Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jgr....9820995h&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 98, no. A12, p. 20,995-21,002
Astronomy and Astrophysics
Astronomy
18
Astronomical Models, Grigg-Skjellerup Comet, Molecular Ions, Plasma Diffusion, Plasma-Particle Interactions, Solar Wind Velocity, Spaceborne Astronomy, Water, Giotto Mission, Gyrofrequency, Heavy Ions, Ion Density (Concentration), Ion Injection, Mathematical Models, Solar Wind
Scientific paper
We compare model predictions of cometary water group ion densities and the solar wind slow down with measurements made by the Giotto Johnstone plasma analyzer implanted ion sensor at the encounter with comet Grigg-Skjellerup (G-S) on July 10, 1992. The observed slope of the ion density profile on approach to the comet is unexpectedly steep. Possible explanations for this are discussed. We present also a preliminary investigation of the quasilinear velocity-space diffusion of the implanted heavy ion population at G-S using a transport equation including souce, convection, adiabatic compression, and velocity diffusion terms. Resulting distributions are anisotropic, in agreement with observations. We consider theoretically the waves that may be generated by the diffusion process for the observed solar wind conditions. At initial ion injections, waves are generated at omega approximately Omegai the ion gyrofrequency, and lower frequencies are predicted for diffusion toward a bispherical shell.
Coates Andrew J.
Huddleston D. E.
Johnstone Alan D.
Neubauer Fritz Manfred
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