Statistics – Computation
Scientific paper
Sep 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..116..323m&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 116, no. 2, 1988, p. 323-348.
Statistics
Computation
22
Gravitational Fields, Magnetic Field Configurations, Magnetohydrostatics, Type 4 Bursts, Computational Astrophysics, Plasma Resonance, Solar Corona, Sunspots
Scientific paper
A recently proposed very general dynamic model for the interpretation of Zebra patterns (Mollwo, 1983) traces back the observed dynamic spectra to a warm helical electron beam travelling through the magnetically confined plasma of a coronal condensation. Supposing a two-dimensional field configuration it is shown that Zebra patterns with two crossing stripe systems supply an adequate number of parameters to calculate the most essential field quantities for the emitting region. The found magnitude of the magnetic field B is in accordance with the results of potential field calculations (cf. Dulk and McLean, 1978). Four events with very different values of the frequency drift of the Zebra stripes among them one with a typical braided Zebra pattern yield rather similar results. It is pointed out that special variants of the mechanism may account for fiber bursts and perhaps also type III b-bursts.
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