- Incoming Solar Radiation - Solar Radiation intercepted at the
surface of the earth.
- Amount and intensity are determined by the sun angle, day length, path
length, ground slope, and state of the atmosphere.
- Sun Angle - angle a beam of light
makes with the
surface of the earth.
- Sun angle determines the area of illuminated and intensity of
heating.
Perpendicular rays (A) concentrate energy over the smallest area. As
the sun angle decreases (B) the area illuminated increases (indicated by dashed line).
- The tilt of the earth's axis determines the sun angle.
- The earth's axis of rotation is inclined 23 1/2 degrees from perpendicular.
- Earth's axis is tilted 66 1/2 degrees from the plane of the ecliptic - the plane the earth orbits the sun in.
- Parallelism means that the earth's axis remains parallel to
its former position as it revolves around the sun.
- Axis "always" points in the same direction.
Subsolar point -
location where the sun is directly overhead at noon. Similar
to declination of the sun.
- Influences local sun angle. Slopes tipped into the sun have higher
sun angles and hence more intense insolation than horizontal or slopes tipped away
from the sun.
- As the distance over which incoming solar radiation increases, greater chance for
diffusion and reflection of light.
- Earth - sun distance is greatest in July, closest in January.

Due to the curvature of the earth, path length
of a beam of light is longer at high latitudes
State of the Atmosphere
-
Elliptical Orbit of the earth around the sun
-
Furthest from the sun in July, closest in January (Do you know why it's warmer in the
summer in the Northern Hemisphere even though the earth is further away?)
Go to Earth Orbit animation

Orientation of Earth to Sun
Axial Tilt, Earth Orientation and Day length
 |
The circle of illumination is the division between day and night over
the earth. The circle of illumination bisects (cuts in half) all latitudes on the spring
and autumnal equinoxes. At this time, all places have equal day length (12 hours). The
circle of illumination always bisects the equator (0 degrees latitude). |
Animation of
day light period through the year (Warning: 3 MB file; long
download)
| |
JUNE SOLSTICE |
SEPTEMBER EQUINOX |
DECEMBER SOLSTICE |
MARCH EQUINOX |
Date |
June 22 |
Sept. 23 |
December 22 |
March 21 |
|
Earth
Orientation to Sun |
North pole
tilted toward sun |
Neither pole tilted
toward sun |
South pole
tilted toward sun |
Neither pole tilted
toward sun
|
Subsolar Point |
23 1/2 degrees N |
Equator
(0 degrees) |
23 1/2 degrees S |
Equator
(0 degrees) |
Tangent Rays |
Arctic and Antarctic Circles |
North and South Poles |
Arctic and Antarctic Circles |
North and South Poles |
Day
length |
24 hours of darkness at South Pole; 24 hours day light
at North Pole; 12 hours day light at Equator |
12 hour day length everywhere |
24 hours of darkness at North Pole; 24
hours day light at South Pole; 12 hours day light at Equator |
12 hour day length everywhere |
Continue
to Radiation
and Energy Balance
|