Global Development of the Supersubstorm of May 28, 2011     

Despirak  I. V.  Kleimenova  N. G.  Lyubchich  A. A.  Setsko  P. V.  Gromova  L. I.  Werner  R. 《Geomagnetism and Aeronomy》2022,62(3):199-208

Geomagnetism and Aeronomy - The paper gives an analysis of the isolated supersubstorm observed during the main phase of the moderate magnetic storm on May 28, 2011 (SYM/H ~ –95 nT), which was...  相似文献   

Modeling of Proton Acceleration in a Magnetic Island Inside the Ripple of the Heliospheric Current Sheet     

Mingalev  O. V.  Khabarova  O. V.  Malova  Kh. V.  Mingalev  I. V.  Kislov  R. A.  Mel’nik  M. N.  Setsko  P. V.  Zelenyi  L. M.  Zank  G. P. 《Solar System Research》2019,53(1):30-55

Crossings of the heliospheric current sheet (HCS) at the Earth’s orbit are often associated with observations of anisotropic beams of energetic protons accelerated to energies from hundreds of keV to several MeV and above. A connection between this phenomenon and the occurrence of small-scale magnetic islands (SMIs) near reconnecting current sheets has recently been found. This study shows how pre-accelerated protons can be energized additionally due to oscillations of multiple SMIs inside the ripple of the reconnecting HCS. A model of the electromagnetic field of an oscillating 3D SMI with a characteristic size of ~0.001 AU is developed. A SMI is supposed to be bombarded by protons accelerated by magnetic reconnection at the HCS to energies from ~1keV to tens of keV. Numerical simulations have demonstrated that the resulting longitudinal inductive electric fields can additionally reaccelerate protons injected into a SMI. It is shown that there is a local “acceleration” region within the island in which particles gain energy most effectively. As a result, their average escape energies range from hundreds of keV to 2 MeV and above. There is almost no particle acceleration outside the region. It is shown that energies gained by protons significantly depend on the initial phase and the place of their entry into a SMI but weakly depend on the initial energy. Therefore, low-energy particles can be accelerated more efficiently than high-energy particles, and all particles can reach the total energy limit upon their escape from a SMI. It is also found that the escape velocity possesses a strong directional anisotropy. The results are consistent with observations in the solar wind plasma.

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