Kilometer-scale fine structures of midlatitude sporadic E (Es) plasma patches have been directly imaged for the first time by an interferogram derived from L band Advanced Land Observation Satellite/Phased Array-type L band Synthetic Aperture Radar data obtained over southwestern Japan. The synthetic aperture radar interferogram captured the eastern part of a large-scale frontal structure of daytime midlatitude Es which spans over 250 km in the east-northeast to west-southwest direction. Fine structures are characterized by frontal and disc-shaped patches which are elongated in the same direction as the large-scale frontal structure. Length and width of the disc-shaped patches are 10-20 km and 5-10km, respectively, and they are quasi-periodically located with a typical separation of 10-15km. The Kelvin-Helmholtz instability with the vertical shear of zonal winds is considered to be the most likely candidate for the generation mechanism of the frontal patch and disc-shaped patches aligned in the zonal direction.
机构:
Ilia Chavchavadze State Univ, Georgian Natl Astrophys Observ, GE-0160 Tbilisi, GeorgiaIlia Chavchavadze State Univ, Georgian Natl Astrophys Observ, GE-0160 Tbilisi, Georgia
Didebulidze, G. G.
;
Lomidze, L. N.
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Ilia Chavchavadze State Univ, Georgian Natl Astrophys Observ, GE-0160 Tbilisi, GeorgiaIlia Chavchavadze State Univ, Georgian Natl Astrophys Observ, GE-0160 Tbilisi, Georgia
机构:
Ilia Chavchavadze State Univ, Georgian Natl Astrophys Observ, GE-0160 Tbilisi, GeorgiaIlia Chavchavadze State Univ, Georgian Natl Astrophys Observ, GE-0160 Tbilisi, Georgia
Didebulidze, G. G.
;
Lomidze, L. N.
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h-index: 0
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Ilia Chavchavadze State Univ, Georgian Natl Astrophys Observ, GE-0160 Tbilisi, GeorgiaIlia Chavchavadze State Univ, Georgian Natl Astrophys Observ, GE-0160 Tbilisi, Georgia