presentation - Center for Adaptive Optics
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IRIS Telescope Camera
Kimberly Bott
Institute for Astronomy
Mentor: Klaus Hodapp
Home Institution: University of Hawaii
at Hilo
2008 Center for Adaptive Optics
Akamai Internship
• Infrared Imaging Survey
System (near IR)
Introduction • Telescope fabrication in
Germany
• Camera fabrication in
US
• IRIS site: Cerro
Armazones Observatory
in Chile
• Telescope Goals
– Occultation
– Variations in reflection
nebulae
• Camera Goals
– Effective IR camera
– Correct for spherical
aberrations
Infrared Camera
• Cryostat interior to vacuum
– Why a cryostat?
• Three components
– Designed mounting
– Designed and fabricated
vacuum casing
– Learned to fabricate on
cryostat piece
– Goals
• Be lightweight, balanced
and strong
• Allow extra volume for
cryostat piece
Infrared Camera
• Cryostat interior to vacuum
– Why a cryostat?
• Three components
– Designed mounting
– Designed and fabricated
vacuum casing
– Learned to fabricate on
cryostat piece
– Goals
• Be lightweight, balanced
and strong
• Allow extra volume for
cryostat piece
Infrared Camera
• Cryostat interior to vacuum
– Why a cryostat?
• Three components
– Designed mounting
– Designed and fabricated
vacuum casing
– Learned to fabricate on
cryostat piece
– Goals
• Be lightweight, balanced
and strong
• Allow extra volume for
cryostat piece
Infrared Camera
• Cryostat interior to vacuum
– Why a cryostat?
• Three components
– Designed mounting
– Designed and fabricated
vacuum casing
– Learned to fabricate on
cryostat piece
– Goals
• Be lightweight, balanced
and strong
• Allow extra volume for
cryostat piece
Testing the Camera’s Existing
Cryostat
• Test vacuum
• Inject liquid nitrogen
into cryostat
– Monitored weight of
camera to determine
holding time
– Improve holding time
– Retest with new
pieces
Design of Mounting Piece
• Designed as strong
connection between
camera and
telescope
Vacuum Casing Design
• AutoCAD drawing
• Connection between
existing casing and
large mounting
piece
• Allowing for an
effective vacuum
– Smooth to reduce
dust/oil presence
– Lower emissivity
Fabricating the Part
• Used lathe to aid
other intern with
small cryostat piece
• Began work on own
part
– Required improvising
due to unusual size
and an octagonal
end
Testing the Part
• Assembled
• Achieved near
perfect vacuum
Filter Wheel Electronics
• 7 IR filters on large
gear
• Driven by stepper
motor
• Located with a Hall
Effect Sensor
• Controlled through
computer (program
in C)
Electronics
• Replaced
connections
– Female electronics
to male
– Female to the
stepper motor and
the Hall Effect
sensor
Electronics Testing and
Results
• Tested connections
with multimeter
• Tested ensemble,
ran program to
begin locating filters
– Did not align
– Fixed number of
teeth in C program
– Still an issue finding
the magnet
Conclusions
Mounting piece:
accurate design
Vacuum casing:
effective vacuum
which does hold
Filter wheel electronics:
good connections but
improper alignment
not due to tooth
number
Acknowledgements and
Sources
• The Akamai Internship Program, funded by the Center for
Adaptive Optics through its National Science Foundation
Science and Technology Center grant (#AST-987683)
• Institute for Astronomy
• Dr. Klaus Hodapp
• Richard Shelton
• “The Infrared Imaging Survey (IRIS) System”, Hodapp et al.
• “Cryostat Design and Construction at the IRTF”, Toomey et al.
• http://uigi.com/nitrogen.html
Additional Links
• http://www.magnet.fsu.edu/education/tut
orials/java/halleffect/index.html
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