Physics
Scientific paper
Aug 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986georl..13..825y&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 13, Aug. 1986, p. 825-828.
Physics
33
Halley'S Comet, Magnetohydrodynamic Waves, Positive Ions, Space Plasmas, Ion Cyclotron Radiation, Japanese Spacecraft, Oxygen Ions, Plasma-Particle Interactions, Transverse Waves, Water
Scientific paper
Long-period HM waves with 150-380 s periods were observed by Sakigake at 7 x 10 to the 6th km upstream from Comet Halley. The wave amplitudes were as great as approximately 2 nT peak to peak. The long-period waves were of an approximately linearly polarized transverse mode and propagated parallel to the ambient magnetic field. Dominant periods of the waves were found to be consistent with the local O(+) (or H2O/+/) cyclotron period and to change as a function of the ambient magnetic field. The long-period HM waves are believed to be excited by a resonant instability with high-energy cometary heavy ions. The necessary cometary ion density for excitation at a distance of 7 x 10 to the 6th km from the comet can be inferred to be of the order of .001-.0001/cu cm for .1-.01 keV O(+) (or H2O/+/) ions.
Nakagawa Takao
Saito Takesi
Yumoto Kiyo
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