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Hot ions observed by the Giotto ion mass spectrometer inside the Comet Halley contact surfaceJust inside the contact surface (approx. 4700 km) the High Energy Range Spectrometer (HERS) sensor of the Giotto ion mass spectrometer detected a sudden, intense burst of ions that lasted until the HERS sensor ceased transmitting data at a distance 3000 km from comet Halley. During this interval ions with M/Q=1, 2, 12, 14, 16, 19, 24 and 28 were observed. The heavier ions appear in two populations (in the S/C frame): a very low energy, almost omnidirectional distribution, and a more energetic (approx. < ram speed) population coming from the ram direction. The low energy ions may belong to the natural Halley environment or be generated at the spacecraft by dust and gas bombardment. The ions may also be related to spacecraft charging processes on Giotto.
Document ID
19870015742
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Goldstein, R.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Young, D. T.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Balsiger, H.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Buehler, F.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Goldstein, B. E.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Neugebauer, M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Rosenbauer, H.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Schwenn, R.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Shelly, E. G.
(Lockheed Aircraft Corp. Palo Alto, Calif., 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 1: Plasma and Gas
Subject Category
Astrophysics
Accession Number
87N25175
Distribution Limits
Public
Copyright
Other

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