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pro vyhledávání: '"Ohsaki, Shuichi"'
By modelling the coronal structures by "slowly" evolving Double-Beltrami two-fluid equilibria (created by the interaction of the magnetic and velocity fields), the conditions for catastrophic transformations of the original state are derived. It is s
Externí odkaz:
http://arxiv.org/abs/astro-ph/0104138
Autor:
OHSAKI, SHUICHI1 shuichi.ohsaki@barcap.com, YAMAZAKI, AKIRA2,3 akira-yamazaki@fintec.co.jp
Publikováno v:
International Journal of Theoretical & Applied Finance. Mar2011, Vol. 14 Issue 2, p239-264. 26p.
Publikováno v:
Journal of Plasma Physics; Dec2006, Vol. 72 Issue 6, p965-970, 6p
Publikováno v:
Physics of Plasmas; Sep2005, Vol. 12 Issue 9, p092901, 5p, 4 Diagrams, 1 Chart
Publikováno v:
Physics of Plasmas; Sep2005, Vol. 12 Issue 9, p092308, 7p, 5 Diagrams
Autor:
Ohsaki, Shuichi, Yoshida, Zensho
Publikováno v:
Physics of Plasmas; Jun2005, Vol. 12 Issue 6, p064505, 4p
Publikováno v:
Physics of Plasmas; Dec2004, Vol. 11 Issue 12, p5643-5647, 5p