Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Max-Planck-Institut für Sonnensystemforschung
Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland
Bulgarian Academy of Sciences, Sofia, Bulgaria
Institute of Astronomy, 72 Tzarigradsko chaussee Blvd, 1784 Sofia, Bulgaria Observatory, College Hill, Armagh BT61 9DG, N. Ireland; Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany; Department of Solar Physics, Royal Observatory of Belgium, Av. Circulaire 3, 1180 Bruxelles, Belgium
Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany; Department of Solar Physics, Royal Observatory of Belgium, Av. Circulaire 3, 1180 Bruxelles, Belgium
Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland; Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK
Mullard Space Science Laboratory, UCL, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UK
Max-Planck-Institut für Sonnensystemforschung Former Max-Planck-Institut für Aeronomie, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany; Department of Solar Physics, Royal Observatory of Belgium, Av. Circulaire 3, 1180 Bruxelles, Belgium
Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland; Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK
Royal Observatory of Belgium, 3 Circular Avenue, 1180 Brussels, Belgium
Solar Influences Data analysis Center, Royal Observatory of Belgium, 3 Circular Avenue, 1180 Brussels, Belgium
Royal Observatory of Belgium, 3 Circular Avenue, 1180 Brussels, Belgium Observatory, College Hill, Armagh, BT61 9DG, N. Ireland
An EUV Bright Point as seen by SUMER, CDS, MDI and EIT on-board SoHO
Bi-Directional Jets at Coronal Hole Boundaries
Can coronal hole spicules reach coronal temperatures?
Chromospheric Magnetic Reconnection caused by Photospheric Flux Emergence: Implications for Jet-like Events Formation
Coronal hole boundaries evolution at small scales: I. EIT 195 A and TRACE 171 A view
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