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

106 citations · 713 across the 24 of their papers we have counts for

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Showing 2014Show all

4 papers · 1 filter

astro-ph.SR2014★ 28 cited

Responsibility of a Filament Eruption for the Initiation of a Flare, CME, and Blast Wave, and its Possible Transformation into a Bow Shock

V. V. Grechnev, A. M. Uralov, I. V. Kuzmenko +3

Multi-instrument observations of two filament eruptions on 24 February and 11 May 2011 suggest the following updated scenario for eruptive flare, CME and shock wave evolution. An i…

astro-ph.SR2014★ 30 cited

A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. IV. Unusual Magnetic Cloud and Overall Scenario

V. V. Grechnev, A. M. Uralov, I. M. Chertok +4

The geomagnetic superstorm of 20 November 2003 with Dst = -422 nT, one of the most intense in history, is not well understood. The superstorm was caused by a moderate solar eruptiv…

astro-ph.SR2014★ 16 cited

A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. III. Catastrophe of the Eruptive Filament at a Magnetic Null Point and Formation of an Opposite-Handedness CME

A. M. Uralov, V. V. Grechnev, G. V. Rudenko +4

Our analysis in Papers I and II (Grechnev et al., 2014, Solar Phys. 289, 289 and 1279) of the 18 November 2003 solar event responsible for the 20 November geomagnetic superstorm ha…

astro-ph.SR2014★ 29 cited

The relativistic solar particle event of 2005 January 20: origin of delayed particle acceleration

K. -L. Klein, S. Masson, C. Bouratzis +3

The highest energies of solar energetic nucleons detected in space or through gamma-ray emission in the solar atmosphere are in the GeV range. Where and how the particles are accel…