultaneous reactions, gas dynamics, dead layers… whose idea was it?All layers above poly&lt;/p&gt;&lt;/div&gt;</description><author>cord</author><pubDate>Tue, 30 Jun 2009 16:01:28 GMT</pubDate><guid>http://www.docstoc.com/docs/7982351/Chemical-Vapor-Deposition-(CVD)</guid></item><item><title>Design Rules for Ultra High Efficiency Solar Cells</title><link>http://www.docstoc.com/docs/7982333/Design-Rules-for-Ultra-High-Efficiency-Solar-Cells</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/7982333/Design-Rules-for-Ultra-High-Efficiency-Solar-Cells title="Design Rules for Ultra High Efficiency Solar Cells"&lt;img src="http://img.docstoc.com/thumb/100/7982333.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/cord"&gt;cord&lt;/a&gt; on: Tuesday, June 30, 2009&lt;p&gt;Design Rules for Ultra High Efficiency Solar CellsAllen Barnett and Christiana Honsberg Electrical and Computer Engineering University of Delaware Newark, Delaware 19716, USA abarnett@udel.edu,Abstract: Significant attention has focused on thermodynamic approaches to reaching the efficiency limits of photovoltaic solar cells. Many of these ap&lt;/p&gt;&lt;/div&gt;</description><author>cord</author><pubDate>Tue, 30 Jun 2009 16:00:31 GMT</pubDate><guid>http://www.docstoc.com/docs/7982333/Design-Rules-for-Ultra-High-Efficiency-Solar-Cells</guid></item><item><title>Physics Formulas</title><link>http://www.docstoc.com/docs/7897158/Physics-Formulas</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/7897158/Physics-Formulas title="Physics Formulas"&lt;img src="http://img.docstoc.com/thumb/100/7897158.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Coda"&gt;Coda&lt;/a&gt; on: Sunday, June 28, 2009&lt;p&gt;A complete collection of physics formulas useful for every graduate and undergraduate student and beyond. See also "Physics Formulas".&lt;/p&gt;&lt;/div&gt;</description><author>Coda</author><pubDate>Sun, 28 Jun 2009 14:28:04 GMT</pubDate><guid>http://www.docstoc.com/docs/7897158/Physics-Formulas</guid></item><item><title>Mathematics Formulas</title><link>http://www.docstoc.com/docs/7897142/Mathematics-Formulas</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/7897142/Mathematics-Formulas title="Mathematics Formulas"&lt;img src="http://img.docstoc.com/thumb/100/7897142.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Coda"&gt;Coda&lt;/a&gt; on: Sunday, June 28, 2009&lt;p&gt;A complete collection of mathematical formulas useful for every graduate and undergraduate student in mathematics and beyond. See also "Physics Formulas"&lt;/p&gt;&lt;/div&gt;</description><author>Coda</author><pubDate>Sun, 28 Jun 2009 14:27:16 GMT</pubDate><guid>http://www.docstoc.com/docs/7897142/Mathematics-Formulas</guid></item><item><title>Getaran Atom</title><link>http://www.docstoc.com/docs/7875211/Getaran-Atom</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/7875211/Getaran-Atom title="Getaran Atom"&lt;img src="http://img.docstoc.com/thumb/100/7875211.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Saturday, June 27, 2009&lt;p&gt;GETARAN ATOM Pada suhu 0K (-2730C), atom-atom tidak bergerak karena atom dalam keadaan energi terendah. Sedangkan bila suhu naik, energi akan meningkat sehingga atom-atom akan bergetar dengan jarak antar atom yang semakin besar pula.Ea=Jarak antar atom (a)Ea=Jarak antar atom (a)ET0 0 a’ET0 0 a’Energi dan pemuaian (a). &lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Sat, 27 Jun 2009 20:22:14 GMT</pubDate><guid>http://www.docstoc.com/docs/7875211/Getaran-Atom</guid></item><item><title>Bahan Ajar Material</title><link>http://www.docstoc.com/docs/7874933/Bahan-Ajar-Material</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/7874933/Bahan-Ajar-Material title="Bahan Ajar Material"&lt;img src="http://img.docstoc.com/thumb/100/7874933.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Saturday, June 27, 2009&lt;p&gt;LOGAM FASA TUNGGALLogam merupakan bahan yang lebih sederhana bila dibandingkan dengan dua kelompok bahan utama lainnya (polimer dan keramik). Hal ini dikarenakan logam pada umumnya hanya terdiri dari satu jenis atom (atau merupakan larutan padat seperti kuningan dimana seng menggantikan tembaga tanpa adanya perubahan struktur).Bagaimana hub&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Sat, 27 Jun 2009 20:18:05 GMT</pubDate><guid>http://www.docstoc.com/docs/7874933/Bahan-Ajar-Material</guid></item><item><title>Sensor Tranducer</title><link>http://www.docstoc.com/docs/7874111/Sensor-Tranducer</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/7874111/Sensor-Tranducer title="Sensor Tranducer"&lt;img src="http://img.docstoc.com/thumb/100/7874111.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/hsg029"&gt;hsg029&lt;/a&gt; on: Saturday, June 27, 2009&lt;p&gt;Bab 1 Sensor dan TransduserTujuan Pembelajaran Umum Setelah mempelajari bab ini diharapkan mahasiswa memahami pengertian sensor dan transduser dan penggunaannya dalam sistem kendali.Tujuan Pembelajaran Khusus Setelah mempelajari topik per topik dalam bab ini, mahasiswa diharapkan :  Dapat menyebutkan definisi dan perbedaan dari sensor, trans&lt;/p&gt;&lt;/div&gt;</description><author>hsg029</author><pubDate>Sat, 27 Jun 2009 19:59:34 GMT</pubDate><guid>http://www.docstoc.com/docs/7874111/Sensor-Tranducer</guid></item><item><title>Centrfugation</title><link>http://www.docstoc.com/docs/6079531/Centrfugation</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/6079531/Centrfugation title="Centrfugation"&lt;img src="http://img.docstoc.com/thumb/100/6079531.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/mail2preji"&gt;mail2preji&lt;/a&gt; on: Tuesday, May 19, 2009&lt;p&gt;No description&lt;/p&gt;&lt;/div&gt;</description><author>mail2preji</author><pubDate>Tue, 19 May 2009 10:43:58 GMT</pubDate><guid>http://www.docstoc.com/docs/6079531/Centrfugation</guid></item><item><title>sushil kumar's paper abstract</title><link>http://www.docstoc.com/docs/5408192/sushil-kumars-paper-abstract</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/5408192/sushil-kumars-paper-abstract title="sushil kumar's paper abstract"&lt;img src="http://img.docstoc.com/thumb/100/5408192.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/sushilk17"&gt;sushilk17&lt;/a&gt; on: Tuesday, April 14, 2009&lt;p&gt;Here I have add abstract of my papers.&lt;/p&gt;&lt;/div&gt;</description><author>sushilk17</author><pubDate>Tue, 14 Apr 2009 09:18:44 GMT</pubDate><guid>http://www.docstoc.com/docs/5408192/sushil-kumars-paper-abstract</guid></item><item><title>Contribucin del momento magntico a la fuerza de reaccin a la radiacin en forma relativista</title><link>http://www.docstoc.com/docs/4578883/Contribucin-del-momento-magntico-a-la-fuerza-de-reaccin-a-la-radiacin-en-forma-relativista</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/4578883/Contribucin-del-momento-magntico-a-la-fuerza-de-reaccin-a-la-radiacin-en-forma-relativista title="Contribucin del momento magntico a la fuerza de reaccin a la radiacin en forma relativista"&lt;img src="http://img.docstoc.com/thumb/100/4578883.