Volume 389, Number 3, July III 2002
|Page(s)||1039 - 1046|
|Section||Celestial mechanics and astrometry|
|Published online||01 July 2002|
Large-scale disturbance of the solar wind by a comet
Max-Planck-Institut für Astrophysik, 85748 Garching, Germany
Corresponding author: email@example.com
Accepted: 26 March 2002
Model calculations for the interaction of the solar wind with a comet are presented that extend 30 million km into the tail. It is shown that the disturbance of the interplanetary magnetic field (IMF) (the draping) is limited to timescales of 10 to 50 hours and length scales of 10 to 50 million km. This is supported by a theoretical argument about the acceleration of the cometary ions. The distribution of ions and protons at the end of the model tails agrees with measurements made by Ulysses far in the tail of comet Hyakutake. It is shown that the ion tail is concentrated in the current sheet between two flux lobes as long as the draping persists. The far tail, however, is flat and concentrated in a plane parallel to the IMF.
Key words: comets: general / Sun: solar wind
© ESO, 2002
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