Parker's dynamo near the excitation threshold

Details Parker's dynamo near the excitation threshold Parker's dynamo near the excitation threshold

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010arep...54..762s&link_type=abstract

Astronomy Reports, Volume 54, Issue 8, pp.762-766

Astronomy and Astrophysics

Astronomy

Scientific paper

A method of constructing asymptotic solutions for nonlinear mean-field dynamo equations near the excitation threshold is developed and applied to equations describing the solar dynamo in a Parker model. The form of solution obtained corresponds to the eigensolution for a kinematic dynamo, for the intensity of the generation sources at which self-excitation of the magnetic field begins (the so-called marginally stable eigenfunction). The wave amplitude is calculated.

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