this year's (2007) winter solstice was on 22 dec... so happy winter solstice!!!
on winter solstice...
- the earth is close to the sun: 147,098,074 km5
- for locations on the tropic of capricorn, the sun appears to be directly overhead at noon
- for locations on the antarctic circle, the sun will set at midnight
- for locations bellow the antarctic circle, the sun will not set
i was having a huge argument with my cus about the two solstices...
he claimed that the earth's orbit around the sun was near circular and hence there is no significant change in the amount of incident solar radiation

for a local area (like a city)... the significant factor that causes seasonal temperature changes is the earth's tilt in relation to the orbital plane... but if you take the northern hemisphere and the southern hemisphere... the southern gets more solar radiation during its summer than what the northern hemisphere would get during its summer... by a significant 6.5% more! if we were in the equator, december would be warmer than july...
readings made from satellites have shown that the solar constant4 varies between 1399 W/m2 to 1310 W/m21... wikipedia claims these values to be 1412 W/m2 to 1321 W/m22... solar constant varies with time because the sun follows a cycle... there are years when the sun is hotter than normal and there are times when its cooler than normal...
so these measured values have a difference of about 6.5%
1- (1310/1399) = 6.36%
and 1- (1321/1412) = 6.44%
we know that the power intensity density (radiation flux or power per unit area) of the sun follows a inverse square law
solar constant GS is given by1,7...
(4πL2) . GS = (4πr2)σTS4
where TS is the black body radiation temperature of the sun, TS = 5762 K or 6035°C and L is the distance between the sun and earth
earth's orbits around the sun is elliptical... with a aphelion of 152,097,701 km and perihelion of 147,098,074 km3
so the difference in solar constants is proportional to L2
147,098,074/152,097,701 = 0.967
the difference of L2 is the square of the above value which is 0.935
so there is a difference of 1-0.935 which is 6.5% between the solar constant during summer solstice and winter solstice!
if you're still confused here is the math
(4πL2) . GS = (4πr2)σTS4
GS = (r2/L2)σTS4
during summer solstice GS, summer = (r2/Lsummer2)σTS4
during winter solstice GS, winter = (r2/L winter 2)σTS4
GS, summer/GS, winter = Lwinter2 / Lsummer2
GS, summer/GS, winter = (147,098,074/152,097,701)2 = 0.9672 = 0.935
so the percentage change is (1-0.935) x 100% = 6.5%
and this corresponds to the measured values of GS, winter / GS, summer which is 6.36% (or 6.44%)
notes
- Yunus A Cengel: Hear Transfer - A Practical Approach - 2002 edition
- Wikipedia: Solar Radiation
- Wikipedia: Earth
- read my prev blog post on summer solstice
- Wikipedia: Solar Constant
- Nasa: Moon Phases
- Nasa: JPL Solar System Simulator
- Nasa: Solar Radiation and the Earth System
may be i should convince marissaj to write a musical about winter solstice!!!
oh btw... although it was poya yesterday (23rd)... full moon falls today (24th) (according to nasa5 that is)
