Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Space Sciences Laboratory, University of California, Berkeley, California, USA
University of Berkeley-SSL, Berkeley, CA
University of California, Berkeley, Space Sciences Laboratory, 7 Gauss Way, Berkeley, CA 94720, USA
Space Sciences Laboratory, University of California, Berkeley 7 Gauss Way #7450, Berkeley, CA 94720, USA
Space Sciences Laboratory, University of California Berkeley, 7 Gauss Way, Berkeley, CA 94720-7450 USA
Space Science Laboratory, Berkeley, USA
Space Sciences Laboratory, University of California at Berkeley, 7 Gauss Way #7450, Berkeley, CA 94720-7450, USA
Space Sciences Laboratory, University of California, Centennial Drive at Grizzly Peak Blvd., Berkeley, CA 94720, USA; Département de Recherche Spatiale, CNRS UMR-8632, Observatoire de Paris, 5 Place Jules Janssen, Meudon, 92195 France
Space Sciences Laboratory, University of California, Berkeley, CA 94720-7450, USA
Space Science Laboratory, University of California, Berkeley, 7 Gauss Way, Berkeley, CA 94720, USA
Space Sciences Laboratory, University of California, 7 Gauss Way, Berkeley, CA 94720-7450, USA
Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA
Space Sciences Laboratory, 7 Gauss Way, University of California, Berkeley, CA 94720
Space Sciences Lab, Centennial Drive at Grizzly Peak, Berkeley, CA 94720
Space Sciences Laboratory, University of California, 7 Gauss Way, BERKELEY, CA 94704-7450, USA
Space Sciences Laboratory, University of California, Berkeley, CA 94720
An asymmetry of the electron foreshock due to the strahl
Anomalous scaling and the role of intermittency in solar wind MHD turbulence: new insights
Basic Properties of Anisotropic Stellar Wind Expansion in the Fluid Approach
Determination of accurate solar wind electron parameters using particle detectors and radio wave receivers
Determination of accurate Solar Wind electron parameters using particle detectors and radio wave receivers
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