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A magnetohydrodynamic simulation study of Kronian field-aligned currents and auroras

A magnetohydrodynamic simulation study of Kronian field-aligned currents and auroras

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1093439178

A magnetohydrodynamic simulation study of Kronian field-aligned currents and auroras

About this item

Full title

A magnetohydrodynamic simulation study of Kronian field-aligned currents and auroras

Publisher

Washington, DC: Blackwell Publishing Ltd

Journal title

Journal of Geophysical Research: Space Physics, 2012-02, Vol.117 (A2), p.n/a

Language

English

Formats

Publication information

Publisher

Washington, DC: Blackwell Publishing Ltd

More information

Scope and Contents

Contents

Magnetohydrodynamic simulations of the interaction of Saturn's magnetosphere with the solar wind indicate that Kelvin‐Helmholtz (K‐H) waves can form on the dayside magnetopause when the interplanetary magnetic field (IMF) is northward. Dayside magnetic reconnection occurs at Saturn for northward IMF, and the combination of K‐H waves and reconnectio...

Alternative Titles

Full title

A magnetohydrodynamic simulation study of Kronian field-aligned currents and auroras

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_1093439178

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1093439178

Other Identifiers

ISSN

0148-0227,2169-9380

E-ISSN

2156-2202,2169-9402

DOI

10.1029/2011JA016945

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