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/iiarocci"&gt;iiarocci&lt;/a&gt; on: Friday, February 27, 2009&lt;p&gt;No description&lt;/p&gt;&lt;/div&gt;</description><author>iiarocci</author><pubDate>Fri, 27 Feb 2009 12:23:04 GMT</pubDate><guid>http://www.docstoc.com/docs/4578883/Contribucin-del-momento-magntico-a-la-fuerza-de-reaccin-a-la-radiacin-en-forma-relativista</guid></item><item><title>Photonics</title><link>http://www.docstoc.com/docs/2845368/Photonics</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/2845368/Photonics title="Photonics"&lt;img src="http://img.docstoc.com/thumb/100/2845368.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/iyangfenny"&gt;iyangfenny&lt;/a&gt; on: Wednesday, December 03, 2008&lt;p&gt;Fotonica PhotonicsRoel BaetsCursus voor de derde bachelor ingenieurswetenschappen: elektrotechniek en de derde bachelor ingenieurswetenschappen: toegepaste natuurkundeCourse for the Erasmus Mundus Master of Science in PhotonicsAcademiejaar 2007-2008 Universiteit Gent Vakgroep Informatietechnologie Faculteit IngenieurswetenschappenAc&lt;/p&gt;&lt;/div&gt;</description><author>iyangfenny</author><pubDate>Wed, 03 Dec 2008 03:27:56 GMT</pubDate><guid>http://www.docstoc.com/docs/2845368/Photonics</guid></item><item><title>TEORIA SOBRE LOS VECTORES</title><link>http://www.docstoc.com/docs/2451808/TEORIA-SOBRE-LOS-VECTORES</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/2451808/TEORIA-SOBRE-LOS-VECTORES title="TEORIA SOBRE LOS VECTORES"&lt;img src="http://img.docstoc.com/thumb/100/2451808.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/ELEKID"&gt;ELEKID&lt;/a&gt; on: Friday, November 07, 2008&lt;p&gt;No description&lt;/p&gt;&lt;/div&gt;</description><author>ELEKID</author><pubDate>Fri, 07 Nov 2008 10:35:15 GMT</pubDate><guid>http://www.docstoc.com/docs/2451808/TEORIA-SOBRE-LOS-VECTORES</guid></item><item><title>probsheet1_solns</title><link>http://www.docstoc.com/docs/2128111/probsheet1_solns</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/2128111/probsheet1_solns title="probsheet1_solns"&lt;img src="http://img.docstoc.com/thumb/100/2128111.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/charlyking"&gt;charlyking&lt;/a&gt; on: Tuesday, October 28, 2008&lt;p&gt;No description&lt;/p&gt;&lt;/div&gt;</description><author>charlyking</author><pubDate>Tue, 28 Oct 2008 14:28:26 GMT</pubDate><guid>http://www.docstoc.com/docs/2128111/probsheet1_solns</guid></item><item><title>probsheet2</title><link>http://www.docstoc.com/docs/2128112/probsheet2</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/2128112/probsheet2 title="probsheet2"&lt;img src="http://img.docstoc.com/thumb/100/2128112.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/charlyking"&gt;charlyking&lt;/a&gt; on: Tuesday, October 28, 2008&lt;p&gt;No description&lt;/p&gt;&lt;/div&gt;</description><author>charlyking</author><pubDate>Tue, 28 Oct 2008 14:28:26 GMT</pubDate><guid>http://www.docstoc.com/docs/2128112/probsheet2</guid></item><item><title>probsheet2_solns</title><link>http://www.docstoc.com/docs/2128113/probsheet2_solns</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/2128113/probsheet2_solns title="probsheet2_solns"&lt;img src="http://img.docstoc.com/thumb/100/2128113.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/charlyking"&gt;charlyking&lt;/a&gt; on: Tuesday, October 28, 2008&lt;p&gt;No description&lt;/p&gt;&lt;/div&gt;</description><author>charlyking</author><pubDate>Tue, 28 Oct 2008 14:28:26 GMT</pubDate><guid>http://www.docstoc.com/docs/2128113/probsheet2_solns</guid></item><item><title>probsheet3</title><link>http://www.docstoc.com/docs/2128114/probsheet3</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/2128114/probsheet3 title="probsheet3"&lt;img src="http://img.docstoc.com/thumb/100/2128114.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/charlyking"&gt;charlyking&lt;/a&gt; on: Tuesday, October 28, 2008&lt;p&gt;No description&lt;/p&gt;&lt;/div&gt;</description><author>charlyking</author><pubDate>Tue, 28 Oct 2008 14:28:26 GMT</pubDate><guid>http://www.docstoc.com/docs/2128114/probsheet3</guid></item><item><title>probsheet3_solns</title><link>http://www.docstoc.com/docs/2128115/probsheet3_solns</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/2128115/probsheet3_solns title="probsheet3_solns"&lt;img src="http://img.docstoc.com/thumb/100/2128115.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/charlyking"&gt;charlyking&lt;/a&gt; on: Tuesday, October 28, 2008&lt;p&gt;No description&lt;/p&gt;&lt;/div&gt;</description><author>charlyking</author><pubDate>Tue, 28 Oct 2008 14:28:26 GMT</pubDate><guid>http://www.docstoc.com/docs/2128115/probsheet3_solns</guid></item><item><title>probsheet1</title><link>http://www.docstoc.com/docs/2128110/probsheet1</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/2128110/probsheet1 title="probsheet1"&lt;img src="http://img.docstoc.com/thumb/100/2128110.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/charlyking"&gt;charlyking&lt;/a&gt; on: Tuesday, October 28, 2008&lt;p&gt;No description&lt;/p&gt;&lt;/div&gt;</description><author>charlyking</author><pubDate>Tue, 28 Oct 2008 14:28:25 GMT</pubDate><guid>http://www.docstoc.com/docs/2128110/probsheet1</guid></item><item><title>ESA’S SMART-1 MISSION AT THE MOON: FIRST RESULTS, STATUS AND NEXT STEPS</title><link>http://www.docstoc.com/docs/1044288/ESA’S-SMART-1-MISSION-AT-THE-MOON-FIRST-RESULTS-STATUS-AND-NEXT-STEPS</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044288/ESA’S-SMART-1-MISSION-AT-THE-MOON-FIRST-RESULTS-STATUS-AND-NEXT-STEPS title="ESA’S SMART-1 MISSION AT THE MOON: FIRST RESULTS, STATUS AND NEXT STEPS"&lt;img src="http://img.docstoc.com/thumb/100/1044288.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Foing, Racca, Grande, Huovelin, Josset, Keller, Nathues, Malkki, Heather, Koschny, Almeida, Frew, Lumb, Volp, Zender (SMART-1 Science &amp; Technology Working Team), SMART-1 Project ESTEC/SCI-PD, Noordwijk, Nederland - SMART-1 is the first in the program of ESA’s Small Missions for Advanced Research and Technology. Its first objective has been achieved to demonstrate Solar Electric Primary Propulsion (SEP) for future Cornerstones (such as Bepi-Colombo) and to test new technologies for spacecraft and instruments. The spacecraft has been launched on 27 Sept. 2003, as an Ariane-5 auxiliary passenger and injected in GTO Geostationary Tranfer Orbit. Thanks to the successful electric propulsion navigation, the spacecraft has left the inner radiation belts in early 2004, and reached lunar capture on 17 November 2004.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:07:00 GMT</pubDate><guid>http://www.docstoc.com/docs/1044288/ESA’S-SMART-1-MISSION-AT-THE-MOON-FIRST-RESULTS-STATUS-AND-NEXT-STEPS</guid></item><item><title>TIDAL FORCES AS DRIVERS OF COLLISIONAL EVOLUTION</title><link>http://www.docstoc.com/docs/1044287/TIDAL-FORCES-AS-DRIVERS-OF-COLLISIONAL-EVOLUTION</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044287/TIDAL-FORCES-AS-DRIVERS-OF-COLLISIONAL-EVOLUTION title="TIDAL FORCES AS DRIVERS OF COLLISIONAL EVOLUTION"&lt;img src="http://img.docstoc.com/thumb/100/1044287.