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Insolation at Specified Location

This web page produces a numerical table of sunrise, sunset, daily insolation at top of atmosphere, and sunlight-weighted cosine of the zenith angle at a single specified location. The produced table contains data for a single month, or if a month is not provided, data for a single calendar year. Latitude and longitude must be given in degrees and hundredths of degrees, not degrees and minutes. Default location is the Central Park weather station, New York City.
Enter latitude: in degrees. North latitude is positive, south latitude is negative.
Enter longitude: in degrees. East longitude is positive, west longitude is negative.
Enter year: A.D.
Enter numerical month:
As explained in the file SRERROR.TXT, the Atmosphere-Ocean Model assumes that the Sun is a point source. The columns for daily insolation and zenith angle in the produced table continue to use this assumption. The maximum error for this assumption occurs at the poles during the equinoxes where the table's algorithm would indicate no insolation but in reality there should be about x.xx (W/mē). The columns for sunrise and sunset, however, do consider the radius of the Sun's disk as seen from the Earth (0.267° on average) and atmospheric refraction of sunlight (approximately 0.583° on the horizon). The table should be accurate to within one minute. During equinoxes, points on the equator see about 12 hours and 7 minutes of daylight. The 7 minutes are due to the radius of the Sun's disk and atmospheric refraction.

SRLOCAT.FOR is the Fortran source code of the program used on this web page.


GEN INFO LINE PLOTS MODEL DATA UNIX MODEL CODE PEOPLE SUNLIGHT
STATISTICS COLOR PLOTS OBSERVA PC MODEL DOC PUBLICA TIDES and MOON

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Curator: Gary L. Russell . . . . . 2008/02/08/18:10:54