Atmosphere II : Climate Flashcards

1
Q

what is climate

A

average or typical conditions of the atmosphere

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2
Q

what are the most common components of climate

A

precipitation and temperature

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3
Q

define proxy measurement

A

A proxy is an indirect measure of the desired outcome which is itself strongly correlated to that outcome. It is commonly used when direct measures of the outcome are unobservable and/or unavailable.

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4
Q

what does climate average out

A

climate averages out weather, but not season

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5
Q

define paleoclimate

A

a climate prevalent at a particular time in the geological past.

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6
Q

do we only have current climate measurements

A

no we have climate measurements that span modern to past climates (paleoclimate)

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7
Q

what are the three ways that energy can be transferred

A

through radiation, conduction and convection

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8
Q

define radiation

A

transfer of energy as waves or particles through air (emission/transmission)

called electromagnetic radiation

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9
Q

what is the electromagnetic spectrum

A

range of frequencies of em radiation and their wavelengths (or energies)

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10
Q

how is the em spectrum seperated into 2

A

as longwave (low energy) and shortwave (high energy)

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11
Q

the energy of EM radiation is inversely proportional to what

A

wavelength

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12
Q

define conduction

A

heat(energy) transfer from one molecule to next as molecules vibrate

rate of transfer of heat depends on temperature difference (gradient)

e.g. heat moving along a metal bar

occurs in all phases, gas, liquid, solid

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13
Q

define convection

A

transfers of heat by movement of a fluid (mass transfer)

caused by buoyancy forces due to changes in density that arise from changes in temperature

set up convection cells - these present in the atmosphere as turbulence (fluid mixing) or an instability (uneven heating)

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14
Q

moist convection leads to…

A

thunderstorms

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15
Q

how do convection cells forms on oceans and land

A

at night landmass cools quicker than the ocean so creates a cell the other way compared to day time

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16
Q

how does convection lead to rainfall

A

When the land warms up, it heats the air above it. This causes the air to expand and rise. As the air rises it cools and condenses. If this process continues then rain will fall.

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17
Q

how does the sun transfer heat

A

by radiation

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18
Q

how does the ground transfer heat

A

the ground absorbs heat through by conduction, heat moves into atmosphere by radiation

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19
Q

how does the atmosphere transfer heat

A

convection

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20
Q

what is earths steady state theory

A

earths climate system, unperturbed, is in a (quasi-) steady state

energy in = energy out

incoming radiation = outgoing radiation

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21
Q

as space is a vacuum, the only form of energy transfer is:

A

em radiation

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22
Q

convection causes what type of cyclone

A

a low pressure cyclone

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23
Q

what is blackbody radiation

A

a perfect blackbody is an object that absorbs all incoming radiation (that is, none is reflected)

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24
Q

radiation emitted by a blacbody depends only what

A

its temperature

25
Q

what is plancks law about

A

plancks law of blackbody radiation defines the relationship how much radiation is emitted at a certain wavelength for a body of a certain temperature

26
Q

what is isotropic, what does it mean?

A

blackbody is isotropic (radiation emitted at equal intensity in all directions)

27
Q

what is radiance

A

power emitted by a blackbody (w/m^2/sr) sr = ser radian

28
Q

what is spectral radiance

A

radiance per unit frequency (w/m^2/sr/Hz)

29
Q

what waves are radiation from the sun

A

shortwave (UV/visible)

30
Q

radiation from the earth is…

A

longwave (infrared)

31
Q

the emission of radiation from the sun and earth…

A

hardly overlap

32
Q

what is the Stefan-Boltzmann law about

A

power radiated from a blackbody in terms of its temperature

33
Q

how to go from kelvin to degrees celsius

A

k = degree Celsius + 273.15k

34
Q

what is stefan-boltzmann law

A

total energy radiated per unit surface area of a blackbody is proportional to T^4

this relationship integrated in all directions over a hemisphere and over all frequencies is:

I = sigma x t^4
where sigma = 5.67 x 10^-8 wm^-2k^-4 is the stefan b constant

I = the blackbody irradiance or energy flux density

35
Q

what is a radiation modifier example

A

albedo and transmittance

36
Q

what is albedo

A

symbol alpha, a, it is the ratio of reflected radiation to incident radiation (incoming light striking a surface)

