Other
Scientific paper
Jan 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jgr....94...37g&link_type=abstract
(Chapman Conference on Plasma Waves and Instabilities in Magnetospheres and at Comets, Sendai, Japan, Oct. 12-16, 1987) Journal
Other
59
Halley'S Comet, Plasma Frequencies, Plasma Turbulence, Power Spectra, Spectrum Analysis, Giotto Mission, Low Frequencies, Polarization (Waves), Solar Wind, Wave Propagation, Comets, Spectra, Frequencies, Plasma, Turbulence, Upstream, Halley, Magnetic Fields, Giotto Mission, Spacecraft Observations, Solar Wind, Position (Location), Bow Shock, Flows, Polarization, Characteristics, Harmonics, Waves, Parameters, Diagrams
Scientific paper
Two upstream regions have been identified in Giotto spacecraft magnetic field and plasma measurements subjected to cross-spectral analyses, in order to determine this cometary environment's low-frequency plasma turbulence spectral characteristics. One region's solar wind magnetic field was approximately parallel, and the other's perpendicular, to the solar wind flow velocity direction. Additional divergences relate to the regions having magnetic field lines that are either connected or disconnected to the cometary bow shock wave in either the quasi-parallel or quasi-perpendicular regions.
Acuña Mario Humberto
Coates Andrew J.
Glassmeier Karl-Heintz
Goldstein Michel L.
Johnstone Alan D.
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