Bi-Directional Jets at Coronal Hole Boundaries

Details Bi-Directional Jets at Coronal Hole Boundaries Bi-Directional Jets at Coronal Hole Boundaries

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.547..397m&link_type=abstract

Proceedings of 'SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO a

Computer Science

Sun, Coronal Hole, Magnetic Reconnection, Bi-Directional Jets

Scientific paper

Our study reveals, for the first time, the presence of bi-directional jets which are considered to be signatures of magnetic reconnection occurring along coronal hole boundaries. The SUMER observations obtained in Ne VIII 770.42 Å (6 10 K) and N IV 765.15 Å (1.3 10 K) show small regions of a few arcsec size with strong blueand red-shifted emission reaching Doppler shifts up to 150 km s which appear along the coronal hole boundaries where evolving loop systems are present.

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