THE COLLAPSE OF TURBULENT CORES AND RECONNECTION DIFFUSION

Fast magnetic reconnection, which takes place in the presence of turbulence, can induce a process of reconnection diffusion that has been elaborated on in earlier theoretical works. We have named this process turbulent reconnection diffusion, or simply RD. This paper continues our numerical study of...

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Veröffentlicht in:	The Astrophysical journal 2013-11, Vol.777 (1), p.1-23
Hauptverfasser:	Leao, M R M, DAL PINO, E M DE GOUVEIA, Santos-Lima, R, Lazarian, A
Format:	Artikel
Sprache:	eng
Schlagworte:	ALFVEN WAVES ASTRONOMY ASTROPHYSICS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Clouds Collapse COMPARATIVE EVALUATIONS Computational fluid dynamics DECOUPLING DIFFUSION Fluid flow Gravitation GRAVITATIONAL COLLAPSE GRAVITATIONAL FIELDS MAGNETIC FIELDS MAGNETIC FLUX MAGNETIC RECONNECTION MAGNETOHYDRODYNAMICS NUMERICAL ANALYSIS POTENTIALS STARS TURBULENCE Turbulent flow
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