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Wednesday April 4, 2012 (Discussion & Worksheet – The Structure of the Atmosphere; Earth- Sun Relationships)

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Wednesday April 4, 2012. (Discussion & Worksheet – The Structure of the Atmosphere; Earth-Sun Relationships). The Launch Pad Wednesday, 4/4/12. NOTE: Put this on your green worksheet to answer Question #1. - PowerPoint PPT Presentation

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Page 1: Wednesday April  4,  2012

WednesdayApril 4, 2012(Discussion &

Worksheet – The Structure of the

Atmosphere; Earth-Sun Relationships)

Page 2: Wednesday April  4,  2012

The Launch PadWednesday, 4/4/12

Which of the following components of our atmosphere would you consider to be

disadvantageous, and why?nitrogenoxygenargon

carbon dioxidewater vapor

smogsmokedust

too much causes the greenhouse effect

air quality pollutantair quality pollutantair quality pollutant

NOTE: Put this on your green worksheet to answer Question #1

Page 3: Wednesday April  4,  2012

Assignment Currently Open

Summative or Formative Date Issued Date Due

Date Into Grade Speed

Last Day

Quiz 24 S5 3/23 3/23

WS - The Coastal Zone and Waves F 3/27 3/30

Quiz 25 S6 3/30 3/30

WS – Weather, Climate, and the

AtmosphereF 4/2 4/5

Page 4: Wednesday April  4,  2012

AnnouncementsI will be available after school today

until 5:00.

Page 5: Wednesday April  4,  2012

Latest News

http://www.sciencedaily.com/releases/2012/03/120330110535.htm

Extreme Weather Threatens Rich Ecosystems

Click below for article:

Page 6: Wednesday April  4,  2012

WorksheetThe Structure of the

Atmosphere; Earth-Sun Relationships

Page 7: Wednesday April  4,  2012

The Structure of the Atmosphere The atmospheric pressure at any

point is the weight of the air above that point.

The average sea level pressure is slightly more than 1,000

millibars, or about 14.7 pounds per square inch.

Atmospheric pressure decreases with altitude.

One-half of the Earth’s atmosphere is below 3.5 miles in

altitude.Ninety percent of our

atmosphere is below 10 miles.

Page 8: Wednesday April  4,  2012

Figure 16.6

Atmospheric Pressure Variation

with Altitude

Page 9: Wednesday April  4,  2012

The Structure of the Atmosphere Earth’s atmosphere can be layered

based upon temperature.

The troposphere is the bottom layer.

As you ascend into the atmosphere, temperature decreases with altitude,

which is referred to as the environmental lapse rate.

6.5˚C per kilometer, or 3.5˚F per 1,000 feet is the average lapse rate

for temperature.

Our atmosphere’s thickness varies, but is on average height about 12 km.

The outer boundary of the atmosphere is called the tropopause.

Page 10: Wednesday April  4,  2012

The Structure of the Atmosphere Earth’s atmosphere can be layered

based upon temperature.

The stratosphere extends from an altitude of about 12 km up to about 50

km.

Temperature increases at the top of the stratosphere.

The stratosphere’s outer boundary is named the stratopause.

The mesosphere begins at an altitude of about 50 km and climbs up to about

80 km.

Here the temperature decreases again.

The outer boundary of the mesosphere is named the mesopause.

Page 11: Wednesday April  4,  2012

The Structure of the Atmosphere Earth’s atmosphere can be layered

based upon temperature.

Above the mesosphere is the thermosphere, which has no well-

defined upper limit.

Just a tiny fraction of our atmosphere’s mass is in this region, with gases moving at high speeds.

Page 12: Wednesday April  4,  2012

Thermal Structure of

the Atmosphere

Figure 16.8

Page 13: Wednesday April  4,  2012

Earth - Sun Relations Remember from our study of

astronomy that the Earth has two major motions:

Earth rotates (spins) on its axis once every 24 hours.

Earth also revolves (orbits) around the Sun once every 365.25 days.What causes our seasons is the changing Sun angle through the Earths yearly revolution cycle. In addition, there is a change in

the length of daylight hours throughout the year.

Page 14: Wednesday April  4,  2012

Relationship of Sun Angle to the Path of Solar Radiation

Figure 16.12

Page 15: Wednesday April  4,  2012

Relationship of Sun Angle and Solar Radiation Received

Figure 16.11

Page 16: Wednesday April  4,  2012

Earth - Sun Relationships

Figure 16.13

Page 17: Wednesday April  4,  2012

Daily Paths of the Sun at 40º N Latitude

Figure 16.10 A

Page 18: Wednesday April  4,  2012

Figure 16.10BDaily Paths of the Sun at 40º N Latitude

Page 19: Wednesday April  4,  2012

Daily Paths of the Sun at 40º N Latitude

Page 20: Wednesday April  4,  2012

Earth - Sun Relations Thus, the seasons are caused by Earth’s changing orientation to

the Sun throughout the year, and the fact that Earth’s axis is inclined 23½º, and the axis is always pointed in the same direction.

Here are some special days in the Northern Hemisphere:

At the Summer solstice (June 21–22), the Sun’s vertical rays are located at the Tropic of Cancer (23½º N latitude.)

At the Winter solstice (December 21–22), the Sun’s vertical rays are located at the Tropic of Capricorn (23½º S latitude.)

At the Autumnal equinox (September 22–23), the Sun’s vertical rays are located at the Equator (0º latitude.)

At the Spring (Vernal) equinox (March 21–22), the Sun’s vertical rays are located at the Equator (0º latitude.)

Page 21: Wednesday April  4,  2012

Characteristics of the Solstices and Equinoxes

Figure 16.14

Page 22: Wednesday April  4,  2012
Page 23: Wednesday April  4,  2012

Multiple exposures of the midnight Sun in late June or July in high northern latitudes.

Page 24: Wednesday April  4,  2012

Average monthly temperatures for

six cities located at different latitudes.

Note that Capetown, South

Africa, experiences winter in June,

July, and August.