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Yokoyama Takaaki - Department of Earth and Planetary Science, University of Tokyo
Magnetohydrodynamic Simulation Solar Coronal X-ray Jets
What is the Condition for Fast Magnetic Reconnection ? T. Yokoyama and K. Shibata
What is the Condition for Fast Magnetic Reconnection ? T. Yokoyama and K. Shibata
Magnetohydrodynamic Simulation of
PASJ: Publ. Astron. Soc. Japan 48, -16 (1997) Numerical Simulation of Solar Coronal X-Ray Jets Based on the
Magnetic Reconnection as the Origin of both X-ray Jets and Hff Surges on the Sun
Will be published in 1997 Jan. 1 i* *ssue of ApJL
