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Magnetic field topology from non-force free extrapolation and magnetohydrodynamic simulation of its...

Magnetic field topology from non-force free extrapolation and magnetohydrodynamic simulation of its...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_crossref_primary_10_1017_S1743921318001163

Magnetic field topology from non-force free extrapolation and magnetohydrodynamic simulation of its eventual dynamics

About this item

Full title

Magnetic field topology from non-force free extrapolation and magnetohydrodynamic simulation of its eventual dynamics

Publisher

Cambridge, UK: Cambridge University Press

Journal title

Proceedings of the International Astronomical Union, 2018-02, Vol.13 (S340), p.183-184

Language

English

Formats

Publication information

Publisher

Cambridge, UK: Cambridge University Press

Subjects

Subjects and topics

More information

Scope and Contents

Contents

Magnetic reconnections (MRs) for various magnetic field line (MFL) topologies are believed to be the initiators of solar eruptive events like flares and coronal mass ejections (CMEs). Consequently, important is a thorough understanding and quantification of the MFL topology and their evolution which leads to MRs. Contemporary standard is to extrapo...

Alternative Titles

Full title

Magnetic field topology from non-force free extrapolation and magnetohydrodynamic simulation of its eventual dynamics

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_crossref_primary_10_1017_S1743921318001163

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_crossref_primary_10_1017_S1743921318001163

Other Identifiers

ISSN

1743-9213

E-ISSN

1743-9221

DOI

10.1017/S1743921318001163

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