Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
University of California
University of California, Berkeley
Kavli Institute for Theoretical Physics, University of California, Santa Barbara, CA 93106; Space Sciences Laboratory, University of California, Berkeley, CA 94720.
UC, Berkeley
Space Sciences Laboratory, University of California, Berkeley, CA 94720-7450, USA
Space Sciences Laboratory, University of California, Berkeley, CA, USA;
Space Science Lab #7450, Univ California Berkeley, Berkeley, CA, USA;
Space Sciences Laboratory, 7 Gauss Way, University of California, Berkeley, CA 94720-7450
UC Berkeley
Space Science Lab, UC Berkeley
Space Sciences Laboratory, University of California, 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.
Space Sciences Laboratory, University of California, Berkeley, 94720-7450
Space Sciences Laboratory, University of California, Berkeley, California 94720-7450
UC Berkeley, Space Sciences Laboratory #7450, Berkeley, CA 94720, USA
SSL / University of California
Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA
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
Space Sciences Laboratory, University of California, Berkeley, CA 94720-7450
Space Sciences Lab, University of California, Berkeley, CA 94720, USA
Space Sciences Laboratory, Berkeley, CA, USA
SSL, University of California at Berkeley, Berkeley, C
3-D MHD Simulations of Flux Tube Emergence
3D MHD Simulation of Flux Tube Dynamics: Comparison with Thin Flux Tube Models
3D MHD Simulations of Magnetic Flux Emergence in Active Regions
3D simulation of flux emergence from convective zone to corona with BATSRUS
A Coupled Model for the Emergence of Active Region Magnetic Flux into the Solar Corona
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Profile ID: LFWR-SCP-P-45315