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Streamer Brightness BoundaryFlow tubes adjacent to closed magnetic field lines on the boundaries of streamers can have spreading factors which change rapidly with height. Numerical models in this thin layer are subject to uncertainties. Here we use an analytic model of magnetically closed and adjacent open regions to analyze the spreading factor close to the closed field lines. The model is based on the one-temperature, isothermal flow model of Pneuman (1968), extended to calculate spreading factors and plasma beta, and to better explain streamer evolution with increasing temperature.
Document ID
20000010646
Acquisition Source
Marshall Space Flight Center
Document Type
Abstract
Authors
Suess, S. T.
(NASA Marshall Space Flight Center Huntsville, AL United States)
Nerney, S.
(Ohio Univ. Lancaster, OH United States)
Date Acquired
August 19, 2013
Publication Date
September 11, 1999
Publication Information
Publisher: European Space Agency
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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