lecture 2 Flashcards
Why do the sun and earth have different spectral properties? wavelength reflects intensity of energy flux
No atmosphere, straight exchange
Values of energy in and out in Wm-2
Planet emits longer wavelength radiation
Temperature of a radiating body definition
is a function of energy out (emissivity) and σ, the Stefan-Bolzmann contstant (5.67 x 10-8), and albedo
Temperature of earth with no atmosphere
-18oC
Abundant atmospheric gases (not GHGs)
Nitrogen, Oxygen and water vapour
GHG molecules, natural gases
Trace atmospheric gases
Co2, methane
Nitrous oxide, ozone
Unnatural gases
Halocarbons
Sulfa Hexafluoride Sf6
= human made and most potent and long lasting of the GHGs
Absorption capacity of atmosphere depends on
amount of each type of molecule present
absorption spectrum of each type of molecule
In order for the greenhouse effect to work what must be present in the atmosphere?
Greenhouse gases
Changing the atmospheric composition of greenhouse gases such as Co2 does what to the atmosphere?
Alters the atmosphere’s capacity to absorb and re-radiate energy
To balance the input and output of energy what is required?
heating of atmosphere and
Earth surface – a planet with atmosphere is
warmer than it would otherwise be
What affects energy pathways?
Albedo
Why is energy exchange usually measured at the top of the troposphere?
GHGs are active below tropopause and therefore lose energy at the top of the troposphere
What is the lapse rate of the troposphere?
warms and becomes denser towards the surface
The more molecules of GHG added, the more what?
interception and re-radiation
What is currently resultant of the ongoing process of adding GHGs and what does this mean?
Disequilibrium - heat loss from the upper troposphere is not keeping up with heat gain via increased GHGs