Formation of Coronal Large-Amplitude Waves and the Chromospheric Response
- 9 December 2015
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 291 (1) , 89-115
Abstract
No abstract availableKeywords
This publication has 68 references indexed in Scilit:
- SDO/AIA ANDHINODE/EIS OBSERVATIONS OF INTERACTION BETWEEN AN EUV WAVE AND ACTIVE REGION LOOPSThe Astrophysical Journal, 2013
- The Wave–Driver System of the Off-Disk Coronal Wave of 17 January 2010Solar Physics, 2012
- UNDERSTANDINGSDO/AIA OBSERVATIONS OF THE 2010 JUNE 13 EUV WAVE EVENT: DIRECT INSIGHT FROM A GLOBAL THERMODYNAMIC MHD SIMULATIONThe Astrophysical Journal, 2012
- FIRST SIMULTANEOUS OBSERVATION OF AN Hα MORETON WAVE, EUV WAVE, AND FILAMENT/PROMINENCE OSCILLATIONSThe Astrophysical Journal Letters, 2012
- PLASMA DIAGNOSTICS OF AN EIT WAVE OBSERVED BY HINODE /EIS AND SDO /AIAThe Astrophysical Journal Letters, 2011
- Three‐dimensional numerical simulation of MHD waves observed by the Extreme Ultraviolet Imaging TelescopeJournal of Geophysical Research, 2001
- Solar flares and coronal shock wavesJournal of Geophysical Research, 2001
- Magnetostatic structures of the solar corona. 2: The magnetic topology of quiescent prominencesThe Astrophysical Journal, 1995
- Recent Observations of Dynamical Phenomena Associated with Solar FlaresPublications of the Astronomical Society of the Pacific, 1960
- Relative Times of Arrival of Bursts of Solar Noise on Different Radio FrequenciesNature, 1947