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タイトルSolar Seismology from Space. a Conference at Snowmass, Colorado
本文(外部サイト)http://hdl.handle.net/2060/19850016749
著者(英)Rhodes, E. J., Jr.; Ulrich, R. K.; Harvey, J.; Toomre, J.
著者所属(英)Jet Propulsion Lab., California Inst. of Tech.
発行日1984-12-15
言語eng
内容記述The quality of the ground based observing environment suffers from several degrading factors: diurnal interruptions and thermal variations, atmospheric seeing and transparency fluctuations and adverse weather interruptions are among the chief difficulties. The limited fraction of the solar surface observable from only one vantage point is also a potential limitation to the quality of the data available without going to space. Primary conference goals were to discuss in depth the scientific return from current observations and analyses of solar oscillations, to discuss the instrumental and site requirements for realizing the full potential of the seismic analysis method, and to help bring new workers into the field by collecting and summarizing the key background theory. At the conclusion of the conference there was a clear consensus that ground based observation would not be able to provide data of the quality required to permit a substantial analysis of the solar convection zone dynamics or to permit a full deduction of the solar interior structure.
NASA分類SOLAR PHYSICS
レポートNO85N25060
JPL-PUB-84-84
NASA-CR-175661
NAS 1.26:175661
権利No Copyright


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