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;E. Asphaug, C. Agnor and Q. Williams, Center for Origin, Dynamics &amp; Evolution of Planets, Earth Sciences Dept. University of California, Santa Cruz - Impacts, Shocks &amp; Tides: Planetary collisions are usually understood as shock-related phenomena, analogous to impact cratering. But at large scales, where the impact timescale is comparable to the gravitational timescale, collisions can be dominated by gravitational torques and disruptive tides.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:06:57 GMT</pubDate><guid>http://www.docstoc.com/docs/1044287/TIDAL-FORCES-AS-DRIVERS-OF-COLLISIONAL-EVOLUTION</guid></item><item><title>Sulfur multiple isotopes of the Moon: 33S and 36S abundances relative to Canon Diablo Troilite.</title><link>http://www.docstoc.com/docs/1044286/Sulfur-multiple-isotopes-of-the-Moon-33S-and-36S-abundances-relative-to-Canon-Diablo-Troilite</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044286/Sulfur-multiple-isotopes-of-the-Moon-33S-and-36S-abundances-relative-to-Canon-Diablo-Troilite title="Sulfur multiple isotopes of the Moon: 33S and 36S abundances relative to Canon Diablo Troilite."&lt;img src="http://img.docstoc.com/thumb/100/1044286.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Farquhar and Wing, Earth System Science Interdisciplinary Center and Department of Geology, University of Maryland, College Park.We are measuring sulfur multiple iso-tope abundances in 10 lunar basalts, a suite of terrestrial igneous rocks, and samples of Canon Diablo Troilite (CDT). Ongoing measurements suggest that the acid volatile sulfur (AVS) in lunar basalts is only slightly enriched in 34S relative to CDT, confirming earlier results. High-precision sulfur multiple isotope measurements also indicate that lunar AVS falls on a fractionation line defined by the bulk com-position of CDT and a slope of 0.515.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:06:29 GMT</pubDate><guid>http://www.docstoc.com/docs/1044286/Sulfur-multiple-isotopes-of-the-Moon-33S-and-36S-abundances-relative-to-Canon-Diablo-Troilite</guid></item><item><title>COMPARISION OF NEWLY ACQUIRED LUNAR SPECTRA WITH THE TITANIUM ABUNDANCE MAPS DERIVED FROM CLEMENTINE</title><link>http://www.docstoc.com/docs/1044285/COMPARISION-OF-NEWLY-ACQUIRED-LUNAR-SPECTRA-WITH-THE-TITANIUM-ABUNDANCE-MAPS-DERIVED-FROM-CLEMENTINE</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044285/COMPARISION-OF-NEWLY-ACQUIRED-LUNAR-SPECTRA-WITH-THE-TITANIUM-ABUNDANCE-MAPS-DERIVED-FROM-CLEMENTINE title="COMPARISION OF NEWLY ACQUIRED LUNAR SPECTRA WITH THE TITANIUM ABUNDANCE MAPS DERIVED FROM CLEMENTINE"&lt;img src="http://img.docstoc.com/thumb/100/1044285.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Holsclaw, McClintock, Robinson, Laboratory for Atmospheric and Space Physics, Boulder, CO, Northwestern University, Evanston .The Mercury Atmospheric and Surface Composition Spectrometer (MASCS) is one of seven science instruments onboard NASA’s MESSENGER mission, currently en-route to the planet Mercury. One of MASCS’s components, referred to as the Visible and Near Infrared Spectrograph (VIRS), will record reflectance spectra of the surface in order to characterize the mineralogy of the planet. The lunar highlands and the average mercurian crust are proposed to be compositionally similar. In preparation to interpret VIRS reflectance spectra of Mercury to be first obtained in 2008, the Moon has been observed with an engineering model of the VIRS from a ground-based telescope. In this study, the ultraviolet and visible region of the spectrum is compared with titanium content in the lunar regolith.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:06:22 GMT</pubDate><guid>http://www.docstoc.com/docs/1044285/COMPARISION-OF-NEWLY-ACQUIRED-LUNAR-SPECTRA-WITH-THE-TITANIUM-ABUNDANCE-MAPS-DERIVED-FROM-CLEMENTINE</guid></item><item><title>USING MODELS OF PERMANENT SHADOW TO CONSTRAIN LUNAR POLAR WATER ICE ABUNDANCES</title><link>http://www.docstoc.com/docs/1044284/USING-MODELS-OF-PERMANENT-SHADOW-TO-CONSTRAIN-LUNAR-POLAR-WATER-ICE-ABUNDANCES</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044284/USING-MODELS-OF-PERMANENT-SHADOW-TO-CONSTRAIN-LUNAR-POLAR-WATER-ICE-ABUNDANCES title="USING MODELS OF PERMANENT SHADOW TO CONSTRAIN LUNAR POLAR WATER ICE ABUNDANCES"&lt;img src="http://img.docstoc.com/thumb/100/1044284.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Elphic, Lawrence, Feldman, Prettyman, Maurice, Bussey, Spudis and Lucey, Space and Atmospheric Sciences, Los Alamos National Laboratory &amp; 2Centre d'Etude Spatiale des Rayonnements (CESR),Toulouse, France, Johns Hopkins Applied Physics Laboratory, Laurel, MD, Hawai’i Institute of Geophysics and Planetology, University of Hawai’i, Honolulu. - Introduction: Reservoirs of volatiles cold-trapped in permanent shadow at the lunar poles are scientifically valuable and a potential in situ resource for exploration.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:05:27 GMT</pubDate><guid>http://www.docstoc.com/docs/1044284/USING-MODELS-OF-PERMANENT-SHADOW-TO-CONSTRAIN-LUNAR-POLAR-WATER-ICE-ABUNDANCES</guid></item><item><title>SPACE WEATHERING AND THERMAL PROPERIES OF FRESH CRATERS ON THE MOON</title><link>http://www.docstoc.com/docs/1044283/SPACE-WEATHERING-AND-THERMAL-PROPERIES-OF-FRESH-CRATERS-ON-THE-MOON</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044283/SPACE-WEATHERING-AND-THERMAL-PROPERIES-OF-FRESH-CRATERS-ON-THE-MOON title="SPACE WEATHERING AND THERMAL PROPERIES OF FRESH CRATERS ON THE MOON"&lt;img src="http://img.docstoc.com/thumb/100/1044283.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;B. B. Wilcox, P. G. Lucey and J. T. Cahill, Hawaii Institute of Geophysics and Planetology, University of Hawaii. - Space weathering processes on the Moon control the production of the regolith and the alteration of its optical properties. Larger impacts produce new regolith from bedrock and smaller impacts work to comminute it to finer particle sizes. Solar wind sputtering and micrometeorite impact vaporization combine to cause regolith spectra to both redden and darken. Two data sets exist that are sensitive to these two processes. Thermal images of the Moon, taken during eclipse, are sensitive to the particle size distribution of the surface (the amount of rocks). Optical Maturity (OMAT) parameter images, on the other hand, are sensitive to the amount of agglutinates and nanophase iron produced as a result of surface exposure to space weathering processes. Analysis of these images offer new insights into the state of the lunar regolith and its evolution.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:04:59 GMT</pubDate><guid>http://www.docstoc.com/docs/1044283/SPACE-WEATHERING-AND-THERMAL-PROPERIES-OF-FRESH-CRATERS-ON-THE-MOON</guid></item><item><title>CRATER VARIETY WITH AND WITHOUT VOLCANIC ROCKS BETWEEN THE MOON AND EARTH</title><link>http://www.docstoc.com/docs/1044282/CRATER-VARIETY-WITH-AND-WITHOUT-VOLCANIC-ROCKS-BETWEEN-THE-MOON-AND-EARTH</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044282/CRATER-VARIETY-WITH-AND-WITHOUT-VOLCANIC-ROCKS-BETWEEN-THE-MOON-AND-EARTH title="CRATER VARIETY WITH AND WITHOUT VOLCANIC ROCKS BETWEEN THE MOON AND EARTH"&lt;img src="http://img.docstoc.com/thumb/100/1044282.