module 2

mod 2

solar energy

insolation: measured in units of watts per square meter therefore varies by latitude and by season

a = as if overhead - insolation at its greatest

b = slanted - same energy spread over larger area

responsible for long shadows in midlatitude summers

insolation varies with the sun’s passage in the sky (ex. passage of the sun at the equator)

equinoxes - at noon the sun is directly overhead

solstices - at noon the sun is at an angle

(ex. passage of the sun at mid latitudes)

equinoxes - at noon the sun is 50 degrees above horizon

solstices - june solstice has a higher angle; december the angle is lower

daily insolation

poleward of artic/antarctic circles, sun is below horizon for part of year

daily insolation at its maximum at the pole during summer solstice

two maxima and two minima in daily isolation at the equator occurring at the equinoxes and solstices respectively

insolation

49% = direct radiation (radiation that goes directly to earth’s surface)

31% = reflected back to space (3% by scatter, 19% by clouds, 9% by ground)

20% = absorbed by atmosphere (3% by clouds, 17% by dust and gases)

22% = scattered by atmosphere (eventually get to earth’s surface as diffuse radiation)

in theory, this could affect the climate (ex: more snow, higher albedo, less energy reaches surface, temp decreases, more snow = ice albedo feedback effect)

radiation balance

in comparison to how much radiation we get, the earth is warmer than it should be

bc it’s harder for longwave radiation to leave, the earth is warmed, longwave is absorbed by gases in the atmosphere

the greenhouse effect

greenhouse gases include carbon dioxide, ozone, water vapor, methane, CFCs

they absorb longwave and then re-radiate it to the surface (counter-radiation)

the earth is warmer (by 35 deg. C or 63 deg. F) than it would be without these gases

this is the greenhouse effect

net radiation

difference between incoming and outgoing radiation

at high latitudes, there is an energy deficit

poleward heat transfer moves surplus energy from low to high latitudes

world latitude zones

globe divided into broad latitude zones that we use to describe climatic and other geographic zones

composition of the atmosphere in the troposhere

constant gases

nitrogen 78% (converted by bacteria in a useful form in soils) oxygen 21% (produced by green plants in photosynthesis and used in respiration)

argon ~1% (inert)

variable gases in the atmosphere

carbon dioxide 0.035% (used by green plants in photosynthesis and produced by respiration, burning of fossil fuels)

gaseous water 0.1-4%

methane (produced by cows, termites, swamps, etc.)

CFCs (entirely human made gas)

dust and particulates (from pollen, sea-salt, volcanic dust, soil, etc.)

the earth’s atmosphere

atmosphere = gaseous envelope surrounding the earth

made up of a series of concentric layers

atmosphere is held down by gravity

most of the atmosphere’s mass is near the surface

structure and science of the atmosphere

the atmosphere consists of several layers with different temperatures, pressures, and compositions

troposphere: warmed by greenhouse gases

stratosphere: warmed by chemicals absorbing light, including ozone & UV

ozone: in the stratosphere, forms the layer, absorbs ultraviolet radiation

mesosphere: atmosphere less dense and gets colder

thermosphere: chemicals highly excited by sunlight

heat balance

sensible heat: heat you can sense (measure using a thermometer)

latent heat: heat used in the evaporation of water or liberated in condensation (cannot be measured by a thermometer)

latent heat transfer: transfers heat from an evaporating surface to the atmosphere

solar energy losses in the atmosphere

shortwave energy absorbed or diverted in different ways

UV absorbed by ozone

scattering produces diffuse radiation

clouds reflect radiation back to space (and also absorb radiation)

counter radiation

surface is also warmed by longwave radiation emitted by the atmosphere

  1. surface emits radiation that goes directly to space

  2. but most is absorbed by the atmosphere

  3. atmosphere emits radiation that goes directly to space

  4. but also radiates energy back to the surface

albedo

radiative energy can either be absorbed (heating) or reflected (no heating)

percentage of solar radiation reflected = albedo

fresh snow = 85-95%

dry sand = 35-40%

tropical forest = ~13%

earth’s albedo = ~30%

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