Influence of a solar active region on the interplanetary magnetic field |
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| Authors: | Kenneth H. Schatten Norman F. Ness John M. Wilcox |
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| Affiliation: | (1) Space Sciences Laboratory, University of California, Berkeley, Calif., U.S.A.;(2) NASA Goddard Space Flight Center, Greenbelt, Md., U.S.A.;(3) Space Sciences Laboratory, University of California, Berkeley, Calif., U.S.A. |
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| Abstract: | ![]()
The interplanetary magnetic field has been mapped between 0.4 and 1.2 AU in the ecliptic plane, extrapolating from satellite measurements at 1 AU. The structure within sectors and the evolution of sectors are discussed. The development of a solar active region appears to produce magnetic loops in the interplanetary medium that result in the formation of a new sector. |
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