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Miura, Dept. Earth Sci., Fac. Sci., Yamaguchi University, Yamaguchi, Japan. - Impact crater on the Moon is defined by typical impact process on the highland. Mare basalt is filled to wide impact crater structure only front side of the Moon, mainly by large impact or tidal forces from Earth. The main purpose of this paper is 1) to elucidate large lunar craters with volcanic rocks compared with terrestrial crater, 2) to classify craters with volacin rocks on Earth.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:04:45 GMT</pubDate><guid>http://www.docstoc.com/docs/1044282/CRATER-VARIETY-WITH-AND-WITHOUT-VOLCANIC-ROCKS-BETWEEN-THE-MOON-AND-EARTH</guid></item><item><title>IMPACT OF LUNAR DUST ON THE EXPLORATION INITIATIVE</title><link>http://www.docstoc.com/docs/1044281/IMPACT-OF-LUNAR-DUST-ON-THE-EXPLORATION-INITIATIVE</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044281/IMPACT-OF-LUNAR-DUST-ON-THE-EXPLORATION-INITIATIVE title="IMPACT OF LUNAR DUST ON THE EXPLORATION INITIATIVE"&lt;img src="http://img.docstoc.com/thumb/100/1044281.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Stubbs, Vondrak and Farrell, NASA Goddard, Greenbelt. - From the Apollo era it is known that dust on the Moon can cause serious problems for exploration activities. Such problems include adhering to clothing and equipment, reducing external visibility on landings, and causing difficulty to breathing and vision within the spacecraft. An important step in dealing with dust-related problems is to understand how dust grains behave in the lunar environment. Past Experiences. All astronauts who walked on the Moon reported difficulties with lunar dust. Eugene Cernan, commander of Apollo 17, stated that “… one of the most aggravating, restricting facets of lunar surface exploration is the dust and its adherence to everything no matter what kind of material, whether it be skin, suit material, metal, no matter what it be and it’s restrictive friction-like action to everything it gets on." Highest Future Priority. Dust has also been highlighted as a priority by the Mars Exploration Program Assessment Group (MEPAG): “1A. Characterize both aeolian dust and particulates that woould be kicked up from the martian regolith by surface operations of a human mission with fidelity sufficient to establish credible engineering simulation labs and/or software codes on Earth.” We shall briefly describe the properties of lunar dust and its impact on the Apollo astronauts, and then summarize three main problems areas for understanding its behavior: Dust Adhesion and Abrasion, Surface Electric Fields and Dust Transport. These issues are all inter-related and must be well understood in order to minimize the impact of dust on lunar surface exploration.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:04:40 GMT</pubDate><guid>http://www.docstoc.com/docs/1044281/IMPACT-OF-LUNAR-DUST-ON-THE-EXPLORATION-INITIATIVE</guid></item><item><title>DISTINGUISHING HIGH-AL MARE BASALT UNITS USING HIGH RESOLUTION CLEMENTINE DATA</title><link>http://www.docstoc.com/docs/1044280/DISTINGUISHING-HIGH-AL-MARE-BASALT-UNITS-USING-HIGH-RESOLUTION-CLEMENTINE-DATA</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044280/DISTINGUISHING-HIGH-AL-MARE-BASALT-UNITS-USING-HIGH-RESOLUTION-CLEMENTINE-DATA title="DISTINGUISHING HIGH-AL MARE BASALT UNITS USING HIGH RESOLUTION CLEMENTINE DATA"&lt;img src="http://img.docstoc.com/thumb/100/1044280.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Kramer, Jolliff, Neal, Kirkland and Fessler University of Notre Dame, Department of Civil Engineering and Geological Sciences &amp; Washington University, Department of Earth and Planetary Sciences; Lunar and Planetary Institute, Houston. - Some of the (Apollo 14) high-Al basalts are old (&gt;4 Ga), and the sample data suggests there are at least three and possibly five distinct sources and episodes of volcanism represented at the Apollo 14 site alone. Exposures of these basalts near the Apollo 14 are likely masked by ejecta from the Imbrium impact, which is responsible for the formation of the Apollo 14 breccias and post-dates eruption of the basalts. This suggests that they could be a significant component of ancient basalts that are now buried beneath impact deposits (cryptomare). The existence of younger aluminous basalts at the Apollo 12 and Luna 16 sites suggest that aluminous basaltic volcanism spanned over a billion years. The high-Al nature of these basalts suggests they are derived from a relatively Al-rich source. This Al probably comes from the presence of plagioclase in the source, which implies that plagioclase flotation was inefficient in the Lunar Magma Ocean (LMO) and that some remains within the uppermost lunar mantle. Identifying high-Al basalt exposures is necessary for locating potential future sampling sites as they may represent outcrops of pre-4 Ga volcanism and be a window to early processes.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:04:36 GMT</pubDate><guid>http://www.docstoc.com/docs/1044280/DISTINGUISHING-HIGH-AL-MARE-BASALT-UNITS-USING-HIGH-RESOLUTION-CLEMENTINE-DATA</guid></item><item><title>Dunite Dikes In The Lunar Mantle?</title><link>http://www.docstoc.com/docs/1044278/Dunite-Dikes-In-The-Lunar-Mantle</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044278/Dunite-Dikes-In-The-Lunar-Mantle title="Dunite Dikes In The Lunar Mantle?"&lt;img src="http://img.docstoc.com/thumb/100/1044278.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Beck, Morgan, Liang and P. Hess; Brown University, Providence. - Experimentally determined multisaturation depths for the lunar picritic glasses suggest that the source region for the glasses is very deep, on the order of 500 km for the Apollo 14 picritic green glasses and the Apollo 15 picritic red glasses. These depths are believed to be a minimum estimate because the glasses have all experienced near surface fractionation of olivine. If multisaturation truly represents a minimum or even average depth of melting, it is very important to understand the extent to which the glasses have reacted with the lunar mantle during their long ascent to the surface.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:04:07 GMT</pubDate><guid>http://www.docstoc.com/docs/1044278/Dunite-Dikes-In-The-Lunar-Mantle</guid></item><item><title>MAGNESIUM ISOTOPES IN LUNAR ROCKS AND GLASSES AND IMPLICATIONS FOR ORIGIN OF THE MOON</title><link>http://www.docstoc.com/docs/1044276/MAGNESIUM-ISOTOPES-IN-LUNAR-ROCKS-AND-GLASSES-AND-IMPLICATIONS-FOR-ORIGIN-OF-THE-MOON</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044276/MAGNESIUM-ISOTOPES-IN-LUNAR-ROCKS-AND-GLASSES-AND-IMPLICATIONS-FOR-ORIGIN-OF-THE-MOON title="MAGNESIUM ISOTOPES IN LUNAR ROCKS AND GLASSES AND IMPLICATIONS FOR ORIGIN OF THE MOON"&lt;img src="http://img.docstoc.com/thumb/100/1044276.