Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Department of Physics, Montana State University, EPS 264B, P.O. Box 173840, Bozeman, MT 59717-3840 of Astronomy and Space Science, School of Space Research, Kyung Hee University, 1, Seocheon-dong, Giheung-gu, Yongin, Gyeonggi-do, 446-701, Korea; Project Office, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588
Montana State University
National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan
Dept. of Astronomy and Space Science, Kyung Hee University, Yongin, 446-701, Korea
Hinode Science Center, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588
SSL, UC Berkeley, 7 Gauss Way, Berkeley, CA 94720-7450, USA Astronomical Observatory of Japan
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka-shi, Tokyo 181-8588, Japan
Space Sciences Laboratory, University of California, Berkeley, CA 94720-7450, USA; Naval Research Laboratory, Code 7675, Washington DC 20375-2352, USA
Kyung Hee Univ., Gyeonggi-do, Republic of Korea; of Astronomy and Space Science, School of Space Research, Kyung Hee University, Yongin, Republic of Korea; of Physics, Montana State University, P.O. Box 173840, Bozeman, MT 59717-3840
Department of Physics, Montana State University, Bozeman, MT 59717-3840 / UCB, SSL
National Astronomical Observatory, Mitaka, Tokyo 181-8588, Japan.
Kwasan Observatory, Kyoto University, Kyoto 607-8471, Japan 2-21-1 Osawa, Mitaka, 181-858, Japan
Montana State University, Department of Physics, EPS 264 Montana State University, Bozeman, MT 59717-3840, USA Science Cente
3-DIMENSIONAL Evolution of a Magnetic Flux Tube Emerging Into the Solar Atmosphere
3-dimensional Evolution of an Emerging Flux Tube in the Sun
3-Dimensional Evolution of an Emerging Flux Tube in the Sun
3-dimensional MHD Simulation of Emerging Flux Tubes
A Comparison of the Minimum Current Corona to a Magnetohydrodynamic Simulation of Quasi-Static Coronal Evolution
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