Physics
Scientific paper
Dec 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.250a.291k&link_type=abstract
In ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 1: Plasma and Gas p 291-295 (SEE N87
Physics
1
Electron Energy, Electrons, Flux (Rate), Halley'S Comet, Energy Spectra, Giotto Mission, Magnetic Measurement, Particle Acceleration, Radiation Counters
Scientific paper
The Energetic Particle Detector system EPA/EPONA onboard Giotto detects ions and electrons with energies greater than 20 keV in various energy channels. In this paper, electron fluxes are presented together with data from the Giotto Magnetometer Experiment. Electrons >180 keV were recorded from the transit of the foreshock, inbound, until the last observation outbound at approximately 03:00 UT on 15 March 1986. Energy spectra for the inbound pass are shown. One flux enhancement in the >300 keV channel and several in the >180 keV channel were recorded outbound. Possible acceleration mechanisms for the energetic electrons are considered.
Kirsch E.
McKenna-Lawlor Susan
Neubauer Fritz Manfred
Osullivan D.
Thompson Abigail
No associations
LandOfFree
Energetic electron fluxes (E180 KeV) observed by the Giotto experiment EPA during encounter with Comet Halley does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Energetic electron fluxes (E180 KeV) observed by the Giotto experiment EPA during encounter with Comet Halley, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Energetic electron fluxes (E180 KeV) observed by the Giotto experiment EPA during encounter with Comet Halley will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1122405