0 < a < 1

37
Q

what is transmittance

A

transmittance, gamma, y, is the ratio of transmitted radiation (radiation that passes through a fluid) to incident radiation:

0 < y < 1

38
Q

what is a grey body

A

a grey body is a body that emits according to plancks formula multiplied by fractional emissivity, epsilon, E

0 < E < 1

39
Q

tell me what the emissivity value means

A

where E is a measure of efficiency of emitting thermal radiation (0 for a shiny object, 1 for a blackbody)

40
Q

what is the global albedo

A

earth is not a perfect blackbody, clouds, ice, reflective land surfaces like deserts increase a and reduce E

earths colour varies from white to deep blue (nearly blue)

41
Q

what are the albedo properties of the earth

A

water = near perfect blackbody

snow = very reflective

albedo varies as a function of properties of surface (land/cloud)

the ocean albedo depends on the angle of the solar radiation striking the surface (sun glint)

the albedo of bare sea ice depends on the density of the air bubbles

earths global average = 0.3

42
Q

tell me about the global mean energy model (incoming radiation)

A

energy of incident shortwave solar radiation (solar constant) S(subscript 0) = 1366 w/m^2

s0 = incident solar radiation

43
Q

how do we calculate the global mean energy model (outgoing radiation)

A

energy of sun incident on earth = epsilon s0 /4

area of the earth the sun intercepts = pi x r^2

fraction of solar constant received by earth = pir^2/4pir^2 = s0/4 = 342 w/m^2

E = 1 - alpha = 0.7

44
Q

how can we integrate global mean temperature and the energy of a blackbody

A

the energy of blackbody is proportional to its temperature

E(out) = sigma x t^4

45
Q

tell me about the penetration of radiation on the atmosphere

A

majority of shortwave penetrates the atmosphere, very little longwave escapes

46
Q

what are the natural greenhouse gases:

A

water vapour, co2, oxygen and ozone, methane, nitrous oxide

47
Q

what is the chemical symbol for methane

A

methane = CH4

48
Q

what is the chemical symbol for nitrous oxie

49
Q

what is the grey atmosphere

A

gray atmoshpere is transparent in shortwave and includes a layer of infrared absorbing gases that intercept outgoing longwave radiation

50
Q

tell me about uneven heat in the world and its redistribution

A

equator gets more sun radiation than the poles, uneven heating.

redistribution of heat:
convection plays a role
not as simple as Hadleys 1735 suggestion that convection cell extends from equator to the poles

redistribution does not account for coriolis effect

51
Q

tell me about tropical Hadley cells

A

sun heats equator
hot air rises
air masses move towards poles
air masses diverge from north-south path due to coriolis effect
cool dry air sinks at about 30 degree latitude (deserts)
still named hadley cell

52
Q

air rising (convective uplift) is associated with…

A

clouds and rain (tropical rainforests)

53
Q

air sinking (subsidence) associated with…

A

dry air (deserts)

54
Q

tell me about convective cells

A

moist, warm air rises forming clouds

cold, dry air subsides (compresses and warms)

55
Q

tell me about surface winds bestie

A

descending branch of cell reaches surfaces, forms surface winds that diverge due to Coriolis effect
poleward and equatorward winds meet, air forced upward, maintains convective cells.

56
Q

tell me about annual mean surface temperature

A

warmest at the equator
coldest at the poles
Antarctic colder than arctic (isolated less land mass to redistribute head)

colder at elevation

canada colder than europe

57
Q

where does rain occur

A

most rain in intertropical convergence zone (ITCZ) (convective uplift)

little rain at edge of tropics ~ 30 degrees north (subsidence)

more rain over equatorial oceans = storm tracks

58
Q

why are circulation patterns not always stable

A
seasonal variation
interannual variability 
north atlantic oscillation 
el-nino southern oscillation
extreme weather 
longer-timescale variability (not the focus of this module)
59
Q

tell me about earths seasons

A

earth is tilted at an angle of 23.5 from its orbital plane

different parts of the earth receive the suns most direct rays

when north pole tilts toward the sun, it is summer in the northern hemisphere

when south pole tilts toward the sun, its winter in the northern hemisphere