G
G. M. Simnett
Researcher at University of Birmingham
Publications - 166
Citations - 11436
G. M. Simnett is an academic researcher from University of Birmingham. The author has contributed to research in topics: Coronal mass ejection & Solar flare. The author has an hindex of 44, co-authored 166 publications receiving 10839 citations.
Papers
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Book ChapterDOI
Solar Particles Observed Near 33° S Latitude
S. J. Tappin,G. M. Simnett +1 more
TL;DR: In this article, the ions and electrons seen by the HI-SCALE instrument on the Ulysses spacecraft in the interval from 21-30 June 1993, ahead of an arrival of the CIR, were analyzed.
Journal ArticleDOI
Observations at the onset of a large solar flare and their relevance to energy transfer
TL;DR: In this article, an analysis of the July 14, 1980 GOES X1 flare is presented, where the impulsive hard X-ray burst occurred near the end of the soft Xray flare.
Prominence activity related to CME observed by SOHO, Yohkoh and ground-based observatories
Brigitte Schmieder,L. vanDriel-Gesztelyi,J. E. Wiik,Therese A. Kucera,Barbara J. Thompson,Craig DeForest,Chris SaintCyr,G. M. Simnett +7 more
TL;DR: In this paper, the authors present examples of destabilization of prominences and their associated coronal mass ejections (CMEs) during the 1996 campaigns of multi-wavelength observations with the Solar and Heliospheric Observatory (SOHO), the Yohkoh satellite's soft X-ray telescope (SXT) and the Meudon (France) H alpha spectroheliograph eruptive solar filaments and prominence associated with the CMEs.
Journal ArticleDOI
Energetic neutral atoms from the Sun: an alternative interpretation of a unique event
TL;DR: In this paper, it was shown that the particle event associated with the first major flare of the current solar cycle, on 5 December 2006, has been interpreted as containing energetic neutral hydrogen atoms (ENA) of at least a few MeV.
Journal ArticleDOI
Origin and location of chromospheric evaporation in flares
TL;DR: In this article, the authors observed that at flare onset the emission in soft (3.5 - 8 keV) and hard (16 - 30 keV), X-rays are predominant at the footpoints of the flaring loops.