Formation of a Kinked Alignment of Solar Active Region View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1996

AUTHORS

R. Matsumoto , T. Tajima , W. Chou , K. Shibata

ABSTRACT

Images of the solar corona as observed by the soft X-ray telescope aboard the Yohkoh satellite sometimes show a sequence of S-shaped X-ray emitting regions in the low latitudes of the northern or southern hemisphere (Matsumoto et al. 1996). Such a structure suggests that they are emergent portions of a submerged large scale helical flux tube in the convection zone. When the magnetic twist exceeds a threshold value, the flux tube deforms itself into a helical structure through the kink instability. We have carried out three-dimensional MHD simulations of such a kink-unstable flux tube in a convectively unstable gas layer. Here we briefly describe our model and numerical results (see Matsumoto et al. 1996 for details). More... »

PAGES

355-356

Book

TITLE

Magnetodynamic Phenomena in the Solar Atmosphere

ISBN

978-94-010-6627-3
978-94-009-0315-9

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-94-009-0315-9_66

DOI

http://dx.doi.org/10.1007/978-94-009-0315-9_66

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1014128146


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