Flare physics in solar activity maximum 22 : proceedings of the International Solar-A Science Meeting held at Tokyo, Japan, 23-26 October 1990 : dedicated to the memory of the late professor K. Tanaka / Y. Uchida [and others], eds.
By: International Solar-A Science Meeting (1990 : Tokyo, Japan)
Contributor(s): Tanaka, Katsuo | Uchida, Y. (Yutaka)
Material type: 
TextSeries: Lecture notes in physics: 387.Publisher: Berlin ; New York : Springer-Verlag, ©1991Description: 1 online resource (x, 360 pages) : illustrationsContent type: text Media type: computer Carrier type: online resourceISBN: 9783540475965; 3540475966Subject(s): Solar activity -- Congresses | Solar flares -- Congresses | Astrophysics -- Congresses | Astronautics in astronomy -- Congresses | Astronautics in astronomy | Astrophysics | Solar activity | Solar flares | Tokio <1990>Genre/Form: Electronic books. | Conference papers and proceedings. | Kongress. Additional physical formats: Print version:International Solar-A Science Meeting (1990 : Tokyo, Japan).: Flare physics in solar activity maximum 22.DDC classification: 523.7/5 LOC classification: QB524 | .I593 1990Online resources: Click here to access online Action note: digitized 2010 committed to preserveSummary: The book reviews the knowledge obtained from ground-based and space-borne solar flare research thus at the same time preparing for the forthcoming mission of the satellite Solar A which will be launched in 1991. Accordinglyone section is devoted to experiments on Solar A. The rest review both theory and observational facts to give a physically realistic picture of flares, including problems of magnetic flux emergence, high energy particles in flares, heating and flows in flares, and further problems of solar activity.
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Includes bibliographical references.
The book reviews the knowledge obtained from ground-based and space-borne solar flare research thus at the same time preparing for the forthcoming mission of the satellite Solar A which will be launched in 1991. Accordinglyone section is devoted to experiments on Solar A. The rest review both theory and observational facts to give a physically realistic picture of flares, including problems of magnetic flux emergence, high energy particles in flares, heating and flows in flares, and further problems of solar activity.
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