Three-dimensional simulation of solar emerging flux using the Earth Simulator I. Magnetic Rayleigh-Taylor instability at the top of the emerging flux as the origin of filamentary structure

Publications of the Astronomical Society of Japan

Volumn 58, Issue 2, 2006, Pages 423-438

  Isobe, Hiroaki ^a,b,c   Miyagoshi, Takehiro ^c   Shibata, Kazunari ^c   Yokoyama, Takaaki ^a  

^a UNIVERSITY OF TOKYO   (Japan)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c KYOTO UNIVERSITY   (Japan)

Author keywords

Magnetohydrodynamics: MHD; Sun: choromosphere; Sun: corona; Sun: filaments

Indexed keywords

RAYLEIGH SCATTERING; STABILITY; SUN; X RAY MICROSCOPES;

CURRENT SHEETS; EARTH SIMULATORS; FILAMENTARY STRUCTURES; FINE STRUCTURES; MAGNETOHYDRODYNAMIC SIMULATIONS; MAGNETOHYDRODYNAMIC: MHD; SUN : CORONA; SUN: CHOROMOSPHERE; SUN: FILAMENTS; THREE DIMENSIONAL SIMULATIONS; MAGNETOHYDRODYNAMIC; SUN: CHROMOSPHERE;

MAGNETOHYDRODYNAMICS;

EID: 33646814746     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/58.2.423     Document Type: Review

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