Physics
Scientific paper
Jun 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981giot.proc....3s&link_type=abstract
In ESA Sci. and Exptl. Aspects of the Giotto Mission p 3-7 (SEE N82-14107 05-12)
Physics
Astronomical Models, Cometary Atmospheres, Magnetic Fields, Magnetohydrodynamic Flow, Solar Wind, Three Dimensional Flow, Bow Waves, Comet Tails, Field Theory (Physics), Interplanetary Magnetic Fields, Magnetic Effects, Shock Waves
Scientific paper
Plasma flow and field amplification, resulting from the interaction of the solar wind with a comet, are studied by model calculations for the rates G = 7 X 10 to the 26 power to 2 X 10 to the 30 power of total cometary gas production. The influence of the magnetic field is investigated, using an axisymmetric model. A three-dimensional magnetohydrodynamic calculation shows how the magnetic field induces an asymmetry. A sudden change of direction in the interplanetary field produces streamer-like structures.
Schmidt Hans-Ulrich
Wegmann Rudolf
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