A comparison of high-energy events in the quiet sun with solar flares

Details A comparison of high-energy events in the quiet sun with solar flares A comparison of high-energy events in the quiet sun with solar flares

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...86..259b&link_type=abstract

(Japan Society for the Promotion of Science and National Science Foundation, U.S.-Japan Seminar on the Recent Advances in the Un

Physics

2

Solar Corona, Solar Flares, Stellar Mass Ejection, Acceleration (Physics), High Resolution, Oso-7, Scaling Laws, Skylab Program

Scientific paper

Observations of high-speed coronal clouds (OSO-7), flare ejecta (Skylab) and high-energy jets (HRTS) are compared. It is possible that the same physical mechanism - an expanding loop - which is responsible for the high speed jets (400 km sec-1, 2.5×1026 ergs) can also account for the high-speed coronal clouds (1300 km sec-1, 4×1030 ergs), which were correlated with a flare-connected spray. Field strength of 15 gauss and 2500 gauss are required for the jets and the sprays, respectively.

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