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タイトルDoppler Measurements of the Suns Meridional Flow
本文(外部サイト)http://hdl.handle.net/2060/19970022597
著者(英)Hathaway, David H.
著者所属(英)NASA Marshall Space Flight Center
発行日1996-04-01
言語eng
内容記述Doppler velocity data obtained with the Global Oscillation Network Group (GONG) instruments in Tucson from 1992 August through 1995 April were analyzed to determine the structure and evolution of the Sun's meridional flow. Individual measurements of the flow were derived from line-of-sight velocity images averaged over 17 minutes to remove the p-mode oscillation signal. Typical flow velocities are poleward at approximately 20 m/s, but the results suggest that episodes may occur with much stronger flows. Such variations may help to explain some of the many disparate reports on the strength and structure of the Sun's meridional flow.
NASA分類Solar Physics
レポートNO97N23111
NAS 1.15:112496
NASA-TM-112496
権利Copyright, Distribution as joint owner in the copyright
URIhttps://repository.exst.jaxa.jp/dspace/handle/a-is/101336


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