Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
SSL / UCB
Space Science Laboratory, University of California, Berkeley
Space Sciences Laboratory, University of California, Berkeley, CA 94720-7450, USA
Space Sciences Lab, Univ California, Berkeley, CA, USA;
Space Sciences Laboratory, University of California, Berkeley, CA, USA;
Space Sci Lab, Univ California Berkeley, Berkeley, CA, USA;
Space Science Lab #7450, Univ California Berkeley, Berkeley, CA, USA;
Space Sciences Laboratory, Univ. of California-Berkeley, Berkeley, CA, USA;
UC Berkeley
Space Sciences Laboratory, UC Berkeley
Space Sciences Laboratory, University of California, 7 Gauss Way, Berkeley, CA 94720-7450; Kavli Institute for Theoretical Physics, Kohn Hall, University of California, Santa Barbara, CA 93106-4030.
California Univ., Berkeley
UC, Berkeley
UC-Berkeley
SSL / UC Berkeley
Lawrence Livermore National Lab., Calif.
SSL, UC Berkeley
University of California Berkeley, Space Sciences
Space Sciences Laboratory, University of California, Berkeley, California 94720-7450
Space Sciences Laboratory, University of California, Berkeley, California, USA
California, University, La Jolla, CA
UC Berkeley, Space Sciences Laboratory #7450, Berkeley, CA 94720-7450, USA
UC Berkeley, Space Sciences Laboratory #7450, Berkeley, CA 94720, USA
Space Sciences Laboratory, University of California
National Solar Observatory, Tucson, AZ
UCB / SSL
SSL / University of California
California Univ., San Diego.
UC Berkeley, Space Sciences Laboratory University of California 7 Gauss Way, Berkeley, CA 97420-7450, USA
Space Sciences Lab, UC-Berkeley, 7 Gauss Way, Berkeley, CA 94720-7450, USA
UC Berkeley, Space Sciences Laboratory # 7450 7 Gauss Way U
3-D MHD Simulations of Flux Tube Emergence
3D MHD Simulation of Flux Tube Dynamics: Comparison with Thin Flux Tube Models
A CME Model for the 1992 July 15 AU MIC Flare Observed by EUVE
A coronal mass ejection model for the 1992 July 15 flare on AU Microscopii observed by the extreme ultraviolet explorer
A Coupled Model for the Emergence of Active Region Magnetic Flux into the Solar Corona
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Profile ID: LFWR-SCP-P-20277