Bright Points and Coronal Jets as Models for Eruptive Phenomena in the Solar Atmosphere

Details Bright Points and Coronal Jets as Models for Eruptive Phenomena in the Solar Atmosphere Bright Points and Coronal Jets as Models for Eruptive Phenomena in the Solar Atmosphere

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...201.8304f&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #83.04; Bulletin of the American Astronomical Society, Vol. 34, p.1242

Astronomy and Astrophysics

Astronomy

Scientific paper

Bright points in X-rays and EUV are an ever-present phenomena in the solar atmosphere and are often the origin of coronal jets. When bright points are examined at high resolution ( 1 arcesec or less) they show structures remarkably similar in morphology to larger scale coronal structures. Furthermore, their dynamics and evolution also show similarities to larger structures. We examine bright points and coronal jets in X-rays and EUV using Yohkoh SXT, TRACE, and EIT imagery in order to determine the extent to which they can be viewed as miniature counterparts of active regions. This work is supported by NASA contract numbers NAS8-40801, NAS5-38099, NAS5-32966, and Stanford University contract PR9162.

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