Publikationsdatum:
2011-08-19
Beschreibung:
Stationary MHD models are used to analyze the data of magnetic field measurements in Comets Giacobini-Zinner and Halley. The contributions of the draping, of changes in the IMF, and of turbulence are separated and extended patches of unidirectional field regions are identified. A time-dependent MHD simulation of the nonstationary flow following a sudden 90 deg rotation in the IMF describes properly the disrupted tail condensations observed from the earth.
Schlagwort(e):
ASTROPHYSICS
Materialart:
Advances in Space Research (ISSN 0273-1177); 9; 3, 19
Format:
text
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