3D MHD Simulation of Magnetic Flux Tubes in Co-Rotating Coordinates View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1996

AUTHORS

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

ABSTRACT

The solar soft X-ray pictures taken by the Yohkoh satellite show a sequence of regularly spaced, S-shaped active regions at low latitude of the north and the south hemispheres. It appears that these active regions are emergent parts, due to magnetic buoyancy (Parker) instability, of a global helical magnetic flux tube embedded in the convection zone. Also, the sunspots, which are the foot points of the emergent flux tube, are arranged as: the preceding polarity of an active region tends to be near the equator, whereas the following polarity is farther from the equator. Here in this paper, we simulate a 3-D flux tube to compare with these observations. More... »

PAGES

613-614

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_164

DOI

http://dx.doi.org/10.1007/978-94-009-0315-9_164

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1015992254


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