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20022010
most citedAn Extreme Solar Event of 20 January 2005: Properties of the Flare and the Origin of Energetic Particles

106 citations

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13 papers · 1 filter

astro-ph200855 cited

Absorption Phenomena and a Probable Blast Wave in the 13 July 2004 Eruptive Event

V. V. Grechnev, A. M. Uralov, V. A. Slemzin +3

We present a case study of the 13 July 2004 solar event, in which disturbances caused by eruption of a filament from an active region embraced a quarter of the visible solar surfac…

astro-ph2008106 cited

An Extreme Solar Event of 20 January 2005: Properties of the Flare and the Origin of Energetic Particles

V. V. Grechnev, V. G. Kurt, I. M. Chertok +9

The extreme solar and SEP event of 20 January 2005 is analyzed from two perspectives. Firstly, we study features of the main phase of the flare, when the strongest emissions from m…

astro-ph200816 cited

Diamagnetic pumping near the base of a stellar convection zone

L. L. Kitchatinov, G. Rüdiger

The property of inhomogeneous turbulence in conducting fluids to expel large-scale magnetic fields in the direction of decreasing turbulence intensity is shown as important for the…

astro-ph20074 cited

Stability of toroidal magnetic fields in the solar tachocline and beneath

L. L. Kitchatinov, G. Rüdiger

Stability of toroidal magnetic field in a stellar radiation zone is considered for the cases of uniform and differential rotation. In the rigidly rotating radiative core shortly be…

astro-ph200713 cited

Effect of angular momentum distribution on gravitational loss-cone instability in stellar clusters around massive BH

Evgeny V. Polyachenko, Valery L. Polyachenko, Ilia G. Shukhman

Small perturbations in spherical and thin disk stellar clusters surrounding massive a black hole are studied. Due to the black hole, stars with sufficiently low angular momentum es…

astro-ph200746 cited

Stability of Toroidal Magnetic Fields in Rotating Stellar Radiation Zones

L. L. Kitchatinov, G. Ruediger

The questions of how strong magnetic fields can be stored in rotating stellar radiative zones without being subjected to pinch-type instabilities and how much radial mixing is prod…