Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Imperial College, London
Department of Physics and Astronomy, Rice University; Solar Physics Lab., NASA Goddard Space Flight Center
Space and Atmospheric Physics Group, The Blackett Laboratory, Imperial College
Space and Atmospheric Physics Department, The Blackett Laboratory, Imperial College
Dept of Physics and Astronomy, Rice Univ, Houston, TX, USA; Laboratory, Imperial College London, Prince Consort Road, London SW7 2BZ, UK of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge, CB3 0WA, UK
NASA Goddard Space Flight Center, Solar Physics Lab., Code 671, 8800 Greenbelt Road, Greenbelt, MD 20771, USA ; Department of Computational and Data Sciences, George Mason University, 4400 University Drive, MSN 6A2, Fairfax, VA 22030, USA of Physics and Astronomy, Rice University, Houston, TX 77005, USA
Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK
Space and Atmospheric Physics, Blackett Laboratory, Imperial College London, Prince Consort Road, SW7 2BZ, London, UK and Atmospheric Physics Group, Blackett Laboratory, Imperial College London, Prince Consort Road, London SW7 2BZ, UK
NASA Goddard Space Flight Center, Solar Physics Lab., Code 671, 8800 Greenbelt Road, Greenbelt, MD 20771, USA; Department of Computational and Data Sciences, George Mason University, 4400 University Drive, MSN 6A2, Fairfax, VA 22030, USA and Atmospheric Physics, Blackett Laboratory, Imperial College London, Prince Consort Road, London, SW7 2BZ, UK & Atmospheric Physics, Blackett Lab
A New Enthalpy-Based Approach to the Transition Region in an Impulsively Heated Corona
A numerical tool for the calculation of non-equilibrium ionisation states in the solar corona and other astrophysical plasma environments
A Reconnection-driven Rarefaction Wave Model for Coronal Outflows
A reinterpretation of the energy balance in active region loops following new results from Hinode EIS
A self-consistent treatment of radiation in coronal loop modelling
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