An interplanetary disturbance relevant to the tail-turning of comet Bradfield (1979l) on 1980 February 6

Physics

Scientific paper

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Comet Tails, Interplanetary Medium, Solar Flares, Solar Wind Velocity, Scintillation, Space Plasmas

Scientific paper

Solar-wind data obtained with spacecraft and interplanetary-scintillation observations in early February 1980 are examined in order to determine large-scale propagation properties of a proposed interplanetary disturbance relevant to a very rapid 10-deg turning of the plasma-tail axis of comet Bradfield (1979l) on February, 6, 1980. It is shown that a solar-flare-associated interplanetary disturbance having an oblate configuration was responsible for the tail event.

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