Observations of X-ray jets with the YOHKOH Soft X-ray Telescope

Details Observations of X-ray jets with the YOHKOH Soft X-ray Telescope Observations of X-ray jets with the YOHKOH Soft X-ray Telescope

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasj...44l.173s&link_type=abstract

PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 44, no. 5, p. L173-L179.

Astronomy and Astrophysics

Astronomy

270

Plasma Jets, Solar Corona, Solar X-Rays, Spaceborne Astronomy, X Ray Telescopes, Japanese Spacecraft, Solar Magnetic Field

Scientific paper

The features of the multiple X-ray jets in the solar corona, revealed by the time series of the Yohkoh Soft X-ray Telescope images are described. The typical size of a jet was from 5 x 10 exp 3 to 4 x 10 exp 5 km, the translational velocity was 30-300 km/s, and the corresponding kinetic energy was estimated to be from 10 exp 25 to 10 exp 28 erg. Many of the jets were found to be associated with flares in X-ray bright points, emerging flux regions, or active regions, and they sometimes occurred several times from the same X-ray feature. One of the jets associated with a flaring bright point was identified as being an H-alpha surge.

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