Results 161 to 170 of about 2,273 (184)

Solar X-ray and EUV corona and their relation to the magnetic activity

Advances in Space Research, 2007
Abstract We have studied the solar magnetic cycle in corona using X-ray data from YOHKOH and Extreme Ultraviolet data from SOHO/EIT. Soft X-ray data last the period from after the maximum cycle 22 to the maximum cycle 23 (1991–2001). The SOHO/EIT Extreme Ultraviolet data are used for the period from 1996 to 2003.
openaire   +1 more source

MHD activity of the solar corona

Science and Supercomputing at Cineca, 2001
R. Betta, G. Einaudi, M. Velli
openaire   +1 more source

Sunspot Activity and the form of the Solar Corona

Monthly Notices of the Royal Astronomical Society, 1938
W. E. Bernheimer, F. J. M. Stratton
openaire   +1 more source

Parker Solar Probe Enters the Magnetically Dominated Solar Corona

Physical Review Letters, 2021
Davin Larson, Jasper S. Halekas, Kristopher G. Klein   +2 more
exaly  

Observations of the Solar Corona From Space

Space Science Reviews, 2020
Louise Harra, Roberto Susino, Daniele Telloni   +2 more
exaly  

Plasma Heating Induced by Tadpole-Like Downflows in the Flaring Solar Corona

Innovation(China), 2021
Hui Tian, Katharine Reeves
exaly  

Signatures of Slow Solar Wind Streams From Active Regions in the Inner Corona

Solar Physics, 2013
Farid Goryaev, Louise Harra, Vladimir Slemzin   +2 more
exaly  

Kinetic Physics of the Solar Corona and Solar Wind

Living Reviews in Solar Physics, 2006
Eckart Marsch
exaly  

Observationally Driven 3D Magnetohydrodynamics Model of the Solar Corona Above an Active Region

Astronomy and Astrophysics, 2013
Sven Bingert, Hardi Peter
exaly  

STRUCTURE AND DYNAMICS OF THE SOLAR CORONA DURING DIFFERENT PHASES OF SOLAR ACTIVITY

БЛИЗКИЯТ КОСМОС – ОБЩА ЦЕЛ
M. Kostov, A. Stoev, P. Stoeva
openaire   +1 more source