Results 161 to 170 of about 2,148 (181)
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Solar X-ray and EUV corona and their relation to the magnetic activity
Advances in Space Research, 2007Abstract 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.
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MHD activity of the solar corona
Science and Supercomputing at Cineca, 2001R. Betta, G. Einaudi, M. Velli
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Sunspot Activity and the form of the Solar Corona
Monthly Notices of the Royal Astronomical Society, 1938W. E. Bernheimer, F. J. M. Stratton
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Parker Solar Probe Enters the Magnetically Dominated Solar Corona
Physical Review Letters, 2021Davin Larson +2 more
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Kinetic Physics of the Solar Corona and Solar Wind
Living Reviews in Solar Physics, 2006Eckart Marsch, Marsch Eckart
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STRUCTURE AND DYNAMICS OF THE SOLAR CORONA DURING DIFFERENT PHASES OF SOLAR ACTIVITY
БЛИЗКИЯТ КОСМОС – ОБЩА ЦЕЛM. Kostov, A. Stoev, P. Stoeva
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Study of the Effect of Active Regions on the Scattering Polarization in the Solar Corona
Publications of the Astronomical Society of the Pacific, 2018M. Derouich, null Badruddin
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Magnetohydrodynamic modeling of the global solar corona
Physics of Plasmas, 1999Roberto Lionello +2 more
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