Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Rice University
Lanl
U. Innsbruck
Los Alamos National Lab, PO Box 1663, MS D466, Los Alamos, NM 87545, USA
Space Science and Applications, Los Alamos National Lab, Los Alamos, NM, USA;
LANL, Los Alamos, NM, USA;
Space Science and Applications, Los Alamos National Laboratory, Los Alamos, NM, USA;
Space Science and Applications, ISR-1, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
Los Alamos National Laboratory, Los Alamos, New Mexico, USA
Institute of Astrophysics, University of Innsbruck, Technikerst. 25 / 8, A-6020 Innsbruck, Austria
Los Alamos National Laboratory, Space Science & Applications Group, Mail Stop D- 466, Los Alamos, NM 87545, USA
Los Alamos National Laboratory, ISR-1, Space Science and Applications, P.O. Box 1663, MS D466, Los Alamos, NM 87545, USA
Space Science and Applications, ISR-1, MS D466, Los Alamos National Laboratory, Los Alamos, NM 87545, USA
Los Alamos National Laboratory, ISR-1: SPACE SCIENCE AND APPLICATIONS MS D466, Los Alamos, NM 87545, USA
Department of Physics and Astronomy, Rice University Institut für Astrophysik, Universität Innsbruck.
Los Alamos National Laboratory, Space Science and Applications, ISR-1 MS D466, Los Alamos, NM 87544, USA
Los Alamos Natinal Lab, Space Science and Applications ISR-1, MS D466, Los Alamos, NM 87545, USA
Los Alamos National Laboratory, Bikini Atoll Road, Los Alamos, NM 87545, USA
Department of Physics, Faculty of Electrical Engineering, Czech Technical University in Prague, Technicka 2, 166 27 6, Prague, Czech Republic
Los Alamos National Laboratory, ISR-1, MS D466, Los Alamos, NM 87545, USA
Los Alamos National Lab, Space Science and Applications PO Box 1664, MS D466, Los Alamos, NM 87544, USA
Los Alamos National Laboratory, Santa Fe, NM, USA
Los Alamos National Lab, Los Alamos, NM, USA
Los Alamos Na
A Statistical Investigation of Electron Radiation Belt Responses to Transient Solar Wind Drivers over a Range of L-values
A study of energetic electrons near the last closed drift shell using THEMIS-SST data
Air Force Data Assimilative Photospheric Flux Transport (ADAPT) Model
Artificial Neural Network L* from different magnetospheric field models
Comet Hale-Bopp over Innsbruck
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