The Origin of Quasistationary Gas Flow from Solar Active Regions. I.

Details The Origin of Quasistationary Gas Flow from Solar Active Regions. I. The Origin of Quasistationary Gas Flow from Solar Active Regions. I.

Jun 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967sva....10..899m&link_type=gif

Soviet Astronomy, Vol. 10, p.899

Astronomy and Astrophysics

Astronomy

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