PowerPoint Presentation by GeAb2hXa


									                 The Earth’s Atmosphere
1. Introduction
    (not in the book)

2. Gases in Earth's

3. Vertical structure of
   atmospheric pressure &

4. Types of weather & climate
    in the atmosphere
                              My Meteorology Timeline
                 (Some interesting meteorological periods and events)
   Meteorology as an exact science is relatively young but….measurements have been made
                                  through recorded history
•400 B.C. – Rainfall measured in India.
• Pre-1600’s – Predictions were based on recurring patterns (example: when the wind switches
from east to south, expect storms). There was no understanding of why these recipes worked (and
why they did not).
• 1600’s – Measurements of surfaces quantities began. Isaac Newton develops his 3 laws of
motion, the beginnings for a mathematical description of meteorology.
• 1800’s – The beginning of determinations of the forces, which act to change the weather, some
simple theories and classifications are developed.
• 1900’s – The understanding that the vertical structure of the atmosphere is important and must
be measured.
• 1944 – The first quantitative map identifying the jet stream. Mid 1940’s to 1950’s – Radars
were beginning to be used for weather experiments.
• 1955 – The first operational weather prediction model was ran on an IBM computer.
• 1960 – The first weather satellite was launched into space (Tiros 1).
• 1974 – The first Geostationary Operational Environmental Satellite (GOES) was launched.
• Early 1990’s – The first NEXt generation RADar (WSR-88D) was implemented at a NWS
weather forecast office.
• 2000's – The Weather Research & Forecasting (WRF) numerical prediction model was created
to merge the forecast and research communities together.
• This decade – Dual Doppler radars and the next generation GOES satellites being used
       Basic Definitions That Are Often Misused and
Weather – the state of the atmosphere at a given location and time along with the short term
  changes in that state (e.g., temperature, wind speed and direction, precipitation, etc.)

Climate – the “average” state of the atmosphere at a given location and over a given period
   of time and the long term changes in that “average” condition. Typically included in the
   definition of “Climate” is the typical range of extremes (example: Denver in September
   has an averaged temperature of 62.4°F with daily averaged highs between 82 – 73°F
   and lows between 53 – 42°F).

Meteorology – the study of the atmosphere and atmospheric phenomena/processes as well
  as the atmosphere’s interaction with the earth’s surface, oceans, and life in general.

   Example of processes that effect weather:
       • Energy from the sun
       • Effects of the earth’s surface
       • Clouds
       • Effects of water (in all 3 phases)
       • Movement of air
       • Societal Impacts (to a degree)
     Meteorological Units of Measurement
In meteorology, for the most part, the International System of Units (SI)
are used instead of the Imperial Units (English/United States). The SI
system is based on the metric units of measure which use meter-kilogram-
second (mks) system instead of centimeter-gram-second (cgs) system.
             Kilometers (km)                    Miles (mi)

                   1.0                            ~ 2/3

                   10.0                          ~ 6 1/4

                  1000                            ~ 625

            Millimeters (mm)                    Inches (in)

                   1.0                             0.04

                   25.4                            1.00
           Meteorological Units (cont.)
Note: There is not a degree character for the Kelvin scale.

 Celsius (°C)         Fahrenheit (°F)           Kelvin (K)
     100                    212                  373.15
     38                     100                   311.15
     27                     80                   300.15
     16                     60                   289.15
      4                     40                   277.15
      0                     32                   273.15
     -18                     0                   255.15
     -40                    -40                  233.15
                     Meteorological Units (cont.)

   millibars (mb)           Pascal (Pa)              lbs/in2 (psi)      Inches of Hg (inHg)

          1                     100                     0.014                 0.02953

         10                     1000                    0.145                 0.2953

        100                    10,000                    1.45                  2.953

        500                    50,000                    7.25                 14.765

        1000                  100,000                   14.45                  29.53

 1013.25* or 1 atm            101,325                    14.7                  29.91

