Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Theoretische Physik IV Ruhr-Universitaet Bochum, Germany
Theoretische Physik IV, Ruhr Universitaet Bochum, Germany
SAIC, 10260 Campus Point Drive, San Diego, CA 92121-1578, USA Science Inc., San Diego, CA, USA;
Predictive Science, Inc., San Diego, CA, USA;
Predictive Science Incorporate, San Diego, CA, USA;
Akademiia Nauk SSSR, Fizicheskii Institut, Moscow, USSR
University of St. Andrews, Fife, UK
Institut für Theoretische Physik, Ruhr-Universität Bochum, D-44780 Bochum, Germany Science, Inc., 11337 Seda Place, San Diego, CA 92124, USA
Theoretische Physik IV, Ruhr-Universität Bochum, 44780 Bochum, Germany
AN SSSR, Fizicheskii Institut, Moscow, USSR
Academy of Sciences, Pereslavl-Zalessky, Russia
Theoretische Physik IV, Ruhr-Universität Bochum, 44780 Bochum, Germany of Mathematical and Computational Sciences, University of St. Andrews
Theoretische Physik IV, Ruhr Universität Bochum, 44780 Bochum, Germany
Predictive Science, Inc, San Diego, CA, USA
Predictive Science, Inc., San Diego, CA, USA
Russian Academy of Sciences, Program Systems Institute, Pereslavl-Zalesski, Russia
Science Applications International Corporation, 10260 Campus Point Drive, San Diego, CA 92121, USA Applications International Corporation, 10260 Campus Point Drive, San Diego, CA 92121-1578, USA Systems Institute of the Russian Academy of Sciences
Predictive Science Inc, San Diego, CA, USA
Program Systems Institute of the Russian Academy of Sciences Pereslavl-Zalessky 152140, Russia
Predictive Science, Inc., 9990 Mesa Rim Rd., Ste. 170, San Diego, CA 92121, USA
Predictive Science, Inc., 9990 Mesa Rim Road, Suite 170, San Diego, CA 92121-2910, USA
A 2-D Model for the Support of a Polar-Crown Solar Prominence
A 2-D model for the support of a polar-crown solar prominence
A model for magnetically coupled sympathetic eruptions
A Model for the Sources of the Slow Solar Wind
A model for X-ray bright points due to unequal cancelling flux sources
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