Self-Generated Inhomogeneous Magnetic Fields in Auroral Zones with Kilometric Radiation

Details Self-Generated Inhomogeneous Magnetic Fields in Auroral Zones with Kilometric Radiation Self-Generated Inhomogeneous Magnetic Fields in Auroral Zones with Kilometric Radiation

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ap%26ss.253..253l&link_type=abstract

Astrophysics and Space Science, Volume 253, Issue 2, pp.253-263

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

It is analytically indicated that self-generated magnetic fields are modulationally unstable with respect to the uniform state of a plasma; such an instability would cause the formation of the field localization. It is able to expect that this localized magnetic flux is responsible for small-scale inhomogeneous magnetic fields, which are required for explanation of the fine structure of auroral kilometric radiaton (AKR).

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