X-ray Jets in Interconnecting Loops

Details X-ray Jets in Interconnecting Loops X-ray Jets in Interconnecting Loops

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002soph..206..143f&link_type=abstract

Solar Physics, v. 206, Issue 1, p. 143-154 (2002).

Physics

3

Scientific paper

We present examples of X-ray jets, observed by the Soft X-ray Telescope on board Yohkoh, which followed trajectories of transequatorial interconnecting loops (TILs). All these TILs were preexisting, seen some time before, but were 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 close to 350 km s-1), but may reach larger lengths, in our examples up to 450 000 km. Exceptions are one jet that moved slower and one that had no brightened area at its supposed source region at the time of its origin (an X-ray bright point appeared there only 3 hours later). It appears that quite a high number of X-ray jets may be of this TIL-associated kind.

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