Lecture 2 Flashcards

Earth's Energy Budget (32 cards)

1
Q

weather

A

state of atmosphere at any given time and place

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2
Q

climate

A

average state of climate over some given time interval

typically 30 year weather “normals”

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3
Q

habitable zone

goldilock’s zone

A
  • sweet spot that allows for evolution of complex life
  • strongly controlled by distance from star
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4
Q

stars

A

astral body that emits different wavelengths of EMR

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5
Q

our sun emits…

A

mostly visible light (50%), some as infrared and longwave (40%), and the rest as UV or shortwave (10%)

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6
Q

wavelengths

A

peak to peak

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7
Q

frequency

A

how many waves in a given amount of time (waves/second)

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8
Q

light is measured in ____, and what are they

A

photons
- tiny balls of energy
- smallest amount of discrete energy transported by an EM wave

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9
Q

solar insolation

A

amount of energy passing through a given area over a given amount of time

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10
Q

flux

A

amount of energy (# of photons) in an EM wave passing through a ceratin area/time

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11
Q

solar flux is ____ at the poles because…

A

lower bc there is more area

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12
Q

flux is dependent on …

A

distance from sun and angle of incidence

inverse square law means distance plays even bigger role

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13
Q

eccentricity

A

elliptical orbit
- controls amount of solar insolation received
- 413000 years

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14
Q

precession

A

wobble
- 24000 years

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15
Q

obliquity

A

tilt
- 41000

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16
Q

blackbody

A

ideal absorber and emitter in all wavelengths
- 100% efficiency
- doesn’t actually exist
- but most objects behave similarly

energy in = energy out

17
Q

Planck’s Law

A

relationship between intensity of radiation flux from a blackbody and its wavelength or frequency

18
Q

Wiens law

A

states rad flux from a blackbody reaches its peak at a max wavelength inverse to its absolute temp

the hotter the object, the shorter the wavelength

19
Q

what explains why the sun is yellow

20
Q

stefan-boltzman law

A

energy flux emitted by a bb is proportional to abs temp ^4

the hotter it is, 4x more flux

21
Q

first law of thermodynamics

A

law of conservation of energy
- when in equilibrium, earth is emitting to space the same amount it is absorbing from sun

22
Q

emissivity

A

thermal radiation emitted from a body’s surface vs the radiation emitted from an ideal blackbody surface at the same temperature

0-1, 1 = perfect emission, perfect blackbody

23
Q

Earth’s energy budget controlled by …

A

incoming/outgoing radiance
- temp of and distance from sun/
- radiated energy and earth’s albedo

24
Q

energy emitted equation

A

stefan-boltzman law and area of a sphere

25
energy absorbed equation
energy intercepted - energy reflected area of a circle and solar constant and 1-albedo
26
important difference between energy absorbed and emitted equations
one uses area of a circle one uses area of a sphere ## Footnote all of earth emits at once, but only half receives sun at once
27
cause of discrepancy between what earth temp should be and what it is
greenhouse gases :) ## Footnote the atmosphere
28
surface temp controlled by
○ Solar constant ○ Number of layers in the atmosphere ○ The albedo
29
One layer atmosphere
○ Transparent to incoming shortwave ○ Opaque to outgoing infrared ○ Behaves like a blackbody (emits what it absorbs) ○ Energy outwards goes to space and energy down is re-absorbed - Calculation is too hot
30
N layer model
The more layers we have, the higher the temperature goes - But each layer produces less warming than the last
31
high clouds emit ___ and reflect ___
less, less ## Footnote warming effect, high and cold wispy clouds don't emit or reflect well
32
low clouds emit ____ and reflect ____
more, more ## Footnote cooling effect, big warm fluffly clouds emit and reflect well