Incoming short-wave solar radiation (light) at top of atmosphere: 7 million calories per square meter per day, averaged for the Earth as a whole 100% 100% Outgoing radiation Light (short-wave radiation), 30% Infrared (long-wave) radiation, 70% = 100% Space 100% 6% 20% 4% 6% 38% 26% Atmosphere Emission by clouds Backscattered Net emission by water vapor, CO2 16% by air Absorbed by water vapor, Reflected by clouds dust, CO2 15% Absorption by water vapor, Co2 Absorbed 3% by clouds Net surface Absorbed by water and land Reflected by water and land surface Latent heat emission of Sensible heat long-wave radiation 51% 21% 7% 23% Figure 8.5 An estimate of the heat budget for Earth. On an average day, about half of the solar energy arriv- ing at the upper atmosphere is absorbed at Earths surface. Light (short-wave) energy absorbed at the surface is converted into heat. Heat leaves Earth as infrared (long-wave) radiation. Since input equals output over long periods of time, the heat budget is balanced. B ujweajabebuag o

Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
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How do you think our present period of global warming relates to Earth’s overall heat budget?

Incoming short-wave solar radiation (light) at top of atmosphere: 7 million
calories per square meter per day, averaged for the Earth as a whole
100%
100%
Outgoing radiation
Light (short-wave radiation), 30%
Infrared (long-wave) radiation, 70%
= 100%
Space
100%
6%
20%
4%
6%
38%
26%
Atmosphere
Emission by
clouds
Backscattered
Net emission by
water vapor,
CO2
16%
by air
Absorbed by
water vapor,
Reflected
by clouds
dust, CO2
15%
Absorption by
water vapor,
Co2
Absorbed
3%
by clouds
Net surface
Absorbed
by water
and land
Reflected by water
and land surface
Latent
heat
emission of
Sensible
heat
long-wave radiation
51%
21%
7%
23%
Figure 8.5 An estimate of the heat budget for Earth. On an average day, about half of the solar energy arriv-
ing at the upper atmosphere is absorbed at Earths surface. Light (short-wave) energy absorbed at the surface
is converted into heat. Heat leaves Earth as infrared (long-wave) radiation. Since input equals output over long
periods of time, the heat budget is balanced.
B ujweajabebuag o
Transcribed Image Text:Incoming short-wave solar radiation (light) at top of atmosphere: 7 million calories per square meter per day, averaged for the Earth as a whole 100% 100% Outgoing radiation Light (short-wave radiation), 30% Infrared (long-wave) radiation, 70% = 100% Space 100% 6% 20% 4% 6% 38% 26% Atmosphere Emission by clouds Backscattered Net emission by water vapor, CO2 16% by air Absorbed by water vapor, Reflected by clouds dust, CO2 15% Absorption by water vapor, Co2 Absorbed 3% by clouds Net surface Absorbed by water and land Reflected by water and land surface Latent heat emission of Sensible heat long-wave radiation 51% 21% 7% 23% Figure 8.5 An estimate of the heat budget for Earth. On an average day, about half of the solar energy arriv- ing at the upper atmosphere is absorbed at Earths surface. Light (short-wave) energy absorbed at the surface is converted into heat. Heat leaves Earth as infrared (long-wave) radiation. Since input equals output over long periods of time, the heat budget is balanced. B ujweajabebuag o
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