NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
A two-fluid model of the solar windA method is presented for the integration of the two-fluid solar-wind equations which is applicable to a wide variety of coronal base densities and temperatures. The method involves proton heat conduction, and may be applied to coronal base conditions for which subsonic-supersonic solar wind solutions exist.
Document ID
19930049573
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Sandbaek, O.
(NASA Headquarters Washington, DC United States)
Leer, E.
(Oslo Univ. Norway)
Holzer, T. E.
(High Altitude Observatory Boulder, CO, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1992
Publication Information
Publication: In: Solar Wind Seven; Proceedings of the 3rd COSPAR Colloquium, Goslar, Germany, Sept. 16-20, 1991 (A93-33554 13-92)
Publisher: Pergamon Press
Subject Category
Solar Physics
Accession Number
93A33570
Funding Number(s)
CONTRACT_GRANT: NASA ORDER W-17016
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available