Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Astronomical Observatory Belgrade, Volgina 7, 11160 Belgrade, Serbia Observatorium, Universiteit Gent, Krijgslaan 281, B-9000 Gent, Belgium
Astronomical Observatory Belgrade, Volgina 7, 11160 Beograd, Serbia and Montenegro
Astronomical Observatory, Volgina 7, 11160 Belgrade, Serbia
Belgian Institute for Space Aeronomy, Ringlaan 3, B-1180 Brussels, Belgium
Institute of Physics, Beograd, Yugoslavia
Center for Plasma-Astrophysics, K.U. Leuven, Celestijnenlaan 200 B, B-3001 Heverlee, Belgium
Celestijnenlaan 200B, B-3001 Heverlee, Belgium
Royal Observatory of Belgium, Ringlaan 3, B-1180 Brussels, Belgium
Institut za Fiziku, Belgrade, Yugoslavia
Departament de Física, Universitat de les Illes Balears, 07071 Palma de Mallorca, Spain
Astronomical Observatory, Volgina 7, 11060 Belgrade 38, Serbia
Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281, 9000 Gent, Belgium
Astronomical Observatory, Volgina 7, 11160 Belgrade, Serbia and Montenegro
Universiteit Gent, Sterrenkundig Observatorium, Krijgslaan 281, B-9000 Gent, Belgium
Departament de Fisica, Universitat de les Illes Balears
Centrum voor Plasma Astrofysica, K.U.Leuven, Celestijnenlaan 200 B, B-3001 Heverlee, Belgium
Centre for Plasma-Astrophysics, K.U. Leuven, Celestijnenlaan 200 B, B-3001 Heverlee, Belgium
Belgian Institute voor Space Aeronomy, Ringlaan 3, B-1180 Brussels, Belgium
Belgisch Instituut voor Ruimte-Aëronomie, Ringlaan 3, B-1180 Ukkel, Belgium
Royal Observatory of Belgium and Belgian Institute for Space Aeronomy, Ringlaan 3, B-1180 Brussels, Belgium
Absorption of magnetosonic waves in presence of resonant slow waves in the solar atmosphere.
Analytical Modeling of Composed Cylindrical Magnetic Structures in the Corona
Analytical Treatment Of Static Magnetic Field Strucures In The Corona From Boundary Conditions On The Photosphere
Applicability problem of Jeans criterion to a stationary self-gravitating cloud
Coronal MHD Perturbation Field Generated by Localized Perturbers in a Photospheric Active Region
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