The physics of the Solar Atmosphere: theory, radiation diagnostics and supercomputing
The Sun, our star, is not only the source of the electromagnetic radiation that bathes our planet; it also sweeps the Earth's magnetosphere with its wind and heliospheric magnetic field. It frequently sends huge ropes of magnetized plasma, the coronal mass ejections, that can hit us and cause solar storms, thus constituting a serious potential
Elena
Khomenko Shchukina
Fernando
Moreno Insertis
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