Climate Science ATS 201

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26 Terms

1
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How does Earth exchange energy with outer space?

Radiation

2
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True or False: Everything with a temperature radiates energy

True

3
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Where does solar radiation peak in the spectrum?

Visible light

4
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What is radiative flux?

The rate that energy flows across a plane

5
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What are the units of radiative flux?

Watts per square meter (W/m²)

6
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When does global mean temperature change occur?

When energy input is different from energy output

7
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What is the inverse square law?

Radiative flux decreases with the square of distance from the source

8
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Inverse square law equation

Flux = Power / (4πr²)

9
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What happens to flux if distance is doubled?

It decreases by a factor of 4

10
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Why does doubling distance reduce flux by a factor of 4?

The surface area over which energy spreads increases by 4

11
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How does solar radiative flux vary among planets?

It decreases with increasing distance from the Sun

12
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What is a blackbody?

An ideal object that absorbs and emits 100% of radiation at all wavelengths

13
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Why are blackbodies important in climate models?

Earth’s emission can be approximated as blackbody radiation

14
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How does temperature affect blackbody radiation wavelength?

Hotter objects emit shorter wavelengths; cooler objects emit longer wavelengths

15
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Which law relates peak wavelength to temperature?

Wien’s Law

16
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Wien’s Law equation

λmax (μm) = 2900 / T (K)

17
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What units must wavelength be in for Wien’s Law?

Microns (μm)

18
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Approximate temperature of the Sun using Wien’s Law

~5800 K

19
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Which law relates emitted flux to temperature?

Stefan-Boltzmann Law

20
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Stefan-Boltzmann Law equation

F = σT⁴

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What is the Stefan-Boltzmann constant (σ)?

5.67 × 10⁻⁸ W m⁻² K⁻⁴

22
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Does blackbody size affect emitted flux?

No, flux depends only on temperature

23
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Does blackbody size affect total power emitted?

Yes

24
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If temperature increases from 100 K to 300 K, how does flux change?

Increases by a factor of 81

25
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Which star is hotter: blue or red?

Blue

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