NDLI: Current sheet magnetic model for the solar corona

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Current sheet magnetic model for the solar corona

Content Provider	NASA Technical Reports Server (NTRS)
Author	Schatten, K. H.
Copyright Year	1972
Description	A new magnetic model is developed and compared with previous models and the observed solar corona. An attempt is made to more accurately compute the three-dimensional currents flowing in the solar corona. Physical reasons are given that require most of the large scale currents flowing in the solar corona to lie near thin sheets. The current sheets are not constrained into any particular geometry or symmetry as in the previous models of Altschuler and Newkirk (1969) and Schatten et al. (1969). A comparison with the axisymmetric, isothermal MHD solution of Pneuman and Kopp (1970) suggests that the model is able to simulate to high accuracy an isothermal corona. A comparison of the model with the May 30, 1965, solar eclipse and the November 12, 1966, solar eclipse shows the model is capable of computing many features including the polar plume orientations as well as radial and nonradial streamers in the solar corona.
File Size	3194053
Page Count	11
File Format	PDF
Alternate Webpage(s)	http://archive.org/details/NASA_NTRS_Archive_19730002037
Archival Resource Key	ark:/13960/t50g8f41p
Language	English
Publisher Date	1972-01-01
Access Restriction	Open
Subject Keyword	Space Radiation Solar Eclipses Solar Corona Magnetohydrodynamics Current Sheets Three Dimensional Flow Solar Physics Mathematical Models Solar Magnetic Field Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science
Content Type	Text
Resource Type	Article

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