Cometary ray closing rates - Comet Kobayashi-Berger-Milon

Details Cometary ray closing rates - Comet Kobayashi-Berger-Milon Cometary ray closing rates - Comet Kobayashi-Berger-Milon

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...247..247m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 247, no. 1, July 1991, p. 247-251. Research supported by NASA and New Mexico I

Astronomy and Astrophysics

Astrophysics

2

Comet Tails, Interplanetary Medium, Solar Wind, Interplanetary Magnetic Fields, Space Plasmas

Scientific paper

Cometary ray closing rates are measured for a sequence of a dozen plates of Comet Kobayashi-Berger-Milon (1975 IX) on July 31, 1975. The angular velocity is a factor of three to six higher than previously published in the literature for other comets. A deceleration of one to two deg/hr-squared, with no secular trend, is measured. Comparisons are made between these observations and some existing models.

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