radiation balance
DESCRIPTION
RADIATION BALANCE. MET 2101 CLIMATOLOGY. RADIATION BALANCE. What Happens to the Solar Beams? What Affects Radiation?. ULTRA VIOLET. VISIBLE. INFRARED. SOLAR BEAM IN THE UPPER ATMOSPHERE (STRATOSPHERE). UV. VIS. IR. Much UV Absorbed by Ozone. - PowerPoint PPT PresentationTRANSCRIPT
RADIATION BALANCE
MET 2101
CLIMATOLOGY
RADIATION BALANCERADIATION BALANCE
What Happensto the SolarBeams?
What Affects Radiation?
VISIBLE
INFRARED
ULTRA VIOLET
UVMuch UV
Absorbed byOzone
SOLAR BEAM IN THE UPPER ATMOSPHERE SOLAR BEAM IN THE UPPER ATMOSPHERE (STRATOSPHERE)(STRATOSPHERE)
VIS
IR
Visible & IR Pass through Ozone with little attenuation
SOLAR BEAM IN THE TROPOSPHERE
The remaining energy goes several places:
Reflected
Sur
fac
e
Reflected Absorbed
Scattered
Clo
ud sAbsorbed
Radiation reaching clouds
Clear Sky Radiation
Solar Radiation Reaching
Troposphere
Dire ctD
iffu
se
Diff
us
e
About 98% of the solar beam passes through the Stratosphere to the Troposphere
On average somewhat more than half passes through clear skies; the rest encounters clouds
The solar radiation is absorbed and scattered by the atmosphere.
It is indirectly reflected by clouds or transmitted to the surface
Radiation scattered by the atmosphere or clouds, but still reaching the surface is called DIFFUSE RADIATION
It hits the surface from all directions
The radiation that passes through without scattering (DIRECT RADIATION) is partially reflected by the surface
Diffuse radiation is not reflected by surface.
Surface Heats Up with Radiation
Thermal IR emitted from heated surface (land & water)
Surface Heats Up with Radiation
Thermal IR increases with daylight
Thermal IR gradually absorbed by clouds and atmosphere
Clouds also reflect part of Thermal IR back down
Radiation Budget in Percent of Solar Input Energy