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Solar wind interaction with Comet Bennett /1969i/.Examination of the relations between the solar-wind and Comet Bennett during the period from Mar. 23 to Apr. 5, 1970. A large kink was observed in the ion tail of the comet on April 4, but no solar-wind stream was observed in the ecliptic plane which could have caused the kink. Thus, either there was no correlation between the solar wind at the earth and that at Comet Bennett (which was 40 deg above the ecliptic) or the kink was caused by something other than a high-speed stream. The fine structure visible in photographs of the kink favors the second of these alternatives. It is shown that a shock probably passed through Comet Bennett on March 31, but no effect was seen in photographs of the comet. A stream preceded by another shock and a large abrupt change in momentum flux might have intercepted the comet between March 24 and March 28, but again no effect was seen in photographs of the Comet.
Document ID
19730056699
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Burlaga, L. F.
Donn, B.
(NASA Goddard Space Flight Center Laboratory for Extraterrestrial Physics, Greenbelt, Md., United States)
Neugebauer, M.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Rahe, J.
Date Acquired
August 7, 2013
Publication Date
May 1, 1973
Publication Information
Publication: Solar Physics
Volume: 30
Subject Category
Space Radiation
Accession Number
73A41501
Funding Number(s)
CONTRACT_GRANT: NGL-21-002-033
Distribution Limits
Public
Copyright
Other

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