1. DAILY INSOLATION OVER THE YEAR AT VARIOUS LATITUDES (NORTH HEMISPHERE)

2. SOLAR DECLINATION (δ): the latitude at which the Sun is directly overhead at solar noon (estimated from the analemma)
-the left axis tells you your declination
-as you follow the analemma, you’ll notice that long dashes indicate the beginning/end of a month
-small dashes indicate a labeled date (e.g. Dec 15)
-once you find the date of interest, look to the left axis for δ

3. What would happen if the Earth had no tilt?
What would happen in Newark if the Earth was tilted 40°?

4. SOLAR AND EARTH RADIATION
ELECTROMAGNETIC RADIATION:
It’s a kind of energy
All objects emit electromagnetic radiation
It’s a collection of waves traveling away from the surface of the objects
Short waves (warmer temperatures)
More energy
TEMPERATURE
Long waves (cooler temperatures)
Less energy

5. In general, the higher the temperature of an object the greater the amount of total energy emitted by that object (Stefan-Boltzman Law)
Earth Temp: 6000 K (5727 C)
Sun Temp: 288 K (15 C)
σ = 5.67 X 10-8 Wm-2K-4

6. Solar radiation wavelength range 0.2 – 2.0 micrometers
Shortwave radiation
Tsun= 5798 K ≈ 6000 K
Terrestrial radiation wavelength range 4 – 25 micrometers
Longwave radiation
Tearth = 288 K ≈ 255 K

7. SOLAR CONSTANT
The amount of solar radiation striking the top of earth’s atmosphere, which is constant (theoretically):
1372 W/m2 7

8. SOLAR RADIATION (short wave radiation, SWR)
INCOMING LWR
As solar radiation passes through
the atmosphere, is affected by absoption
and reflection
Absorption:
Molecules and particles in the atmosphere
intercept and absorb radiation
(oxygen and ozone)
Reflection:
Solar radiation passing through the
Atmosphere can be reflected
Albedo: An important property of a surface. It measures how much solar energy will be reflected:
A surface with high albedo (snow, ice) reflects most of the solar radiation
A surface with low albedo (black pavement) absorbs most of incoming solar radiation 8

9. Albedo: reflectivity of the surface to the solar radiation
ESTIMATION OF ALBEDO
Albedo: reflectivity of the surface to the solar radiation

10. LONG WAVE RADIATION (LWR)
INCOMING LWR
The solar energy is absorbed by the atmosphere, land or ocean and raises the temperature
The atmosphere, land and ocean also emit energy in the form of long wave radiation 10

11. Incoming LWR: Counterradiation
The Earth’s surface emits energy to the atmosphere that is absorbed by the atmosphere and radiated back down to Earth’s surface

12. NET RADIATION (RADIATION BUDGET)
It is the difference between total upward and downward radiation fluxes and is a
measure of the energy available at the ground surface.
R = INPUT – OUTPUT
R = ( SWR + LWR) – ( SWR + LWR)
INCOMING LWR

13. WHY IS NET RADIATION IMPORTANT?
Net radiation is the energy available at the earth’s surface to drive climate and life processes (evaporation, air temperature, photosynthesis)