Premium
The variation of protons, alpha particles, and the magnetic field across the bow shock of comet Halley
Author(s) -
Neugebauer M.,
Neubauer F. M.,
Balsiger H.,
Fuselier S. A.,
Goldstein B. E.,
Goldstein R.,
Mariani F.,
Rosenbauer H.,
Schwenn R.,
Shelley E. G.
Publication year - 1987
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/gl014i010p00995
Subject(s) - solar wind , physics , comet , halley's comet , bow shock (aerodynamics) , bow wave , shock (circulatory) , astrophysics , magnetometer , magnetic field , shock wave , proton , plasma , astronomy , geophysics , nuclear physics , mechanics , quantum mechanics , medicine
Data from the Ion Mass Spectrometer and the magnetometer on the Giotto spacecraft are used to examine the structure of the inbound crossing of the comet Halley bow shock on March 13, 1986. It is found that the velocity decrease, the field strength increase, and the heating of picked up cometary protons occurred over a broad region corresponding to several heavy‐ion gyroradii. The solar‐wind protons and alphas, on the other hand, were compressed and heated at a narrow structure, which might be called a subshock, on the leading edge of the broad shock region. The electrostatic potential difference across the shock was less than 40 V.