Physics
Scientific paper
Nov 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986georl..13.1085s&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 13, Nov. 1986, p. 1085-1088. Research supported by the Canada-France-Hawaii
Physics
14
Comet Tails, Giacobini-Zinner Comet, International Sun Earth Explorer 3, Cometary Magnetospheres, Diameters, Magnetic Fields, Magnetic Variations, Space Observations (From Earth)
Scientific paper
Comparison of ground-based and in situ observations of P/Giacobini-Zinner are used to investigate the morphology of a type I cometary tail. ICE magnetic field and plasma measurements show a well-defined cometary magnetotail composed of two magnetic lobes in pressure equilibrium with a central plasma sheet. A dependence of ion tail width on IMF direction is found which strongly suggests that the classical type I ion tails observed on the ground consist predominantly of emissions from the slab-shaped plasma sheet separating the magnetic lobes. The width of the G-Z magnetotail is determined to be 9.8 (+ or - 0.5) x 10 to the 3rd km with a quasi-circular cross section. The results of this study also indicate that some of the dynamical thinnings and thickenings observed in long type I tails may be caused by IMF variations changing the angle with which the plasma sheet is viewed at earth.
Bame J. Jr. S.
Goldberg Bruce A.
McComas David John
Slavin James Arthur
Smith Edward. J.
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