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Detailed Reference Information |
Judge, D.L., McMullin, D.R. and Ogawa, H.S. (1999). Absolute solar 30.4 nm flux from sounding rocket observations during the solar cycle 23 minimum. Journal of Geophysical Research 104: doi: 10.1029/1999JA900314. issn: 0148-0227. |
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A transmission grating extreme ultraviolet (EUV) spectrometer, nominally identical to the Charge, Element, and Isotope Analysis System/Solar EUV Monitor (CELIAS/SEM) instrument on the Solar and Heliospheric Observatory (SOHO), has obtained accurate measurements of the integrated absolute solar extreme ultraviolet irradiance in an 8 nm band pass centered at 30.4 nm. The spectrometer also measured the EUV/soft X-ray flux, but those data will be reported in a later paper. The instrument was launched on two sounding rocket flights from White Sands Missile Range, New Mexico, on June 26, 1996, and again on August 11, 1997, to provide a SOHO underflight calibration database in the EUV. The full disk solar 30.4¿40 nm fluxes measured by it on the above 2 days were 1.21¿1010 and 1.42¿1010 photons cm-2 s-1 at 1 AU, respectively. These measurements have an absolute 1&sgr; uncertainty of 8.1%. ¿ 1999 American Geophysical Union |
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BACKGROUND DATA FILES |
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Abstract![](/images/icons/spacer.gif) |
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Keywords
Solar Physics, Astrophysics, and Astronomy, Solar irradiance, Solar Physics, Astrophysics, and Astronomy, Ultraviolet emissions, Solar Physics, Astrophysics, and Astronomy, X rays, gamma rays, and neutrinos, Solar Physics, Astrophysics, and Astronomy, Instruments and techniques |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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