- Latitude lines, or parallels, divide the earth from east
to west; Longitude lines, or meridians, divide the earth from north
to south.
- We assume that the rays of the sun are all parallel.
- Insolation is the amount of radiation received at surface.
- Equinox: equal day, equal night; sun over
the equator.
- Soltice: the sun is furthest from the equator. 23½°
N is the Tropic of Cancer; 23½° S is the Tropic of
Capricorn.
Vernal equinox | March 21 |
Summer solstice | June 21 |
Autumnal equinox | September 21 |
Winter solstice | December 21 |
- The path of the earth's orbit around the sun is elliptical.
Its nearest point in January is 91 million miles away and is
called the perihelion (near sun). Its farthest point in
July is 96 million miles and called the aphelion.
- During the aphelion the earth travels the slowest, while during
the perihelion, the earth travels fastest.
- The amount of insolation varies with season and latitude.
- Averaged, the northern and southern hemispheres receive the
same amount of insolation each year as proved by Alexander von
Humboldt, despite the variations in earth-sun distance.
- There is about a one month lag between the longest day and the
warmest day (or shortest and coldest days). This is caused by
the temperature responding to the balance of incoming and outgoing
radiation.
- The onset of spring warming season is delayed because of the energy needed
to first melt the snow and ice.
- The basic cause of the weather is that the poles are cold and
the equator is warm (due to angle of incidence) and the atmos-
phere attempts to find a balance.