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Detailed Reference Information |
Tobiska, W.K., Pryor, W.R. and Ajello, J.M. (1997). Solar hydrogen Lyman-a variation during solar cycles 21 and 22. Geophysical Research Letters 24: doi: 10.1029/97GL00835. issn: 0094-8276. |
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A full-disk, line-integrated solar Lyman-&agr; dataset is presented that spans two solar cycles. The dataset is created partially from AE-E and SME data that is scaled to the Pioneer Venus Orbiter Ultraviolet Spectrometer (PVOUVS) upwind Lyman-&agr; sky background data which is converted to a solar surrogate. PVOUVS measurements overlap AE-E, SME, and UARS observing periods and are calibrated to UARS/SOLSTICE irradiance units at 1 AU. The scaled AE-E/SME, the SOLSTICE, and the PVOUVS surrogate data in the interim between the satellites collectively form a composite dataset with a quiet sun value of 3.0¿0.1¿1011 photons cm-2 s-1 common for three solar minima and a solar maximum value of 6.75¿0.25¿1011 photons cm-2 s-1 common to cycles 21 and 22.¿ 1997 American Geophysical Union |
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Abstract |
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Keywords
Solar Physics, Astrophysics, and Astronomy, Ultraviolet emissions, Ionosphere, Solar radiation and cosmic ray effects |
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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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