I have a question for any of the physicists that roam these boards.
How much energy in joules hits the earth at the equator on a day to day basis?
any help would be greatly appreciated.
Question regarding the earths energy.
Moderator: Alyrium Denryle
- Wyrm
- Jedi Council Member
- Posts: 2206
- Joined: 2005-09-02 01:10pm
- Location: In the sand, pooping hallucinogenic goodness.
D'ya mean solar energy?
Darth Wong on Strollers vs. Assholes: "There were days when I wished that my stroller had weapons on it."
wilfulton on Bible genetics: "If two screaming lunatics copulate in front of another screaming lunatic, the result will be yet another screaming lunatic. "
SirNitram: "The nation of France is a theory, not a fact. It should therefore be approached with an open mind, and critically debated and considered."
Cornivore! | BAN-WATCH CANE: XVII | WWJDFAKB? - What Would Jesus Do... For a Klondike Bar? | Evil Bayesian Conspiracy
wilfulton on Bible genetics: "If two screaming lunatics copulate in front of another screaming lunatic, the result will be yet another screaming lunatic. "
SirNitram: "The nation of France is a theory, not a fact. It should therefore be approached with an open mind, and critically debated and considered."
Cornivore! | BAN-WATCH CANE: XVII | WWJDFAKB? - What Would Jesus Do... For a Klondike Bar? | Evil Bayesian Conspiracy
- Kuroneko
- Jedi Council Member
- Posts: 2469
- Joined: 2003-03-13 03:10am
- Location: Fréchet space
- Contact:
The Sun's luminosity is P = 3.827e26W, with a distance of AU = 149597870691m, the incident radiation for a surface normal is I = P/(4πAU²) = 1.361e3W/m². As per Lambert's law, the intensity is I(θ) = [I/2][cos θ], where θ is the angle of incidence. Since the ecliptic is at 23.5°relative to the equator, the intensity of at the equator at high noon is S = 1.248e3W/m², without adjusting for atmospheric albedo or absorption. One can apply Lambert's law again to adjust for the varying angle of incidence throughout the day, but there's an easier way. Since the equatorial radius is R = 6378135m, a band of thickness δ<<R and length 2R will have incident energy 2δSR, but since this energy is spread throughout the whole band, a δ-long piece will have only δ/(2πR) of it, so that the average power on the is δ²S/π = 397.2W if δ = 1m. Over a twenty-four hour period, this makes 3.43e7J. Again, this is before adjusting for atmospheric reflection and absorption, but since I'm unsure of those parameters, I'll simply guesstimate 2.9-3.4eJ.
Note on Edit: I'm not sure what my addled mind was thinking yesterday, but that factor of 1/2 on the Lambert's cosine law should not be there (I think I was compensating for night, nevermind that this way it would have been done twice). Hence, the figures should be doubled to 3.44e7J per twenty-four hours. How much the atmosphere affects this depends on the ('average') weather conditions, obviously, but I still have no data regarding that.
Note on Edit: I'm not sure what my addled mind was thinking yesterday, but that factor of 1/2 on the Lambert's cosine law should not be there (I think I was compensating for night, nevermind that this way it would have been done twice). Hence, the figures should be doubled to 3.44e7J per twenty-four hours. How much the atmosphere affects this depends on the ('average') weather conditions, obviously, but I still have no data regarding that.
Last edited by Kuroneko on 2006-01-01 12:23pm, edited 1 time in total.