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Exercises for Weather and Climate 8th Edition Greg Carbone Solutions Manual
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Solutions Manual to
Exercises for Weather & Climate, 8th ed.
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Appendix A
Appendix B
Appendix C
Vertical Structure of the Atmosphere
EarthโSun Geometry
4
The Surface Energy Budget
8
The Global Energy Budget
10
Atmospheric Moisture
12
Saturation and Atmospheric Stability
Cloud Droplets and Raindrops
Atmospheric Motion
21
Weather Map Analysis
28
Mid-Latitude Cyclones
33
Weather Forecasting
19
37
Thunderstorms and Tornadoes
Hurricanes
43
46
Climate Controls
1
50
Climate Classification
53
Climatic Variability and Change
Simulating Climatic Change
Dimensions and Units
Earth Measures 62
GeoClock 63
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1
1.
Vertical Structure of the Atmosphere
Height (km)
22.4
16.8
11.2
5.6
% of atmosphere above
6.25
12.5
25
50
Height Above the Surface (km)
2. & 3.
34
32
30
28
26
24
22
20
18
16
14
12
10
8
6
4
2
0
2
3
0 10 20 30 40 50 60 70 80 90 100
Percentage of the Atmosphere Above
0 100 200 300 400 500 600 700 800 900 1000
4.
25%
58.4%
5.
210 mb
6.
123 mb
69 mb
Pressure (mb)
250 mb
584 mb
58.4%
33%
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7. Ozone absorbs solar radiation (particularly in the ultraviolet portion of the electromagnetic spectrum). This absorption leads to warming in the stratosphere.
8.
2000
2.0ยฐC
4000
โ11ยฐC
6000
โ24ยฐC
8000
โ37ยฐC
10000
โ50ยฐC
9. & 11.
20000
Key West
18000
Fairbanks
16000
standard atmosphere
14000
12000
10000
8000
6000
4000
2000
0
-80
10. a. Key West
-60
-40
-20
b. Key West
0
20
40
c. Fairbanks
11. See 9 above.
12. Key West tropopause: ~16,000 m, ~ โ75ยฐC; Fairbanks tropopause: ~10,000 m, ~ โ53ยฐC;
13. The greater the average temperature, the higher the tropopause. Our example suggests that vertical
mixing is greater when temperature is warmer.
14. 170 mb
15. 92 mb
16. Because of greater air density in the lower layer, the pressure drop between 2 and 4 km is nearly
double that between 8 and 10 km.
17. 182 mb
18. Air pressure decreases with height because there is less atmosphere to exert downward force. The
pressure drop will be greatest when air density is highest because the mass of the atmosphere above
decreases at a faster rate.
19. California desert: 1003.9 mb; Michigan UP: 1018.6 mb; New Brunswick: 1003.7 mb.
20. The Michigan and New Orleans stations have the same pressure (1018.6 mb), but a 30ยฐF temperature difference. The New Brunswick and southern California stations have similar low pressures
(1003.7 mb and 1003.9 mb), but a 30ยฐF temperature difference.
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21. The ideal gas law shows that pressure is proportional to the product of density times temperature.
Therefore, to have a similar pressure, but be 30ยฐF warmer, New Orleans must have a lower density.
22. The Michigan and New Brunswick stations have higher air density than the other two.
Review Questions
1. Air pressure and density decrease exponentially with height above Earthโs surface. This is because
gas molecules are concentrated near the surface and a given height increase at these lower levels means
passing through more molecules than the same height increase at higher elevations. Temperature also
decreases with height in the troposphere. This rate of decrease varies, but is typically linear compared to
pressure or density.
2. The thickness of the troposphere is a function of temperature. Warmer temperatures in tropical
regions create mixing to greater depths, pushing the tropopause higher.
3. The higher its relative density, the more likely air is to sink. Density is influenced by temperature
and pressure. At the low pressure of the mid and upper troposphere, density is lower than it is at lower
elevations.
4. Pressure changes much faster vertically than it does horizontally. It drops 100 mb in the lowest
kilometer of the atmosphere.
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2
1.
EarthโSun Geometry
N
June 21
23ยฝยฐ
66ยฝยฐ
30ยฐ
D 90ยฐ
A
0ยฐ
Sunโs Rays
231/2ยฐ
B
C
D
S
831โ2ห
47ห
43ห
661โ2ห
1 2ห
66 โ N
30ห N
0ห
231โ2ห S
A
B
C
D
June 21 profile view
March 21
90ยฐ
66ยฝยฐ
A
30ยฐ
B
Sunโs Rays
0ยฐ
C
D
23ยฝยฐ
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231โ2ห
661โ2ห N
60ห
30ห N
A
B
661โ2ห
90ห
0ห
231โ2ห S
C
D
March 21 profile view
2.
