Envelope Soliton in Solar Radio Emission

Details Envelope Soliton in Solar Radio Emission Envelope Soliton in Solar Radio Emission

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000chphl..17..355w&link_type=abstract

Chinese Physics Letters, Volume 17, Issue 5, pp. 355-357 (2000).

Physics

1

Scientific paper

Several envelope soliton fine structures have been observed in solar radio metric-wave emission. We present a model of longitudinal modulational instability to explain these fine structures. It is found that this instability can only occur in the condition of sound velocity being larger than Alfvén velocity in corona. Therefore, the envelope soliton fine structures should display in the coronal region with high temperature and low magnetic field, which corresponds to the solar radio emission in the region of meter and decameter wavelength.

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