Extraterrestrial solar spectrum 360-1050 nm from Rotating Shadowband Spectroradiometer measurements at the Southern Great Plains (ARM) site

Details Extraterrestrial solar spectrum 360-1050 nm from Rotating Shadowband Spectroradiometer measurements at the Southern Great Plains (ARM) site Extraterrestrial solar spectrum 360-1050 nm from Rotating Shadowband Spectroradiometer measurements at the Southern Great Plains (ARM) site

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003jgrd..108.4424h&link_type=abstract

Journal of Geophysical Research Atmospheres, Volume 108, Issue D14, pp. ACL 8-1, CiteID 4424, DOI 10.1029/2001JD001311

Astronomy and Astrophysics

Astrophysics

3

Meteorology And Atmospheric Dynamics: Radiative Processes, Meteorology And Atmospheric Dynamics: Remote Sensing, Solar Physics, Astrophysics, And Astronomy: Solar Irradiance, Solar Physics, Astrophysics, And Astronomy: Instruments And Techniques

Scientific paper

Two years of Langley extrapolations made from the Southern Great Plains (SGP) site of the Atmospheric Radiation Measurement (ARM) Program using two very different RSS instruments and a NIST-derived irradiance scale show larger extraterrestrial solar irradiances in the 400 to 600 nm domain by as much as 4.5% compared to the Neckel and Labs [1984] data. Our results are more congruent with that of Thuillier et al. [1998a, 1998b] in this domain but do not show larger irradiances than the Neckel and Labs data at wavelengths less than 400 nm. In addition to the question of the true extraterrestrial solar spectrum, the data we present here are directly useful for the interpretation of spectral measurements calibrated with current National Institute of Standards and Technology (NIST) irradiance standards, for which we believe this represents the most extensive determination of the solar irradiance.

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