Comparison between Yohkoh soft x-ray images and 3D MHD simulations of solar emerging flux regions. [MHD (Magnetohydrodynamic)]
Ryōji Matsumoto(The University of Texas at Austin), N. Nitta, L. Acton, K. T. Strong(University College London), M. Kaisig, H. Kurokawa, Maki Akioka(National Institute of Information and Communications Technology), Y. Ishido, T. Tajima, S. Tsuneta(The University of Tokyo), Katsunori M. Shibata(The Graduate University for Advanced Studies, SOKENDAI), Goro Kawai
OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information)
January 1, 1992
Cited by 0
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