Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Department of Physics and Astronomy, The University, Glasgow G12 8QQ, UK of Theoretical Astrophysics, P.B. 1029, Blindern, 0315 Oslo, Norway
Department of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK of Physics, The University of Alabama in Huntsville, Huntsville, AL 35899; Department of Physics and Astronomy, University of Glasgow, The Kelvin Building, Glasgow G12 8QQ, UK of Physics and Astronomy, University of Glasgow, The Kelvin Building, Glasgow, G12 8QQ, UK; Department of Physics, The University of Alabama in Huntsville, Huntsville, AL 35899 of Physics and Astronomy, University of Glasgow, The Kelvin Building, Glasgow G12 8QQ, UK of Physics and Astronomy, University of Glasgow, The Kelvin Building, G12 8QQ, UK; Department of Physics, The University of Alabama in Huntsville, Huntsville, AL 35899 of Physics and Astronomy, The University, Glasgow G12 8QQ, Scotland, UK
Lockheed Martin Advanced Technology Center, Solar & Astrophysics Laboratory, Dept. L9-41, Bldg.252, 3251 Hanover St., Palo Alto, CA 94304, USA
Astronomy and Astrophysics Group, Department of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK
University of Glasgow.
Department of Physics and Astronomy, The University, Glasgow G12 8QQ, UK
National Science Center `Kharkov Institute of Physics and Technology', 310108 Kharkov, Ukraine
Physics and Astronomy, Univ Glasgow, Glasgow, United Kingdom; of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom; & Astrophysics Group, University of Glasgow, Glasgow, United Kingdom; St
A visibility-based approach using regularization for imaging-spectroscopy in solar X-ray astronomy
Acceleration, magnetic fluctuations and cross-field transport of energetic electrons in a solar flare loop
An Explanation for Non-Power-Law Behavior in the Hard X-Ray Spectrum of the 2002 July 23 Solar Flare
Anisotropic Bremsstrahlung Emission and the Form of Regularized Electron Flux Spectra in Solar Flares
Characteristics of the flare acceleration region derived from simultaneous hard X-ray and radio observations
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Profile ID: LFWR-SCP-P-23528