Computer Science – Numerical Analysis
Scientific paper
Aug 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..673s&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, July-Aug. 1989, p. 673-675. In Russian.
Computer Science
Numerical Analysis
Equatorial Regions, F Region, Geomagnetism, Magnetic Equator, Taylor Instability, Earth Ionosphere, Nonlinear Systems, Numerical Analysis
Scientific paper
An approximate equation is proposed which considers the development of the Rayleigh-Taylor instability (RTI) along the geomagnetic field in the nonlinear regime. Using this equation, it is shown that, at heights with elevated dissipative recombination, the RTI assumes a threshold character with respect to 'bubble' depth and dimensions. A static solution is obtained that describes the 'bubble' as a solitary dissipative structure along the geomagnetic field.
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