631โ2ยฐ; December 21
3.
261โ2ยฐ
4.
a. 0ยฐ (equator)
b. 231โ2ยฐ N
c. 0ยฐ (equator)
d. 231โ2ยฐ S
e. [variable]
5.
a.
b.
c.
d.
e.
6.
New Orleans
60ยฐ
831โ2ยฐ
60ยฐ
361โ2ยฐ
[variable]
Helsinki
30ยฐ
531โ2ยฐ
30ยฐ
61โ2ยฐ
[variable]
[variable]
7. Answer is date dependent. Example for 34ยฐ N latitude on February 1, a two-meter pole casts a
shadow measuring 2.52 meters.
tan ฮ =
(length of pole)
(length of shadow)
ฮ = tanโ1 (0.7937)
ฮ = 38.44ยฐ
8.
[variable]
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9.
60ยฐ N Dec. 22
Sun angle 6.5ยฐ
Sunโs rays
1 unit
Zenith angle
83.5ยฐ
8.83 units
30ยฐ N June 21
60ยฐ N June 21
Sunโs rays
Sunโs rays
1 unit
1 unit
Zenith angle
6.5ยฐ
Zenith angle
36.5ยฐ
Sun angle
53.5ยฐ
Sun angle
83.5ยฐ
1.24 units
1.01 units
10. Summer temperature is highest because solar radiation is more concentrated. During the winter,
itโs cooler as the solar beam is spread over a greater surface area.
11. There is a much greater seasonal range in daylight hours in polar regions than in tropical regions.
12.
30ยฐ N
June solstice
14
Equinoxes
12
December solstice 10
60ยฐ N
18
12
6
13. 60ยฐ N
14. The change in daylight hours is greatest near the equinoxes (when solar declination changes are
greatest) and smallest near the solstices.
15. a. At 30ยฐ N, the sun rises due east and sets due west on the equinoxes. Between the March and
September equinoxes, it rises slightly north of east and sets slightly north of west. Between the
September and March equinoxes, it rises slightly south of east and sets slightly south of west.
b. The same general pattern is found at 60ยฐ N, but it is more extreme. In fact, the figure shows that
on the June solstice the sun rises just north of NE (45ยฐ) and sets just north of NW (315ยฐ N). On the
December solstice, the sun rises just south of SE (135ยฐ) and sets just south of SW (225ยฐ).
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Exercises for Weather and Climate 8th Edition Greg Carbone Solutions Manual
Full Download: http://testbanklive.com/download/exercises-for-weather-and-climate-8th-edition-greg-carbone-solutions-manual/
16. March 21: 500 Wmโ2
June 21: 349 Wmโ2
September 22: 500 Wmโ2
December 22: 658 Wmโ2
17. The seasonal difference in solar intensity (beam spreading) and daylight hours is greater at 60ยฐ N
than at 30ยฐ N.
18. The difference in beam spreading between 60ยฐ N and 30ยฐ N is greater in winter. Furthermore, 60ยฐ
N has a shorter daylight period than 30ยฐ N in winter, while in summer the daylight hours are actually
greater at 60ยฐ N.
19. [variable}
20. Most direct rays: 1 unit beam = 1.000 surface units; Date March 21, September 22
Least direct rays: 1 unit beam = 1.090 surface units; Date June 21, December 21
21. 9%
22. [variable]
23. [variable]
24. The higher the latitude, the greater the seasonal range in solar intensity. This results in a larger
annual temperature range at high latitudes than in the tropics.
25.
60ยฐ N
50ยฐ N
40ยฐ N
30ยฐ N
20ยฐ N
December Solstice June Solstice
8.834
1.244
3.521
1.117
2.241
1.043
1.681
1.006
1.379
1.002
26. The solar intensity gradient across the mid-latitudes is much greater in winter and contributes to a
greater temperature gradient.
Review Questions
1. A given change at low sun angles is much more effective than the same change at higher sun angles.
Therefore, the seasonal shift of sun angle from 36.5ยฐ to 83.5ยฐ at New Orleans results in less change in
solar intensity than the shift from 6.5ยฐ to 53.5ยฐ at Helsinki.
2. A greater range in solar intensity and daylight hours will result in a greater range in solar radiation
received and temperature.
7
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