Proton flares and the topology of the magnetic field in the active regions of the Sun

Details Proton flares and the topology of the magnetic field in the active regions of the Sun Proton flares and the topology of the magnetic field in the active regions of the Sun

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ijga....6i2003p&link_type=abstract

International Journal of Geomagnetism and Aeronomy, Volume 6, Issue 2, CiteID GI2003

Astronomy and Astrophysics

Astrophysics

Solar Physics, Astrophysics, And Astronomy: Flares, Solar Physics, Astrophysics, And Astronomy: Magnetic Fields, Solar Physics, Astrophysics, And Astronomy: Energetic Particles (2114)

Scientific paper

[1] Events in flare productive active regions (ARs) accompanied by proton flares are considered on the basis of the observations from the ground and spacecrafts during the recent decades. The principal features of the morphology, magnetic fields, and substance mass motions in the ARs and also their variations with time are analyzed. All the considered ARs had a common feature in the magnetic field structure: a rather extended configuration of the δ type existed in them. The observations in the high-altitude expedition of the Sternberg Institute and the data from publications have been used.

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