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Paul H. Warren, Eric Tonui and Edward D. Young, Institute of Geophysics, UCLA, Los Angeles. - Volatile depletion was a ubiquitous concomitant of planet formation, especially in the inner solar system. Isotopic variations of Mg, a major element with three stable isotopes, can potentially provide insight into this important aspect of planetary origin.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:03:45 GMT</pubDate><guid>http://www.docstoc.com/docs/1044276/MAGNESIUM-ISOTOPES-IN-LUNAR-ROCKS-AND-GLASSES-AND-IMPLICATIONS-FOR-ORIGIN-OF-THE-MOON</guid></item><item><title>UNIFIED LUNAR CONTROL NETWORK 2005 AND TOPOGRAPHIC MODEL</title><link>http://www.docstoc.com/docs/1044275/UNIFIED-LUNAR-CONTROL-NETWORK-2005-AND-TOPOGRAPHIC-MODEL</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044275/UNIFIED-LUNAR-CONTROL-NETWORK-2005-AND-TOPOGRAPHIC-MODEL title="UNIFIED LUNAR CONTROL NETWORK 2005 AND TOPOGRAPHIC MODEL"&lt;img src="http://img.docstoc.com/thumb/100/1044275.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Archinal, Rosiek and Redding, U. S. Geological Survey, Flagstaff. There are currently two generally accepted lunar control networks. These are the Unified Lunar Control Network (ULCN) and the Clementine Lunar Control Network (CLCN), both derived by M. Davies and T. Colvin at RAND. We address here our efforts to merge and improve these networks into a new ULCN.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:03:30 GMT</pubDate><guid>http://www.docstoc.com/docs/1044275/UNIFIED-LUNAR-CONTROL-NETWORK-2005-AND-TOPOGRAPHIC-MODEL</guid></item><item><title>Global Mapping of elemental abundance on lunar surface by SELENE gamma-ray spectrometer</title><link>http://www.docstoc.com/docs/1044274/Global-Mapping-of-elemental-abundance-on-lunar-surface-by-SELENE-gamma-ray-spectrometer</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044274/Global-Mapping-of-elemental-abundance-on-lunar-surface-by-SELENE-gamma-ray-spectrometer title="Global Mapping of elemental abundance on lunar surface by SELENE gamma-ray spectrometer"&lt;img src="http://img.docstoc.com/thumb/100/1044274.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Kobayashi, Berezhnoy, d’Uston, Fujii, Hasebe, Hiroishi, Kaneko, Miyachi, Mori, Maurice, Nakazawa, Narasaki, Okudaira, Shibamura, Takashima, Yamashita; Advanced Research Institute of Sci.&amp; Eng., Waseda Univ. Tokyo; Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Kanagawa, Niihama Works, Sumitomo Heavy Industry Ltd., Niihama, Ehime, Moriya Works, Meisei Electric Co., Ltd., Clear Pulse Co., Tokyo, Japan &amp; Centre d’Etude Spatiale des Rayonnements, CNRS/UPS, Colonel Roche, France. - Elemental composition on the surface of a planet is very important information for solving the origin and the evolution of the planet and also very necessary for understanding the origin and the evolution of solar system. Planetary gamma-ray spectroscopy is extremely powerful approach for the elemental composition measurement. Gamma-ray spectrometer (GRS) will be on board SELENE (Kayuga), advanced lunar polar orbiter, and employ a large-volume Ge detector of 252cc as the main detector. SELENE (Kayuga) GRS is, therefore, approximately twice more sensitivity than Lunar Prospector GRS, four times more sensitive than APOLLO GRS. The high sensitivity of SELENE GRS will enable us to map element abundances of O, Mg, Fe, Al, Si, Ti, K, Ca, Th, and U, with lower detection limit than the past missions. The Japanese lunar polar orbiter SELENE is scheduled for launch in 2007 and the GRS will observe the whole area of the moon including the polar region.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:03:03 GMT</pubDate><guid>http://www.docstoc.com/docs/1044274/Global-Mapping-of-elemental-abundance-on-lunar-surface-by-SELENE-gamma-ray-spectrometer</guid></item><item><title>A COMPARISON OF IMPACT-RELATED DEPOSITS SURROUNDING CRATERS ON THE MOON, VENUS, AND MARS</title><link>http://www.docstoc.com/docs/1044273/A-COMPARISON-OF-IMPACT-RELATED-DEPOSITS-SURROUNDING-CRATERS-ON-THE-MOON-VENUS-AND-MARS</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044273/A-COMPARISON-OF-IMPACT-RELATED-DEPOSITS-SURROUNDING-CRATERS-ON-THE-MOON-VENUS-AND-MARS title="A COMPARISON OF IMPACT-RELATED DEPOSITS SURROUNDING CRATERS ON THE MOON, VENUS, AND MARS"&lt;img src="http://img.docstoc.com/thumb/100/1044273.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Ghent, Carter, Leverington and Campbell, Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington.  The goal of this work is to explore the distribution and properties of surficial impactrelated deposits on the Moon, Mars, and Venus.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:02:55 GMT</pubDate><guid>http://www.docstoc.com/docs/1044273/A-COMPARISON-OF-IMPACT-RELATED-DEPOSITS-SURROUNDING-CRATERS-ON-THE-MOON-VENUS-AND-MARS</guid></item><item><title>ISOTOPIC COMPOSTION OF LUNAR SOILS AND THE EARLY DIFFERENTIATION OF THE MOON</title><link>http://www.docstoc.com/docs/1044271/ISOTOPIC-COMPOSTION-OF-LUNAR-SOILS-AND-THE-EARLY-DIFFERENTIATION-OF-THE-MOON</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044271/ISOTOPIC-COMPOSTION-OF-LUNAR-SOILS-AND-THE-EARLY-DIFFERENTIATION-OF-THE-MOON title="ISOTOPIC COMPOSTION OF LUNAR SOILS AND THE EARLY DIFFERENTIATION OF THE MOON"&lt;img src="http://img.docstoc.com/thumb/100/1044271.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Ranen and Jacobsen, Department of Earth and Planetary Sciences, Harvard University, Cambridge. - The isotopic composition of the Lunar Highlands crust is still not well defined. This study will measure Hf-W, Rb-Sr, Lu-Hf, and 147,146Sm- 143,142Nd on a suite of 14 lunar soils from the Apollo 14 and Apollo 16 missions. The overall goal of this project is to estimate the isotopic composition of the average lunar crust in order to constrain timescales and magnitude of magma ocean crystallization.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:01:56 GMT</pubDate><guid>http://www.docstoc.com/docs/1044271/ISOTOPIC-COMPOSTION-OF-LUNAR-SOILS-AND-THE-EARLY-DIFFERENTIATION-OF-THE-MOON</guid></item><item><title>LUNAR GEOLOGIC MAPPING: PRELIMINARY RESULTS FOR THE COPERNICUS QUAD</title><link>http://www.docstoc.com/docs/1044270/LUNAR-GEOLOGIC-MAPPING-PRELIMINARY-RESULTS-FOR-THE-COPERNICUS-QUAD</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044270/LUNAR-GEOLOGIC-MAPPING-PRELIMINARY-RESULTS-FOR-THE-COPERNICUS-QUAD title="LUNAR GEOLOGIC MAPPING: PRELIMINARY RESULTS FOR THE COPERNICUS QUAD"&lt;img src="http://img.docstoc.com/thumb/100/1044270.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Gaddis, Skinner, Hare1, Tanaka, Hawke, Spudis, Bussey, Pieters and Lawrence, U.S. Geological Survey, Astrogeology Program, Flagstaff, PGD/SOEST, Univ. Hawaii, Honolulu, HI; Johns Hopkins Univ., Baltimore, MD; Dept. Geological Sciences, Brown Univ., Providence; Los Alamos National Laboratory.  