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Magnetohydrodynamic simulation of a solar flare: 2. Flare model and simulation using active-region m...

Magnetohydrodynamic simulation of a solar flare: 2. Flare model and simulation using active-region m...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1011211649

Magnetohydrodynamic simulation of a solar flare: 2. Flare model and simulation using active-region magnetic maps

About this item

Full title

Magnetohydrodynamic simulation of a solar flare: 2. Flare model and simulation using active-region magnetic maps

Publisher

Dordrecht: SP MAIK Nauka/Interperiodica

Journal title

Geomagnetism and Aeronomy, 2012-04, Vol.52 (2), p.162-175

Language

English

Formats

Publication information

Publisher

Dordrecht: SP MAIK Nauka/Interperiodica

More information

Scope and Contents

Contents

The results of a three-dimensional MHD simulation and data obtained using specialized spacecraft made it possible to construct an electrodynamic model of solar flares. A flare results from explosive magnetic reconnection in a current sheet above an active region, and electrons accelerated in field-aligned currents cause hard X rays on the solar sur...

Alternative Titles

Full title

Magnetohydrodynamic simulation of a solar flare: 2. Flare model and simulation using active-region magnetic maps

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_1011211649

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1011211649

Other Identifiers

ISSN

0016-7932

E-ISSN

1555-645X,0016-7940

DOI

10.1134/S0016793212020119

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