Diamagnetic Reduction in the Magnetic Field above a Sunspot in the Gamma-Ray Burst on July 14, 2000статья
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Дата последнего поиска статьи во внешних источниках: 19 сентября 2015 г.
Аннотация:Earlier, the authors proposed a model for describing the motion of trapped ions accelerated to
energies of 10–100 MeV/nucleon in an electric field of 0.01–0.1 V/cm with a nonzero magnetic-field-aligned
component in coronal solar loops with a characteristic size of ~100 000 km. The simulation results were used
to interpret the properties of gamma-ray sources in a powerful solar burst that occurred on July 14, 2000.
According to the proposed model, the gamma-ray source emitting lines with photon energies of 4.1–6.7 MeV
was located above the sunspot and the source of the 2.223-MeV line coincided with the region of the observed
drop-out of accelerated ions into dense layers of the solar atmosphere in the sunspot, where a short-term
reduction in the photospheric magnetic field by about 100 G was simultaneously observed. An idea is stated
and justified for the first time that the local reduction in the magnetic field in the sunspot is caused by the
diamagnetic effect created by accelerated ions in the magnetic mirror of the coronal magnetic flux rope above
the sunspot.