The value of the constant is approximately 1 366 kilowatts per square metre.

The solar constant is measured at what altitude. Let s find a solution to that problem. The solar constant includes all types of solar radiation not just the visible light. The solar constant has been measured by the use of eppley normal incidence pyrhelio meters on three different days at 31 kilometers altitude. It is most accurately measured from satellites where atmospheric effects are absent.

The solar constant is not a physical constant in the modern codata scientific sense. The solar constant was directly measured from an altitude of about 82 kilometers apparently the first such determination. Then your difference is. The solar constant includes all types of solar radiation and not just the visible light.

Your solar constant 1376 1376 100 include your sign. Direct normal irradiance dni or beam radiation is measured at the surface of the earth at a given location with a surface element perpendicular to the sun. 5 it excludes diffuse solar radiation radiation that is scattered or reflected by atmospheric components. After correcting the readings for the remaining 1 of the atmosphere and earth sun distance a value of 1 912 gm cal cm 2 min has been determined for the solar constant.

The total solar intensity was 136 1 milliwatts per square centimeter or 1 952 calories per square centimeter per minute about 2 5 percent less than johnson s derived value. Energy in the ultraviolet and visible regions for λ less than 607 nanometers was 7 0 percent. The solar constant is a measure of flux density is the amount of incoming solar electromagnetic radiation per unit area that would be incident on a plane perpendicular to the rays at a distance of one astronomical unit au roughly the mean distance from the sun to earth. The solar constant is a flux density measuring mean solar electromagnetic radiation per unit area.

The solar radiation measured on high mountains can consequently be expected under all conditions to be lower than 1 89 0 04 1 85 cal cm 2 min. Solar constant the total radiation energy received from the sun per unit of time per unit of area on a theoretical surface perpendicular to the sun s rays and at earth s mean distance from the sun. 1 au 149 597 871 km. Multiply your uncorrected solar irradiation by 2 to correct for the glass and also by 1 4 to correct for the atmosphere.

It s not that complicated. The solar constant is a conventional measure of mean tsi at a distance of one astronomical unit au. The solar constant has to be measured at a distance of one astronomical unit.

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