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Detailed Reference Information |
Burlaga, L.F. (1988). Magnetic clouds and force-free fields with constant alpha. Journal of Geophysical Research 93: doi: 10.1029/88JA01200. issn: 0148-0227. |
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Magnetic clouds observed at 1 AU are modeled as cylindrically symmetric, constant alpha force-free magnetic fields. The model satisfactorily explains the types of variations of the magnetic field direction that are observed as a magnetic cloud moves past a spacecraft in terms of the possible orientations of the axis of a magnetic cloud. The model also explains why the magnetic field strength is observed to be higher inside a magnetic cloud than near its boundaries. However, the model predicts that the magnetic field strength profile should be symmetric with respect to the axis of the magnetic cloud, whereas observations show that this is not generally the case. ¿ American Geophysical Union 1988 |
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Abstract |
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Keywords
Interplanetary Physics, Solar wind plasma, Interplanetary Physics, Interplanetary magnetic fields |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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