Bidirectional MeV/n ion intervals - Observations from the Goddard Space Flight Center instruments on the ISEE 3/ICE, IMP 8, HELIOS 1 and HELIOS 2 spacecraft

Details Bidirectional MeV/n ion intervals - Observations from the Goddard Space Flight Center instruments on the ISEE 3/ICE, IMP 8, HELIOS 1 and HELIOS 2 spacecraft Bidirectional MeV/n ion intervals - Observations from the Goddard Space Flight Center instruments on the ISEE 3/ICE, IMP 8, HELIOS 1 and HELIOS 2 spacecraft

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991icrc....3..292r&link_type=abstract

IN: International Cosmic Ray Conference, 22nd, Dublin, Republic of Ireland, Aug. 11-23, 1991, Laboratory for High Energy Astroph

Astronomy and Astrophysics

Astrophysics

Energetic Particles, Explorer 50 Satellite, Helios 1, Helios 2, International Sun Earth Explorer 3, Magnetohydrodynamic Flow, Solar Wind, Annual Variations, Heliosphere, Interplanetary Medium, Satellite-Borne Instruments, Solar Cycles, Solar Electrons

Scientific paper

A search is made for intervals of bidirectional energetic ion streaming in approximately 1 MeV data from the instruments on ISEE 3/ICE, IMP 8 and Helios 1 and 2 during 1973 to 1989. The longest duration intervals are found around solar maximum, consistent with the expected association with coronal mass ejections. The ISEE 3/ICE intervals are associated with previously identified bidirectional 35-1000 keV ions and solar-wind electron heat fluxes, though additional bidirectional intervals are found.

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