X-Ray Jets in Interconnecting Loops

Details X-Ray Jets in Interconnecting Loops X-Ray Jets in Interconnecting Loops

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mwoc.conf...81f&link_type=abstract

Multi-Wavelength Observations of Coronal Structure and Dynamics -- Yohkoh 10th Anniversary Meeting. Proceedings of the conferenc

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Scientific paper

We present several examples of X-ray jets, observed by the SXT onboard Yohkoh, which followed trajectories of transequatorial interconnecting loops (TILs). All these TILs were preexisting, seen some time before, but mostly invisible at the time of the onset of the jet which often made them bright along their total length. With few exceptions, these TIL-associated jets have properties very similar to other jets ejected inside active regions or along open field lines (footpoints in X-ray bright points, recurrence, strong collimation, average speed between 340 and 380 km s-1, but may reach very large lengths, in excess of 450 000 km. Exceptions are one jet that moved slower and one that had no brightened area at its source region at the time of its origin (an X-ray bright point appeared there only 3 hours later). It appears that less than 20% of X-ray jets are of this kind.

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