We describe prelimary 1:2.5 M scale geologic map results of the Copernicus quad as part of a new pilot program for systematic, global lunar geologic mapping. This program continues the systematic lunar geologic mapping efforts that ended almost 30 years ago during the Apollo era.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:01:52 GMT</pubDate><guid>http://www.docstoc.com/docs/1044270/LUNAR-GEOLOGIC-MAPPING-PRELIMINARY-RESULTS-FOR-THE-COPERNICUS-QUAD</guid></item><item><title>THE FIRST ISOTOPIC DATING OF THE DHOFAR 025 LUNAR METEORITE BY U-Pb METHOD USING ACCESSORY ZIRCON</title><link>http://www.docstoc.com/docs/1044269/THE-FIRST-ISOTOPIC-DATING-OF-THE-DHOFAR-025-LUNAR-METEORITE-BY-U-Pb-METHOD-USING-ACCESSORY-ZIRCON</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044269/THE-FIRST-ISOTOPIC-DATING-OF-THE-DHOFAR-025-LUNAR-METEORITE-BY-U-Pb-METHOD-USING-ACCESSORY-ZIRCON title="THE FIRST ISOTOPIC DATING OF THE DHOFAR 025 LUNAR METEORITE BY U-Pb METHOD USING ACCESSORY ZIRCON"&lt;img src="http://img.docstoc.com/thumb/100/1044269.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Leontieva, Matukov, Nazarov, Sergeev and Yu. Shukolyukov, Department of Geology, St-Petersburg State University; Center of Isotopic Research, All-Russian Geological Research Institute (VSEGEI), St-Petersburg, Vernandsky Institute of Geochemistry and Analytical Chemistry, Moscow, Institute of Geology and Geochronology of Precambrian, St-Petersburg, .At present there are more than 50 known lunar meteorites found all over the world – in Antarctica, Africa and Australia. Most of them are very well studied with different methods. The isotopic composition of noble gases, oxygen, strontium, lead, and other elements was reported in these meteorites.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:01:44 GMT</pubDate><guid>http://www.docstoc.com/docs/1044269/THE-FIRST-ISOTOPIC-DATING-OF-THE-DHOFAR-025-LUNAR-METEORITE-BY-U-Pb-METHOD-USING-ACCESSORY-ZIRCON</guid></item><item><title>ORDINARY CHONDRITE IMPACT ON THE MOON: RESULTS FROM THE 3.9 GA IMPACT MELT AT THE LANDING SITE OF APOLLO 17</title><link>http://www.docstoc.com/docs/1044268/ORDINARY-CHONDRITE-IMPACT-ON-THE-MOON-RESULTS-FROM-THE-39-GA-IMPACT-MELT-AT-THE-LANDING-SITE-OF-APOLLO-17</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044268/ORDINARY-CHONDRITE-IMPACT-ON-THE-MOON-RESULTS-FROM-THE-39-GA-IMPACT-MELT-AT-THE-LANDING-SITE-OF-APOLLO-17 title="ORDINARY CHONDRITE IMPACT ON THE MOON: RESULTS FROM THE 3.9 GA IMPACT MELT AT THE LANDING SITE OF APOLLO 17"&lt;img src="http://img.docstoc.com/thumb/100/1044268.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Roald Tagle, Inst. Mineralogy, Nat. History Museum, Berlin,  The Moon allows a view to the past of Earth, offering a unique opportunity to study the ancient impact history of our planet. Since the first impact melt (IM) samples were brought back by the Apollo missions, controversies existed regarding the ancient impact population and the projectile types involved in the late heavy bombardment.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:01:41 GMT</pubDate><guid>http://www.docstoc.com/docs/1044268/ORDINARY-CHONDRITE-IMPACT-ON-THE-MOON-RESULTS-FROM-THE-39-GA-IMPACT-MELT-AT-THE-LANDING-SITE-OF-APOLLO-17</guid></item><item><title>SECTRAL PHOTOMETRIC PROPERTIES OF THE MOON</title><link>http://www.docstoc.com/docs/1044266/SECTRAL-PHOTOMETRIC-PROPERTIES-OF-THE-MOON</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044266/SECTRAL-PHOTOMETRIC-PROPERTIES-OF-THE-MOON title="SECTRAL PHOTOMETRIC PROPERTIES OF THE MOON"&lt;img src="http://img.docstoc.com/thumb/100/1044266.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Domingue and Vilas, Johns Hopkins University Applied Physics Laboratory, Laurel, NASA JSC, Houston  We modeled the solar phase curves of the moon at a series of wavelengths using the full disk telescopic observations.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:01:25 GMT</pubDate><guid>http://www.docstoc.com/docs/1044266/SECTRAL-PHOTOMETRIC-PROPERTIES-OF-THE-MOON</guid></item><item><title>DIELECTRIC CONSTANT MEASUREMENTS FOR CHARACTERIZING LUNAR SOILS</title><link>http://www.docstoc.com/docs/1044265/DIELECTRIC-CONSTANT-MEASUREMENTS-FOR-CHARACTERIZING-LUNAR-SOILS</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044265/DIELECTRIC-CONSTANT-MEASUREMENTS-FOR-CHARACTERIZING-LUNAR-SOILS title="DIELECTRIC CONSTANT MEASUREMENTS FOR CHARACTERIZING LUNAR SOILS"&lt;img src="http://img.docstoc.com/thumb/100/1044265.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Anderson, Buehler, Seshadri, Kuhlman, and Schaap, JPL, Pasadena, University of California, Riverside: The return to the Moon has ignited the need to characterize the lunar regolith using fast, reliable in-situ methods. Characterizing the physical properties of the rocks and soils can be very difficult because of the many complex parameters that influence the measurements.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:01:21 GMT</pubDate><guid>http://www.docstoc.com/docs/1044265/DIELECTRIC-CONSTANT-MEASUREMENTS-FOR-CHARACTERIZING-LUNAR-SOILS</guid></item><item><title>IS ILMENITE ALWAYS THE DOMINANT CARRIER OF TITANIUM IN LUNAR MARE BASALTS?</title><link>http://www.docstoc.com/docs/1044264/IS-ILMENITE-ALWAYS-THE-DOMINANT-CARRIER-OF-TITANIUM-IN-LUNAR-MARE-BASALTS</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044264/IS-ILMENITE-ALWAYS-THE-DOMINANT-CARRIER-OF-TITANIUM-IN-LUNAR-MARE-BASALTS title="IS ILMENITE ALWAYS THE DOMINANT CARRIER OF TITANIUM IN LUNAR MARE BASALTS?"&lt;img src="http://img.docstoc.com/thumb/100/1044264.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Riner, Robinson, Tangeman and Elphic, Department of Geological Sciences, Northwestern University, Center for Planetary Sciences &amp; Containerless Research, Inc., Evanston, &amp; Los Alamos National Laboratory.The dominant cause for lunar visible color differences is variations in the degree of soil maturity and the abundance of FeO and opaque minerals, such as ilmenite. The addition of opaque minerals to a lunar soil tends to decrease the overall reflectance and continuum slope (darkens and decreases “redness”). As a soil weathers its reflectance is also lowered but its slope increases (darkens and increases “redness”). By exploiting these color trends numerous studies have attempted to correlate the abundance of TiO2 in the form of ilmenite to variations in blue to red ratios (i.e. 415 to 750 nm Clementine bandpasses) with varying degrees of success. Discrepancies between independent methods.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:00:53 GMT</pubDate><guid>http://www.docstoc.com/docs/1044264/IS-ILMENITE-ALWAYS-THE-DOMINANT-CARRIER-OF-TITANIUM-IN-LUNAR-MARE-BASALTS</guid></item><item><title>THE HF-W AGE OF THE LUNAR MAGMA OCEAN</title><link>http://www.docstoc.com/docs/1044263/THE-HF-W-AGE-OF-THE-LUNAR-MAGMA-OCEAN</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044263/THE-HF-W-AGE-OF-THE-LUNAR-MAGMA-OCEAN title="THE HF-W AGE OF THE LUNAR MAGMA OCEAN"&lt;img src="http://img.docstoc.com/thumb/100/1044263.