On energetic particle flux variations inside a magnetic cloud

Details On energetic particle flux variations inside a magnetic cloud On energetic particle flux variations inside a magnetic cloud

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995jgr...10023507v&link_type=abstract

Journal of Geophysical Research, Volume 100, Issue A12, p. 23507-23514

Astronomy and Astrophysics

Astrophysics

2

Interplanetary Physics: Interplanetary Magnetic Fields, Solar Physics, Astrophysics, And Astronomy: Flares, And Astronomy: Magnetic Fields

Scientific paper

Helios 1 observed a magnetic cloud on the spacecraft's closest approach to the Sun (0.3 AU) on March 26, 1976. Fluxes of energetic particles detected by the spacecraft generally decrease during the passage of a cloud, but in this case the smooth intensity depression was interrupted by a sharp peak-like increase coinciding with a deep drop of the magnetic field magnitude. This behavior is observed for protons and electrons in several energy bands. A possible explanation of this event is given by the spheroidal model of magnetic clouds, applicable for the plasmoid geometry (having field lines fully disconnected with the Sun).

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