* The pressure observed at sea-level under standard atmospheric conditions.
Naming Convention of Meteorological Graphs and Maps
Graphs and maps help to display and illustrate certain meteorological principles
and data in a more concise way. Most graphs fall under 2 categories.
Vertical Profile or Profile – a map or graph that displays variables as a function
of the distance above the earth surface over a single point.
Horizontal / Plan-view Map – a type of map/graph that displays
information on a horizontal plane with a geographical map usually as
set as a background, which makes it easier to determine geographical
Vertical Cross-Section – is a map/graph that looks at the atmosphere
in a vertical plane along a horizontal line. It is useful to illustrate
atmospheric characteristic associated with particular phenomena
(e.g., fronts, thunderstorms, etc.). Vertical cross-section can be
thought of as taking a slice of the atmosphere.
       What is a “Real” Meteorologist?
• An individual who shows aptitude in the following fields:
   – Mathematics
   – Physics
   – Chemistry
   – Geography
   – Computer Science

• An individual who uses these (above mention) skills to
  develop a better understanding on how the atmosphere
  behaves in the short- and long-term.

• Moreover, the individual must have completed the
  requirements for a college degree (B.S.) in
  meteorology/atmospheric science.
                      The Importance of Solar Energy

•Nearly 150 million kilometers separate the sun and earth, yet solar radiation (radiant energy)
drives earth's weather.

•Sun’s radiant energy also helps to maintain an average temperature of 15 °C at the surface of
the earth but a wide range of temperatures is experience as well.

•Examples of the temperature extremes that can be experienced on the earth surface are 1) on a
chilly Antarctic night, temperatures can drop below -85°C (-121°F) and 2) over a hot
subtropical desert (like the Sahara Desert), the thermometer can climb to 50°C (122°F).
          Earth's Atmosphere
• Our atmosphere is a thin, gaseous shell made
up of mostly nitrogen and oxygen, with small
amounts of other gases.

• About 99% of atmospheric gases, including
water vapor, extend only 30 kilometer (km)
above earth's surface but the last 1% reaches
heights greater than 600 km.

•So a majority of our atmosphere is below 30
km in height. There is no true hardtop of the
atmosphere but rather the earth's atmosphere
and space merges together.

• At 600 km, the mean free path between air
molecules is about 10 km.

• Most of our weather, however, occurs within
the first 10 to 15 km.
         99% of the                                      Highly
        atmosphere          Greenhouse Gases             Variable
• Composition of the Atmosphere can be separated into 2 categories:
    1. Permanent Gases
    2. Variable Gases
Permanent Gases
99% of the earth's atmosphere is made up of predominantly two gases: 1) Oxygen (O2)
and Nitrogen (N2). Out of a possible 100%, N2 consists of 78% of the earth's
atmosphere. O2 is responsible for 21% of the earth's atmosphere and the remaining 1%
is a potpourri of different trace gases. Permanent gas percentages represent a constant
amount of gas which are very slow to change but cycles of destruction and production
are constantly maintaining this amount on a daily, weekly and yearly basis.

Variable Gases
Variable gases concentration can change greatly from day-to-day or year-to-year
depending on the gas constituent. Sometimes, changes in these trace gases’
concentrations can have a large effect.
Do these trace/variable gases play an important role in the
•   Take water vapor (H2Ov) for example, the percentage of water vapor can vary
    anywhere from 0% to 4% which is dependent on the evaporation and condensation
    rates over a particular location. If the condensation rate dominates then the chances of
    precipitation increase and vice versa with evaporation.

•   However, as a society, we are almost always concerned about the possibility of

•   Sometimes, changes in these trace/variable gases can have a large effect.

•   H2Ov (water vapor) are invisible and concentration varies at different latitudes.
         • becomes visible when changing into a larger liquid or solid particles, such as
           cloud droplets and ice crystals.
         • Condensation – vapor state to liquid
         • Evaporation – liquid to vapor
         • Latent heat is release during condensation; this is a source of atmospheric
           energy beside the sun (drives storms)
         • It is a form of green house gas because it absorbs outgoing radiant energy (e.g.
           glass of a green house)
Atmospheric Gases
                    •Nitrogen, oxygen,
                    argon, water vapor,
                    carbon dioxide, and
                    most other gases are

                    • Clouds are not gas,
                    but condensed vapor in
                    the form of liquid

                    • Ground based smog,
                    which is visible,
                    contains reactants of
                    nitrogen and ozone
                    (bad type).
The atmospheric carbon dioxide cycle

                        • CO2 is being released into the
                          atmosphere via man-made
                          and natural sources.

