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Dynamic pressure model derived from an observation by Sakigake for Comet Halley on 31 December, 1985An outstanding disconnection event (DE)-like knot was observed on 31 Dec. 1985 in P/Halley's tail. Analysis of the Sakigake/IMF data reveals that comet Halley did not encounter the heliospheric neutral sheet on the day, demanding a new explanation of the DE-like event. During this event, the comet encountered a high-speed solar wind from a coronal hole tongue of the Sun. The event can be explained by a dynamic pressure model, according to which the DE-like plasmoid was caused by a sudden increase in the dynamic pressure of the solar wind. A simulation result is found to support this interpretation. The dynamic pressure model for a comet can be compared with the mechanism of a possible geotail disturbance during a spacecraft triggered auroral substorm.
Document ID
19870017311
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Saito, Takao
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Yumoto, Kiyohumi
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Hirao, Kunio
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Saito, Keiji
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Nakagawa, Tomoko
(Onagawa Magnetic Observatory Japan)
Smith, Edward
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
September 5, 2013
Publication Date
December 1, 1986
Publication Information
Publication: ESA, Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 3: Posters
Subject Category
Astrophysics
Accession Number
87N26744
Distribution Limits
Public
Copyright
Other

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