Observations of plasma dynamics in the coma of P/Halley by the Giotto Ion Mass Spectrometer

Details Observations of plasma dynamics in the coma of P/Halley by the Giotto Ion Mass Spectrometer Observations of plasma dynamics in the coma of P/Halley by the Giotto Ion Mass Spectrometer

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991sicd.reptq....g&link_type=abstract

In LMSC, A Study of Ion Composition and Dynamics at Comet Halley 23 p (SEE N93-13465 03-90)

Computer Science

Alpha Particles, Giotto Mission, Halley'S Comet, Heavy Ions, Ionopause, Magnetohydrodynamic Flow, Mass Spectrometers, Plasma Dynamics, Angular Distribution, Distribution Functions, Far Fields, Protons, Solar Wind

Scientific paper

Observations in the coma of P/Halley by the Giotto Ion Mass Spectrometer (IMS) are reported. The High Energy Range Spectrometer (HERS) of the IMS obtained measurements of protons and alpha particles from the far upstream region to the near ionopause region and of ions from mass 12 to 32 at distances of about 250,000 to 40,000 km from the nucleus. Plasma parameters from the High Intensity Spectrometer (HIS) of the IMS obtained between 150,000 to 5000 km from the nucleus are also discussed. The distribution functions of water group ions (water group will be used to refer to ions of 16 to 18 m/q, where m is in AMU and q is in unit charges) are observed to be spherically symmetric in velocity space, indicating strong pitch angle scattering. The discontinuity known as the magnetic pile-up boundary (MPB) is apparent only in proton, alpha, and magnetometer data, indicating that it is a tangential discontinuity of solar wind origin. HERS observations show no significant change in the properties of the heavy ions across the MPB. A comparison of the observations to an MHD model is made. The plasma flow directions at all distances greater than 30,000 km from the nucleus are in agreement with MHD calculations. However, despite the agreement in flow direction, within 200,000 km of the nucleus the magnitude of the velocity is lower than predicted by the MHD model and the density is much larger (a factor of 4). Within 30,000 km of the nucleus there are large theoretical differences between the MHD model flow calculations for the plane containing the magnetic field and for the plane perpendicular to the magnetic field. The observations agreed much better with the pattern calculated for the plane perpendicular to the magnetic field. The data obtained by the High Energy Range Spectrometer (HERS) of the IMS that are published herein were provided to the International Halley Watch archive.

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