                        • An excess in CO2
                          concentration in the
                          atmosphere will rise the
                          overall global temperature if
                          the CO2 creation process
                          does not equal the removal

                        • The ocean is a huge sink of
                          CO2 along with the
                          photosynthesis process which
                          helps to remove the CO2
                          from the atmosphere.
                            Increasing Greenhouse Gases

•The 50-year graph (left) provides an example on how the CO2 concentration can vary on a seasonal basis
with vegetation growth peaking during the spring and summer (gray line is the actual observation and the
blue line is the yearly average).

•In order to get a better understanding on how the CO2 concentration has increase rapidly, let's look at the last
1000 years.

•Most of the past CO2 concentration data are acquired from ice core samples. The 1000-year graph (right)
shows an actual decline in CO2 concentration from 1500 to 1600 when Europe experienced a mini-ice age.

•From 1800 to the present, the CO2 concentration accelerates almost exponentially.
                               Aerosols & Pollutants

•Human and natural activities displace tiny soil, salt, and ash particles as suspended aerosols, as
well as sulfur dioxide, nitrogen dioxide, and hydrocarbons as pollutants.

•In addition, atmosphere contains impurities from natural (dust and soil) and man-made sources
called aerosols.

•Aerosols are disbursed into the atmosphere by the wind and helps with the formation of
precipitation (to be discussed further in depth on a later module).

•Pollutants are associated with man-made impurities, such as carbon monoxide (CO), that cause
health hazard.
    Early atmosphere (4.6 billion yr ago)
•   1st atmosphere made up of helium and hydrogen escaped
    –   too light
•   2nd atmosphere from constant volcanic eruptions and
    “outgassing” of WV (80%) and CO2 (10%) and a few %
    of N2.
•   As rain fell for 1000s of years, forming lakes, rivers, and
    oceans, CO2 was dissolved into the ocean or became
    carbonate sedimentary rock such as limestone.
•   N2 (not chemically active) started to dominated with the
    depletion of CO2.
•   O2 were produced either by:
    –   H2O being broken down by the sun energy
    –   Plants forming in an O2 free environment (photosynthesis)
                            Pressure & Density
The properties of the atmosphere change as you move away form the surface, particularly,
                           pressure, temperature and density.

                                                       •Weight = mass × gravity (kg)

                                                       •Density = mass ÷ volume (kg/m3)

                                                       •Pressure = force ÷ area (lb/in2)

                                                       •Gravity pulls gases toward earth's
                                                       surface, and the whole column of
                                                       gases weighs 14.7 psi at sea level, a
                                                       pressure of 1013.25 mb or 29.92

                                                       •Pressure and density decreasing with
                                                       height is not a linear relationship but
                                                       rather a logarithmic relationship.

                                                       •Interestingly, the weight of the
                                                       atmosphere is approximately 5600
                                                       trillion (5.6 quadrillion) tons.
  Vertical structure of atmospheric pressure &
• The properties of the atmosphere change as one moves away
from the surface, particularly, pressure, temperature and

• Air molecules are held closer near the earth by gravity, this
effect the numbers of molecules in a given volume.

• Air density is the greatest at the surface because it is defined
as the numbers of air molecules in a volume.

• Air molecules have weight => act as a force upon the earth =>
this force can measured => air pressure or atmospheric pressure
– the amount of force exert over a surface area.
                                  Vertical Pressure Profile

•This figure illustrates the rapid decrease of air
pressure with height

•Pressure increases at a curved rate (logarithmically)
proportional to altitude squared, but near the surface
a linear estimate of 10 mb per 100 meters works well.

•Basically, half the atmosphere (500mb) is below the
elevation of 5.5 km or 18,000 ft.

•Mount Everest elevation is approximately 9 km or
29,000ft above sea-level. The pressure reading
should be around 300 mb there nearly 70% of the air
molecules that exist in the entire atmosphere is below
Mount Everest.

•The atmosphere stretches in the vertical for
hundreds of kilometer until eventually becoming
thinner and thinner to the point of merging with
space. This level where the atmosphere and space
merges is approximately 600 km.
 Atmospheric Layers
• Five layers are defined by
constant trends in average air
temperature (which changes
with pressure and radiation),
where the outer exosphere is
not shown.

