Physics
Scientific paper
Jun 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987georl..14..644r&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 14, June 1987, p. 644-647. BMFWF-supported research.
Physics
84
Cometary Atmospheres, Cometary Magnetospheres, Halley'S Comet, Magnetohydrodynamic Stability, Magnetospheres, Magnetospheric Instability, Satellite Observation, Magnetic Flux, Magnetic Measurement, Magnetosheath, Plasma Dynamics, Vega Project, Comets, Halley, Stability, Magnetosphere, Vega Missions, Temperature, Magnetosheath, Magnetic Properties, Ions, Concentration, Features, Plasma, Spacecraft Observations, Analysis, Plasmag Instrument
Scientific paper
High resolution Vega 1 and 2 magnetic measurements in the cometary magnetosphere and magnetosheath of Halley reveal the presence of fluctuations with the signature expected for the mirror instability. This instability is a mechanism by which homogeneously produced cometary ions with a large perpendicular temperature anisotropy can be concentrated into discrete linear features. Thus, the mirror instability may provide a new mechanism for the generation of cometary rays. To our knowledge the presence of this instability in the cometary plasma was not predicted.
Riedler Willi
Russell Christopher T.
Schwingenschuh Konrad
Yeroshenko Ye.
No associations
LandOfFree
Mirror instability in the magnetosphere of 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 Mirror instability in the magnetosphere of Comet Halley, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mirror instability in the magnetosphere of Comet Halley will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1817621