论文信息 - K corona and magnetic sector boundaries

K corona and magnetic sector boundaries

Solar white-light intensity maxima form a characteristic spatial pattern at the solar root of an interplanetary sector boundary, different for +/− and for −/+ boundaries. At a sector boundary, interplanetary magnetic polarities correspond to solar follower fields in the ascending part of the solar activity cycle and to leader fields in the decline.

C. Sawyer | R. Hansen | S. Hansen

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