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Report from solar physicsA discussion of the nature of solar physics is followed by a brief review of recent advances in the field. These advances include: the first direct experimental confirmation of the central role played by thermonuclear processes in stars; the discovery that the 5-minute oscillations of the Sun are a global seismic phenomenon that can be used as a probe of the structure and dynamical behavior of the solar interior; the discovery that the solar magnetic field is subdivided into individual flux tubes with field strength exceeding 1000 gauss. Also covered was a science strategy for pure solar physics. Brief discussions are given of solar-terrestrial physics, solar/stellar relationships, and suggested space missions.
Document ID
19900009019
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Walker, A. B. C.
(Stanford Univ. CA., United States)
Acton, L.
(Lockheed Solar Observatory Palo Alto, CA., United States)
Brueckner, G.
(New Hampshire Univ. Durham., United States)
Chupp, E. L.
(Stanford Univ. CA, United States)
Hudson, H. S.
(Stanford Univ. CA, United States)
Roberts, W.
(San Jose State Univ. CA., United States)
Date Acquired
September 6, 2013
Publication Date
September 1, 1989
Publication Information
Publication: NASA, Marshall Space Flight Center, Solar-Terrestrial Science Strategy Workshop
Subject Category
Solar Physics
Accession Number
90N18335
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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