On Possible Existence of Elongated Magnetical Structure in Circumsolar Space

Details On Possible Existence of Elongated Magnetical Structure in Circumsolar Space On Possible Existence of Elongated Magnetical Structure in Circumsolar Space

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988atsir1526...17v&link_type=abstract

Astronomicheskii Tsirkulyar NO.1526/FEB, P. 17, 1988

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The proton events, observed from "Prognoz-8" and connected with the flares of April 28 and 30, 1981 were analyzed. The temporal profiles of proton flux were characterized by discrete structure, and from bursts' duration the total sizes of the magnetic structure (L = 3.5×106km) and characteristic sizes of the fine structure (L = 25 - 30×103km) were evaluated.

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