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Solar cycle study of interplanetary Lyman-alpha variations - Pioneer Venus Orbiter sky background resultsPVO observations of the interplanetary Ly-alpha (IPL) background, obtained over an entire solar cycle (SC) from 1979 to 1985, are compiled and analyzed statistically, along with data from other instruments and earlier solar cycles. The results are presented in extensive tables and graphs and characterized in detail. Findings reported include SC variation of 1.8 for the longitudinally averaged IPL intensity (in agreement with the variation of the 27-d disk-averaged integrated solar Ly-alpha flux), yearly averaged ecliptic H-atom lifetime at 1 AU equal to 1.0 Ms at solar minimum and 1.5 Ms at solar maximum, interplanetary H density equal to 0.07 + or - 0.01/cu cm, and interplanetary H/He within the heliopause but far from the sun of 7 + or - 3.
Document ID
19870057371
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Ajello, J. M.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Stewart, A. I.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Thomas, G. E.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Graps, A.
(Colorado, University Boulder, United States)
Date Acquired
August 13, 2013
Publication Date
June 15, 1987
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 317
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
87A44645
Distribution Limits
Public
Copyright
Other

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