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Kleine, Mezger &amp; Palme, Zentrallabor fr Geochronologie, Universitt Mnster, Corrensstr. Institut fr Isotopengeologie und Mineralische Rohstoffe, Departement fr Erdwissenschaften, ETH Zrich, Institut fr Mineralogie und Geochemie, Universitt zu Kln, Zlpicherstr, Kln, Germany  The early chemical differentiation of the Moon was dominated by the crystallization of a magma ocean. Determining the crystallization age of the lunar magma ocean (LMO) is critical for understanding the timing of Moon formation, melting, and subsequent differentiation and cooling.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:00:46 GMT</pubDate><guid>http://www.docstoc.com/docs/1044263/THE-HF-W-AGE-OF-THE-LUNAR-MAGMA-OCEAN</guid></item><item><title>Evaluation of chemical methods for projectile identification in terrestrial and lunar impactites</title><link>http://www.docstoc.com/docs/1044262/Evaluation-of-chemical-methods-for-projectile-identification-in-terrestrial-and-lunar-impactites</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044262/Evaluation-of-chemical-methods-for-projectile-identification-in-terrestrial-and-lunar-impactites title="Evaluation of chemical methods for projectile identification in terrestrial and lunar impactites"&lt;img src="http://img.docstoc.com/thumb/100/1044262.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Tagle and Hecht, Institute of Mineralogy, National History Museum, Berlin&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:00:38 GMT</pubDate><guid>http://www.docstoc.com/docs/1044262/Evaluation-of-chemical-methods-for-projectile-identification-in-terrestrial-and-lunar-impactites</guid></item><item><title>MODEL OF LIGHT SCATTERING BY LUNAR REGOLITH AT MODERATE PHASE ANGLES: NEW RESULTS</title><link>http://www.docstoc.com/docs/1044261/MODEL-OF-LIGHT-SCATTERING-BY-LUNAR-REGOLITH-AT-MODERATE-PHASE-ANGLES-NEW-RESULTS</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044261/MODEL-OF-LIGHT-SCATTERING-BY-LUNAR-REGOLITH-AT-MODERATE-PHASE-ANGLES-NEW-RESULTS title="MODEL OF LIGHT SCATTERING BY LUNAR REGOLITH AT MODERATE PHASE ANGLES: NEW RESULTS"&lt;img src="http://img.docstoc.com/thumb/100/1044261.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Velikodsky and Korokhin. Astronomical Institute of Kharkov University. Sumskaya Ul., Ukraine.We have presented in a model for the polarimetric and photometric characteristics of the lunar regolith at moderate phase angles based on realistic assumptions on regolith microstructure (see description below). Now we have new important observational data, which allow to improve a determination of model parameters and to make some conclusions about physical characteristics of the lunar surface.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:00:30 GMT</pubDate><guid>http://www.docstoc.com/docs/1044261/MODEL-OF-LIGHT-SCATTERING-BY-LUNAR-REGOLITH-AT-MODERATE-PHASE-ANGLES-NEW-RESULTS</guid></item><item><title>CALCULATIONS OF THE FLUXES OF 10-250 keV LUNAR LEAKAGE GAMMA RAYS</title><link>http://www.docstoc.com/docs/1044260/CALCULATIONS-OF-THE-FLUXES-OF-10-250-keV-LUNAR-LEAKAGE-GAMMA-RAYS</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044260/CALCULATIONS-OF-THE-FLUXES-OF-10-250-keV-LUNAR-LEAKAGE-GAMMA-RAYS title="CALCULATIONS OF THE FLUXES OF 10-250 keV LUNAR LEAKAGE GAMMA RAYS"&lt;img src="http://img.docstoc.com/thumb/100/1044260.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Kim, Reedy &amp; Gasnault, Institute of Meteoritics, University of New Mexico, Albuquerque, Centre d’Etude Spatiale des Rayonnements, ToulouseThe gamma rays measured above the surface of planetary objects can be used to study that surface’s composition. Previous and cur-rent measurements have mainly used gamma rays with energies &gt;500 keV, although most missions measured down to ~100 keV. Gamma rays above ~100 keV are very penetrating and thus hard to collimate, so previ-ous missions to the Moon and Mars have measured gamma rays arriving from the entire visible surface. The spatial resolution was not better than about the distance above the planet’s surface&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:00:25 GMT</pubDate><guid>http://www.docstoc.com/docs/1044260/CALCULATIONS-OF-THE-FLUXES-OF-10-250-keV-LUNAR-LEAKAGE-GAMMA-RAYS</guid></item><item><title>A DYNAMIC FOUNTAIN MODEL FOR LUNAR DUST</title><link>http://www.docstoc.com/docs/1044259/A-DYNAMIC-FOUNTAIN-MODEL-FOR-LUNAR-DUST</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044259/A-DYNAMIC-FOUNTAIN-MODEL-FOR-LUNAR-DUST title="A DYNAMIC FOUNTAIN MODEL FOR LUNAR DUST"&lt;img src="http://img.docstoc.com/thumb/100/1044259.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Stubbs, Vondrak &amp; Farrell, NASA Goddard. During the Apollo era of exploration it was discovered that sunlight was scattered at the terminators giving rise to “horizon glow” and “streamers” above the lunar surface. This was observed from the dark side of the Moon during sunset and sunrise by both surface landers and astronauts in orbit. These observations were quite unexpected, as the Moon was thought to be a pristine environment with a negligible atmosphere or exosphere. Subsequent investigations have shown that the sunlight was most likely scattered by electrostatically charged dust grains originating from the surface.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 22:00:09 GMT</pubDate><guid>http://www.docstoc.com/docs/1044259/A-DYNAMIC-FOUNTAIN-MODEL-FOR-LUNAR-DUST</guid></item><item><title>PLANETARY GAMMA-RAY IMAGER USING HIGH PRESSURE XENON TIME PROJECTION CHAMBER</title><link>http://www.docstoc.com/docs/1044258/PLANETARY-GAMMA-RAY-IMAGER-USING-HIGH-PRESSURE-XENON-TIME-PROJECTION-CHAMBER</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044258/PLANETARY-GAMMA-RAY-IMAGER-USING-HIGH-PRESSURE-XENON-TIME-PROJECTION-CHAMBER title="PLANETARY GAMMA-RAY IMAGER USING HIGH PRESSURE XENON TIME PROJECTION CHAMBER"&lt;img src="http://img.docstoc.com/thumb/100/1044258.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Hasebe, Yamashita, Kobayashi, Miyachi, Miyajima, Okudaira, Kobayashi, Hosojima, Pushkin, Tezuka, Doke, &amp; Shibamura, Advanced Research Institute for Science and Engineering, Waseda Univ., Tokyo, College of Health Science, Saitama Prefectural Univ.,Koshigaya, Saitama.  Explorations of lunar and planetary surfaces by gamma-ray spectroscopy have been obtaining excellent results in recent missions. However, due to the difficulty of gamma-ray collimation, the spatial resolution of gamma-ray spectrometers is not comparable to X-ray, visible, UV, or IR cameras. Compton Telescopes cannot uniquely identify the arrival direction of a single incident gamma ray, and are only applicable for point-like sources.