Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Jet Propulsion Laboratory, California Institute of Technology, CA USA;
Jet Propulsion Laboratory, Caltech
Universita di Firenze
Dipartimento di Astronomia, Università di Firenze, Largo E. Fermi 2, Firenze, FI 50125 Italy; Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA di Astronomia, Università di Firenze, Largo E Fermi 2, Firenze, FI 50125 Italy; Jet Propulsion Laboratory, 4800 Oak Grove Dr., Pasadena, CA 91109, USA University
Osservatorio di Firenze
Department of Mathematical Sciences, University of St. Andrews, Fife, KY16 9SS, Scotland
Departement de Recherche Spatiale, Observatoire de Meudon, 92190 Meudon, France
Florence Univ., Italy
Department of Astronomy and Space Sciences, University of Florence, Largo E. Fermi 2, 50125 Florence, Italy
Dipartimento di Astronomia e Scienza dello Spazio, Università di Firenze, Firenze, Italy
Jet Propulsion Laboratory, Pasadena, CA, USA; Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA; Plasmas, Jet Propulsion Laboratory, California Institute of Technology, NASA, Pasadena, CA, USA; Andrews, University, Scotland
Dipartimento di Astronomia e Scienza dello Spazio, Università di Firenze, Largo Enrico Fermi, 2, Firenze, 50125 Italy Propulsion Laboratory;, Università degli Studi
JPL
Jet Propulsion Laboratory, California Institute of Technology., 4800 Oak Grove Drive, Pasadena, CA 91109, USA Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA di Astronomia e Scienza dello Spazio, Università di Firenze, Largo E. Fermi 5, I-50125 Firenze, Italy
Dip. di Astronomia e Scienze dello Spazio, Università di Firenze
Jet Propulsiona Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA Propulsion Laboratory, 4800 Oak Grove
'Alfvenic' versus 'standard' turbulence in the solar wind
3D MHD description of the region beyond the termination shock: The behaviour of the Current Sheet
3d Mhd Simulation Of Sympathetic Eruptions On 1 August 2010
A MHD-turbulence model for solar corona
A model for magnetically coupled sympathetic eruptions
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