Energetic ion observations in the magnetic cloud of 14-15 January 1988 and their implications for the magnetic field topology

Details Energetic ion observations in the magnetic cloud of 14-15 January 1988 and their implications for the magnetic field topology Energetic ion observations in the magnetic cloud of 14-15 January 1988 and their implications for the magnetic field topology

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991icrc....3..597r&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

Interplanetary Medium, Magnetic Clouds, Magnetic Field Configurations, Solar Corpuscular Radiation, Imp, Lines Of Force, Magnetic Flux, Satellite Observation, Shock Wave Propagation

Scientific paper

On 14-15 January 1988, a magnetic cloud with a local field topology consistent with an east-west aligned cylindrical flux-rope and which formed the driver of an interplanetary shock passed the earth. Using 0.5-4 MeV/n ion data from the instrument on IMP 8, the paper addresses the question of whether or not magnetic field lines within the magnetic cloud were connected to the sun. An impulsive solar particle event was detected inside the magnetic cloud strongly suggesting that the field lines were rooted at the sun.

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