• Temperature starting at the
surface usually decreases with
height until 11 km (36,000 ft or
7 mi).

•This is due to sunlight
warming the earth’s surface
and which in turn the surface
warms the air above it.
                Vertical Temperature Trend
• The rate at which temperature decreases with height is called a
lapse rate.
       • The “average” lapse rate is 6.5 C/1000 m
       • Lapse rate varies daily and even hourly
       • The “norm” in the troposphere

• On occasions, temp increases with height, this is called a
temperature inversion.

• An isothermal layer is defined as a region where there is no
change in temperature with height.

• Radiosonde is used to measure temperature high up in the
Troposphere is located from the surface to about 11 km above mean sea-level (MSL). This is
where most of the weather takes place. Normally, temperature decreases with height, where the
temperature no longer decreases with height over a large depth marks the top of the troposphere.

Stratosphere is the layer above the troposphere and characterized by temperature increasing with
height. This warming is associated with the absorption of sun's energy by the ozone layer.

Tropopause – is the interface or boundary separating the troposphere and stratosphere. Little
mixing occurs between the two layers. Where air mixes from the two layers occurs near jet
streams where tropopause tends to break or weaken. The tropopause height varies with latitude
and seasons.

Mesosphere – is located above the stratosphere. Atmospheric density is extremely low at this
level and even though about 21% of the atmosphere still consists of oxygen, life can only be
sustained with a breathing apparatus. On the average, this is the coldest layer of the atmosphere.
It has an average temperature of -90 °C.

Thermosphere – is where air molecules are few and far between. Atmosphere, as we know it, in
this region is unrecognizable. Lighter molecules dominate and travel very fast due to the strong
absorption of the sun’s energy. Air temperature can exceed 500 °C. Due to the few molecules
in this region, one would not feel hot but rather quite frigid if shielded from the sun.

Stratopause and Mesopause – are the boundaries the stratosphere-mesosphere and mesosphere-
thermosphere, respectively.
                  Atmospheric Mixture & Charge
                               Temperature   Composition Properties

layers include:

a) the
with 78%
nitrogen and
21% oxygen

b) the poorly

c) the
Exosphere – is upper limit of the atmosphere where space and atmosphere merge
together. Molecules and atoms in this region can escape the earth’s gravity.

Homosphere – is the layer of the atmosphere where the composition of the
atmosphere remains constant (78% Nitrogen and 21% Oxygen). This uniformity is
achieved through turbulent mixing. This layer goes up from the surface to 85 km,
where the thermosphere begins.

Heterosphere – starts at 85 km above the earth’s surface and extend out into free
space. Collision between atoms and molecules are infrequent so the atmosphere is
unable to keep up the mixing process. Heavier elements and molecules settle to the
bottom of the layer while the lighter materials rise to the top.

Ionosphere – is not “real” a layer but rather an electrified region within the upper
atmosphere where fairly large concentrations of ions and free electrons exist. It
extends from 60 km above the earth’s surface to the top of the atmosphere. It also
plays a major role in radio communication.
                    Radio Wave Propagation

AM radio waves are long enough to interfere with ions in the sun-
charged D layer, but at night the D layer is weak and the AM signal
propagates further, requiring stations use less power.
                        Weather & Climate

Weather is comprised of measured variables which
  can be predicted:

1.   Air temperature – how hot or how cold the air is? (degree of hotness
     and coldness)
2.   Air pressure – the force of air exerted above an area
3.   Humidity – a measure of the amount of water vapor (moisture) in the air
4.   Clouds – a visible mass of tiny water droplets and/or ice crystals that are
     above the earth’s surface
5.   Precipitation – any form if water, either liquid or solid (rain, ice, or
     snow), that falls from clouds and reaches the ground
6.   Visibility – the greatest distance one can see (fog and pollutants)
7.   Wind – the horizontal movement of air

Climate represents long-term (e.g. 30 yr) averages of weather
   (Climatology); can also be thought of as a local, regional, or
   global trend.
  Remote Sensing Instruments
•Meteorologists may study larger
weather patterns with space borne
instruments, while ground-based
tools often measure a single point.

