Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...123...25l&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 123, no. 1, June 1983, p. 25-28.
Astronomy and Astrophysics
Astronomy
Comet Tails, Comets, Plasma Interactions, Solar Wind, Helios 2, Ion Density (Concentration), Magnetohydrodynamic Stability, Particle Acceleration, Solar Flares, Comets, Bradfield 1979X, Comet Tails, Plasma, Observations, Data, Ions, Solar Wind, Astronomy, Helios 2, Velocity, Density, Hydrodynamics, Temperature
Scientific paper
The tail event observed by Brandt et al. (1980) in comet Bradfield 1979 X on 1980 February 6 is shown to be due to an interplanetary solar wind disturbance detected aboard Helios 2 and on Earth. Helios 2 was at 0.15 AU from the comet. The tail follows the bulk direction of the solar wind. Acceleration of cometary ions seems to result from small scale hydrodynamic instabilities. Cometary ion density and temperature are deduced.
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