Interplanetary variability in particle fluxes recorded by the low energy charged particle detector SLED (about 30 keV to greater than 30 MeV) during the Cruise Phase of the PHOBOS Mission to Mars and its moons

Details Interplanetary variability in particle fluxes recorded by the low energy charged particle detector SLED (about 30 keV to greater than 30 MeV) during the Cruise Phase of the PHOBOS Mission to Mars and its moons Interplanetary variability in particle fluxes recorded by the low energy charged particle detector SLED (about 30 keV to greater than 30 MeV) during the Cruise Phase of the PHOBOS Mission to Mars and its moons

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991angeo...9..348m&link_type=abstract

Annales Geophysicae (ISSN 0939-4176), vol. 9, May 1991, p. 348-356. Research supported by Irish National Board for Science and T

Astronomy and Astrophysics

Astronomy

2

Interplanetary Medium, Mars Probes, Particle Telescopes, Solar Planetary Interactions, U.S.S.R. Space Program, Charged Particles, Energy Spectra, Solar Cycles, Solar Wind, Spaceborne Astronomy

Scientific paper

Two lightweight telescope detector systems, codenamed SLED-1 and SLED-2, with the capability to monitor electron and ion fluxes within an energy range spanning 34 keV to a few tens of MeV, were launched on the twin spacecraft of the Soviet Phobos Mission to Mars and its moons in July 1988. Solar-related particle enhancements recorded during the Cruise Phase, and also in the near Martian environment, over the interval 19 July 1988-27 March 1989 while the interplanetary medium was in course of changing over from solar-minimum to solar-maximum dominated conditions, are presented. In particular, examples of signatures characterizing events associated with each of these phenomenological states are provided in the context of attempting to elucidate how the solar interplanetary medium evolves from one condition to the other.

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