Slowly moving disturbances in the X-ray corona

Details Slowly moving disturbances in the X-ray corona Slowly moving disturbances in the X-ray corona

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...63..279r&link_type=abstract

Solar Physics, vol. 63, Sept. 1979, p. 279-295.

Astronomy and Astrophysics

Astronomy

13

Magnetohydrodynamics, Skylab Program, Solar Corona, Solar X-Rays, X Ray Astronomy, Filaments, H Alpha Line, Propagation Velocity, Satellite Observation, Solar Flares

Scientific paper

Sequences of soft X-ray pictures, taken aboard Skylab between May and November, 1973, have made it possible to detect slowly moving disturbances originating in disrupted filaments and causing subsequent brightenings of distant coronal structures. With speeds decreasing from approximately 400 km/sec shortly after the filament disruption to approximately 10 km/sec four or five hours later, these disturbances appear to be identical with slow waves earlier inferred by Bruzel (1952, 1969), Oehman (1953), and Yajima (1971) from chromospheric observations.

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