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Saturday, August 1, 2020 | History

2 edition of Normal incident solar radiation measurements at Upton, New York found in the catalog.

Normal incident solar radiation measurements at Upton, New York

J. G. Cottingham

Normal incident solar radiation measurements at Upton, New York

by J. G. Cottingham

  • 191 Want to read
  • 15 Currently reading

Published by Dept. of Energy, [Office of Energy Research], Brookhaven National Laboratory, Accelerator Dept., for sale by the National Technical Information Service] in Upton, N.Y, [Springfield, Va .
Written in English

    Subjects:
  • Solar radiation -- New York (State) -- Upton -- Measurement.

  • Edition Notes

    StatementJ. G. Cottingham.
    SeriesBNL ; 50939, BNL (Series) -- 50939.
    ContributionsBrookhaven National Laboratory. Accelerator Dept., United States. Dept. of Energy. Office of Energy Research.
    The Physical Object
    Paginationiii, 12 p. :
    Number of Pages12
    ID Numbers
    Open LibraryOL17649885M

      Normal and Horizontal Solar Radiation - Convertion weather from EPW to BIN; Weather Processor; Variation in incident solar radiation on east and west surface of a building in different simulation tool; Fwd: Variation in incident solar radiation on east and west surface of . A variety of critical energy measurements, from power generated to incident solar radiation to ambient air and heat transfer fluid temperatures, are monitored by the FST solution and made available to users and owner/operators in a real-time web view.

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Normal incident solar radiation measurements at Upton, New York by J. G. Cottingham Download PDF EPUB FB2

Get this from a library. Normal incident solar radiation measurements at Upton, New York. [J G Cottingham; Brookhaven National Laboratory. Accelerator Department.; United States. Department of Energy. Office of Energy Research.].

Normal incident solar energy measurements made at Upton, L.I., New York are reported and analyzed relative to the total energy received on a horizontal surface. A method for computing normal incident solar radiation is developed and used to study long term variations in this energy source at Upton and to estimate average values for other east coast locations.

Author: J.G. Cottingham. Solar irradiance is the power per unit area (watt per square metre, W/m 2), received from the Sun in the form of electromagnetic radiation as reported in the wavelength range of the measuring instrument. Solar irradiance is often integrated over a given time period in order to report the radiant energy emitted into the surrounding environment (joule per square metre, J/m 2), during that time.

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Century Edinburgh, Scotland September 15–16, National Renewable Energy File Size: KB. Extraterrestrial Solar Radiation: Insolation is the incident solar radiation and it is measured as power per unit area (units W/m²). Solar constant at a mean distance from earth to sun is defined as the amount of solar radiation falling on surface normal to the sun rays outside the atmosphere of the earth.

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– 14). @article{osti_, title = {Comparison of model estimated and measured direct-normal solar irradiance}, author = {Halthore, R N and Schwartz, S E and Michalsky, J J and Anderson, G P and Ferrare, R A and Holben, B N and Ten Brink, H M}, abstractNote = {Direct-normal solar irradiance (DNSI), the energy in the solar spectrum incident in unit.

Chapter 2 Solar Radiation Measurements Solar Radiation Components at the Ground Level In a point at the top of Earth’s atmosphere, the beam of nearly parallel incident sunrays is referred to as extraterrestrial radiation (ETR). ETR fluctuates about % during a year (from Wm-2 in January to Wm-2 in July) dueFile Size: KB.

Radiation levels surged 17 times higher than normal this week near the Chernobyl nuclear power station in Ukraine, as forest fires tore through the disaster area, officials said. 13/55 Radiative flux density out of atmosphere solar radiative flux incident on area unit perpendicular to direction of propagation changes during the year, variable distance Sun-Earth (eliptic orbit) change of distance 1,7 %, change of flux 3,3 % value for mean distance Sun-Earth solar constant G sc = W/m2 (value from WRC, 1 %) original measurements Ch.

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