Log in to save to my catalogue

The role of non-axisymmetry of magnetic flux rope in constraining solar eruptions

The role of non-axisymmetry of magnetic flux rope in constraining solar eruptions

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_7985afaf78ce4f84b94ba50eb7fd66be

The role of non-axisymmetry of magnetic flux rope in constraining solar eruptions

About this item

Full title

The role of non-axisymmetry of magnetic flux rope in constraining solar eruptions

Author / Creator

Publisher

London: Nature Publishing Group UK

Journal title

Nature communications, 2021-05, Vol.12 (1), p.2734-2734, Article 2734

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

Contents

Whether a solar eruption is successful or failed depends on the competition between different components of the Lorentz force exerting on the flux rope that drives the eruption. The present models only consider the strapping force generated by the background magnetic field perpendicular to the flux rope and the tension force generated by the field...

Alternative Titles

Full title

The role of non-axisymmetry of magnetic flux rope in constraining solar eruptions

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_doaj_primary_oai_doaj_org_article_7985afaf78ce4f84b94ba50eb7fd66be

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_7985afaf78ce4f84b94ba50eb7fd66be

Other Identifiers

ISSN

2041-1723

E-ISSN

2041-1723

DOI

10.1038/s41467-021-23037-8

How to access this item