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pro vyhledávání: '"Tähtinen, Ismo"'
The relation between the intensity of chromospheric emissions and the photospheric magnetic field strength has been examined in several studies, but the effect of the magnetic field inclination on chromospheric emissions remains almost unexplored. We
Externí odkaz:
http://arxiv.org/abs/2409.17771
The open solar flux, that is, the total magnetic flux escaping the Sun, is one of the most important parameters connecting solar activity to the Earth. The open solar flux is commonly estimated from photospheric magnetic field measurements by making
Externí odkaz:
http://arxiv.org/abs/2408.11525
Publikováno v:
A&A 664, A2 (2022)
The bright regions in the solar chromosphere and temperature minimum have a good spatial correspondence with regions of intense photospheric magnetic field. Their observation started more than a hundred years ago with the invention of the spectroheli
Externí odkaz:
http://arxiv.org/abs/2204.13944