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 21:59:55 GMT</pubDate><guid>http://www.docstoc.com/docs/1044258/PLANETARY-GAMMA-RAY-IMAGER-USING-HIGH-PRESSURE-XENON-TIME-PROJECTION-CHAMBER</guid></item><item><title>Antipodal magnetic anomalies on the Moon, contributions from impact induced currents due to positive holes and flexoelectric phenomena and dynamo</title><link>http://www.docstoc.com/docs/1044257/Antipodal-magnetic-anomalies-on-the-Moon-contributions-from-impact-induced-currents-due-to-positive-holes-and-flexoelectric-phenomena-and-dynamo</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044257/Antipodal-magnetic-anomalies-on-the-Moon-contributions-from-impact-induced-currents-due-to-positive-holes-and-flexoelectric-phenomena-and-dynamo title="Antipodal magnetic anomalies on the Moon, contributions from impact induced currents due to positive holes and flexoelectric phenomena and dynamo"&lt;img src="http://img.docstoc.com/thumb/100/1044257.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Kletetschka, Freund, Wasilewski and Kohout; Department of Physics, Catholic University of America Washington, NASA Goddard, Institute of Geology, Academy of Sciences of the Czech Republic, Department of Applied Geophysics, Faculty of Science, Charles University in Prague, Division of Geophysics, Department of Physical Sciences, University of Helsinki, Helsinki, Finland.Large impacts on the Moon generate large pressure pulses that penetrate the whole body. Several of these large impacts may have generated antipodal structurewith  anomalous magnetic intensity.These regions can be more than a thousand km across, with fields of the order of tens to hundreds of nT. This is the case of Orientale, Imbrium, Serenitatis, Crisium, and Nectaris impact basins.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 21:59:40 GMT</pubDate><guid>http://www.docstoc.com/docs/1044257/Antipodal-magnetic-anomalies-on-the-Moon-contributions-from-impact-induced-currents-due-to-positive-holes-and-flexoelectric-phenomena-and-dynamo</guid></item><item><title>UNIQUE PROPERTIES OF LUNAR SOIL FOR IN-SITU RESOURCE UTILIZATION ON THE MOON</title><link>http://www.docstoc.com/docs/1044255/UNIQUE-PROPERTIES-OF-LUNAR-SOIL-FOR-IN-SITU-RESOURCE-UTILIZATION-ON-THE-MOON</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044255/UNIQUE-PROPERTIES-OF-LUNAR-SOIL-FOR-IN-SITU-RESOURCE-UTILIZATION-ON-THE-MOON title="UNIQUE PROPERTIES OF LUNAR SOIL FOR IN-SITU RESOURCE UTILIZATION ON THE MOON"&lt;img src="http://img.docstoc.com/thumb/100/1044255.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Taylor and Taylor, Planetary Geosciences Institute, University of Tennessee, Knoxville.Moon is an enormous Earthorbiting space station, a natural satellite outside of Earth’s gravity well, with raw materials that can be put to practical use as humanity expands outward into the solar system&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 21:59:08 GMT</pubDate><guid>http://www.docstoc.com/docs/1044255/UNIQUE-PROPERTIES-OF-LUNAR-SOIL-FOR-IN-SITU-RESOURCE-UTILIZATION-ON-THE-MOON</guid></item><item><title>Pickup Ion Mass Spectrometry for Surface Bounded Exospheres and Composition Mapping of Lunar and Planetary Surfaces</title><link>http://www.docstoc.com/docs/1044254/Pickup-Ion-Mass-Spectrometry-for-Surface-Bounded-Exospheres-and-Composition-Mapping-of-Lunar-and-Planetary-Surfaces</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044254/Pickup-Ion-Mass-Spectrometry-for-Surface-Bounded-Exospheres-and-Composition-Mapping-of-Lunar-and-Planetary-Surfaces title="Pickup Ion Mass Spectrometry for Surface Bounded Exospheres and Composition Mapping of Lunar and Planetary Surfaces"&lt;img src="http://img.docstoc.com/thumb/100/1044254.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Keller and Zurbuchen, Baragiola, Cassidy, Chornay, Collier, Hartle, Johnson, Killen, Koehn, Ogilvie1, Scherer, Stubbs, NASA Goddard &amp; University of Michigan, Ann Arbor, University of Maryland, College Park &amp; Engineering Physics, University of Virginia, CharlottesvilleMany of the small to medium sized objects in the solar system can be characterized as having surface bounded exospheres, or atmospheres so tenuous that scale lengths for inter-particle collisions are much larger than the dimensions of the objects. The atmospheres of these objects are the product of their surfaces, both the surface composition and the interactions that occur on them and also their interiors when gases escape from there. Thus by studying surface bounded exospheres it is possible to develop insight into the composition and processes that are taking place on the surface and interiors of these objects. The Moon and Mercury are two examples of planetary bodies with surface bounded exospheres that have been studied through spectroscopic observations of sodium, potassium, and, on the moon, mass spectrometric measurements of lunar gases such as argon and helium&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 21:58:54 GMT</pubDate><guid>http://www.docstoc.com/docs/1044254/Pickup-Ion-Mass-Spectrometry-for-Surface-Bounded-Exospheres-and-Composition-Mapping-of-Lunar-and-Planetary-Surfaces</guid></item><item><title>VISIBLE AND NIR BRDF MEASUREMENTS OF LUNAR SOIL SIMULANT</title><link>http://www.docstoc.com/docs/1044253/VISIBLE-AND-NIR-BRDF-MEASUREMENTS-OF-LUNAR-SOIL-SIMULANT</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044253/VISIBLE-AND-NIR-BRDF-MEASUREMENTS-OF-LUNAR-SOIL-SIMULANT title="VISIBLE AND NIR BRDF MEASUREMENTS OF LUNAR SOIL SIMULANT"&lt;img src="http://img.docstoc.com/thumb/100/1044253.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Gunderson &amp; Whitby and Thomas, Physikalisches Institut, University of Bern, Switzerland.Bidirectional reflectance distribution functions (BRDFs) characterize the outgoing intensity of light from illuminated surfaces according to the illumination and observation geometries of those surfaces&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 21:58:40 GMT</pubDate><guid>http://www.docstoc.com/docs/1044253/VISIBLE-AND-NIR-BRDF-MEASUREMENTS-OF-LUNAR-SOIL-SIMULANT</guid></item><item><title>GARNET IN THE LUNAR MANTLE: FURTHER EVIDENCE FROM VOLCANIC GLASS BEADS</title><link>http://www.docstoc.com/docs/1044252/GARNET-IN-THE-LUNAR-MANTLE-FURTHER-EVIDENCE-FROM-VOLCANIC-GLASS-BEADS</link><description>&lt;div&gt;&lt;a href=http://www.docstoc.com/docs/1044252/GARNET-IN-THE-LUNAR-MANTLE-FURTHER-EVIDENCE-FROM-VOLCANIC-GLASS-BEADS title="GARNET IN THE LUNAR MANTLE: FURTHER EVIDENCE FROM VOLCANIC GLASS BEADS"&lt;img src="http://img.docstoc.com/thumb/100/1044252.png" alt="" style="border: 1px solid #C3E6D8; float: right;" /&gt;&lt;/a&gt;&lt;br /&gt;shared by: &lt;a href="http://www.docstoc.com/profile/Prospero"&gt;Prospero&lt;/a&gt; on: Tuesday, August 12, 2008&lt;p&gt;Neal, Shearer &amp; Kramer, Dept. Civil Eng. &amp; Geological Sci., University of Notre Dame &amp; Univ. of New Mexico, Albuquerque.  Volcanic glass beads returned from the Moon represent a unique class of igneous material through which the interior of the Moon can be studied.&lt;/p&gt;&lt;/div&gt;</description><author>Prospero</author><pubDate>Tue, 12 Aug 2008 21:58:33 GMT</pubDate><guid>http://www.docstoc.com/docs/1044252/GARNET-IN-THE-LUNAR-MANTLE-FURTHER-EVIDENCE-FROM-VOLCANIC-GLASS-BEADS</guid></item></channel></rss>