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Interplanetary space - A new laboratory for rarefied gas dynamicsInterplanetary space provides simultaneously the best vacuum available to man and, because of the solar wind, a tenuous and unsteady high-speed outflow of predominantly hydrogen gas from the sun, a remarkable variety of rarefied gasdynamics phenomena to observe. This paper provides a review of these phenomena, and of the way in which the present level of understanding has been achieved.
Document ID
19740060842
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Spreiter, J. R.
(Stanford University Stanford, Calif., United States)
Rizzi, A. W.
(NASA Ames Research Center Computational Fluid Dynamics Branch, Moffett Field, Calif., United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1974
Subject Category
Space Sciences
Meeting Information
Meeting: International Symposium on Rarefied Gas Dynamics
Location: Stanford, CA
Start Date: July 10, 1972
End Date: July 14, 1972
Accession Number
74A43592
Funding Number(s)
CONTRACT_GRANT: NSF GA-37691
CONTRACT_GRANT: NGR-05-020-330
Distribution Limits
Public
Copyright
Other

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