Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Queen's University Belfast, UK
Queen's University of Belfast
Institute of Astronomy & Astrophysics, National Observatory of Athens, Greece
Department of Pure and Applied Physics, Queen's University Belfast, Belfast BT7 1NN
Department of Physics and Astronomy, University of Manchester, Manchester, M13 9PL, UK of Pure and Applied Physics, The Queen's University of Belfast, Belfast BT7 1NN, Northern Ireland
Department of Physics and Astronomy, University of Manchester, Oxford Rd., Manchester M13 9PL, UK
Department of Pure and Applied Physics, The Queen's University of Belfast, Belfast, BT7 1NN, Ireland
Department of Solar Physics, Royal Observatory of Belgium, Avenue Circulaire -3- Ringlaan, B-1180, Belgium; Department of Pure and Applied Physics, Queen's University Belfast, Belfast, BT7 1NN, UK T.Katsiyannisatoma.be
Royal Observatory of Belgium, Ave. Circulaire -3- Ringlaan, B-1180, Brussels, Belgium
Institute of Astronomy and Astrophysics, National Observatory of Athens, I. Metaxa & V. Paulou, Penteli, 15236 Athens, Greece; Royal Observatory of Belgium, Solar Physics, Ringlaan 3, 1180 Brussels, Belgium
Institute of Astronomy and Astrophysics, National Observatory of Athens, I. Metaxa and V. Paulou, Penteli, 15236 Athens, Greece
Department of Pure and Applied Physics, The Queen's University of Belfast, Belfast, BT7 1NN, N. Ireland of Pure and Applied Physics, Queen's University, Belfast BT7 1NN
Department of Pure and Applied Physics, Queen's University, Belfast BT7 1NN, Northern Ireland, UK of Pure and Applied Physics, Queen's University, Belfast BT7 1NN, Northern Ireland, UK Observatory of Belgium, Belgium
A Comparison of Theoretical mg vi Emission Line Strengths with Active-Region Observations From Serts
A Comparison of Theoretical Si <Emphasis Type="SmallCaps">VIII</Emphasis> Emission Line Ratios with Observations from Serts
An observational study of a magneto-acoustic wave in the solar corona
Aristarchos RISE2: A Wide-Field Fast Imager for Exoplanet Transit Timing
Brown dwarfs and low-mass stars in the Pleiades and Praesepe:- Membership and binarity
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