•Satellites provide a large view of
the present weather. Geostationary
Satellite (36,000 km or 22,300 mi)
travels the same rate as the earth
axis rotation. It allows for
continuous coverage over a certain

•Doppler radars provide a local
 view of smaller present weather.
• Middle latitudes (mid-latitudes) is where the US is located between 30°N to 50°N.
Known as the “active weather latitudes” – hurricanes, tornadoes, thunderstorms, hails, flash
floods, blizzards, etc are found in this region.

• Tropics – equator to 30°N or S

• Different Storm sizes
          1) Mid-latitude Cyclonic Cyclone (middle-latitude cyclonic storm,
          mid-latitude cyclone, extratropical cyclone) – storms outside the tropics. It spins
          counterclockwise in the NH. Over 2000 km in size
          2) Hurricane (tropical cyclone) – smaller but more vigorous storm has a
          tropical origin.
                     ~ Spins the same way as (middle-latitude cyclonic storm but
                     usually have higher sustain surface winds (> 74 MPH)
                     ~ An eye of a hurricane is calm and clear. The lowest pressure of
          the storm is located there. Highest winds are located just outside the eye
                     in a region called the eyewall.
          3) Thunderstorms are even smaller. Developed from cumulus cloud
          (Puffy white cloud with a vertical growth to them).
                     ~ Lightening, thunders, strong gusty winds, heavy rain, and
                     possible hail are associated with T’storms
                     ~ Organized T’storms (supercell) can produce tornadoes.
                     ~Tornado wind can exceed 230 mph but are usually less than
                     140 mph.
                          Surface Weather Map

•Meteorologists generate diagrams of observed weather from ground-based

• This surface map overlaps in time with the previous satellite but a radar image can
also be overlaid to provide a better representation of the present weather/atmosphere.
• Surface map can be overlaid in time with satellite and radar images to provide a better
  representation of the present weather/atmosphere.
      • L values are called low and marks the center of the middle-latitude cyclonic storm.
       Blows counterclockwise and inward. Stormy weather.
      • H represents high or anticyclone. Blows clockwise and outward. Fair weather.
      • Surface weather stations are depicted by small circle on the map reporting temperature,
       cloud cover, wind speed and direction (Wind direction is reported by which way the
       wind is coming from).
               • Wind speed is indicated by wind barbs
      • Points to note:
               • Winds – blows form high to low due to the horizontal pressure differences
                 (primary driving force of the wind)
               • Due to the earth’s rotation, the winds are deflected to the right in the NH
               • This deflection causes winds to blow:
                  -> Clockwise and outward at the center of H
                  -> Counterclockwise and inward at the center of L

• Winds within a surface low center at the surface has the wind eventually converging together
  and rise where rising air cools to become clouds.
     • Usually stormy weather

• Air within a surface high pressure sinks and usually causes clear sky.
• Front is surface boundary that separate different air masses with different
characteristics and is associated with sharp atmospheric changes such as:
          ~Wind direction

• Cold front – in blue, replaces warmer air ahead with the triangle pointing at the
direction of the frontal movement

• Warm front – in red replaces cooler air ahead with semi-circle pointing at the
direction of the frontal direction.

• Occluded Front – is when a cold front catches up with a warm front.

• Stationary front – a boundary between cool air and warm air with no or little

• Ahead of the first three frontal types, warm air is rising to produce clouds and

• All four fronts can produce a significant amount of precipitation.
             Societal Impacts
• Cold windy day - Wind Chill - must dress appropriately
• Summer day - Proper hydrated or heat exhaustion/stoke
• Chinook wind
• Long term temperature trends
    –Cold Spell
    –Heat waves
• Severe T’Storms
• Flash Flood - Number one Natural phenomenon causalities
• Air Travel
    –Downburst – destroying crops as well
    –Wind shear – directional or speed change in the wind
    Societal Impacts of Weather 1/5

Thunderstorms developing along an approaching cold front
Societal Impacts of Weather 2/5

    An ice storm causing power outage.
              Societal Impacts of Weather 3/5

Tornadoes annually inflict widespread damage and cause the loss of many lives
                  Societal Impacts of Weather 4/5

Flooding during April 1997, inundates Grand Forks, ND, as flood waters of the Red River
                              extend over much of the city.
                   Societal Impacts of Weather 5/5

      Estimates are that lightening strikes the Earth about 100 times every second
(8.64 million strikes per day). About 25 million lightning strikes hit the U.S. every year.

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