Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Department of Astronomy, Physics of the Earth, and Meteorology, Faculty of Mathematics, Physics and Informatics, Comenius University, Mlynská Dolina F2, 842 48 Bratislava, Slovak Republic
Department of Astronomy, Physics of the Earth and Meteorology, Faculty of Mathematics, Physics and Informatics, Comenius University; LESIA, Observatoire de Paris, CNRS, UPMC, Université Paris Diderot
Department of Astronomy and Astrophysics, DAPEM, Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovakia
Department of Astronomy, Physics of the Earth and Meteorology, Faculty of Mathematics, Physics and Informatics, Comenius University, Mlynská Dolina F2, 842 48 Bratislava, Slovak Republic
Department of Astronomy, Physics of the Earth and MeteorologyFaculty of Mathematics, Physics and Informatics, Comenius University, Mlynská Dolina F2, 842 48, Bratislava, Slovak Republic ; Astronomical Institute of the Academy of Sciences of the Czech Republic, Fričova 298, 251 65, Ondřejov, Czech Republic
Astronomical Institute of the Academy of Sciences of the Czech Republic, 25165, Ondřejov, Czech Republic; Dept. of Astronomy, Physics of the Earth and Meteorology, Faculty of Mathematics, Physics and Informatics, Comenius University, 84248, Bratislava, Slovak Republic
Astronomical Institute of the Academy of Sciences of the Czech Republic, Fričova 298, 251 65, Ondřejov, Czech Republic; Faculty of Mathematics Physics and Informatics, Comenius University, Mlynská dolina F2, 842 48, Bratislava, Slovakia
Department of Astronomy, Physics of the Earth, and MeteorologyFaculty of Mathematics, Physics and Informatics, C
Analytical model of static coronal loops
C IV emission and magnetic topology. (Slovak Title: Emisia C IV a magnetická topológia)
C IV Enhanced Emission and the Non-Thermal Electron Distribution
Changes in Filament Connectivity and its Structure during the C-Class Flare
EUV filter responses to plasma emission for the nonthermal κ-distributions
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Profile ID: LFWR-SCP-P-480652