COOL TRANSITION REGION LOOPS OBSERVED BY THE INTERFACE REGION IMAGING SPECTROGRAPH

We report on the first Interface Region Imaging Spectrograph (IRIS) study of cool transition region loops, a class of loops that has received little attention in the literature. A cluster of such loops was observed on the solar disk in active region NOAA11934, in the Si IV 1402.8 angstrom spectral raster and 1400 slit-jaw images images. We divide the loops into three groups and study their dynamics. The first group comprises relatively stable loops, with 382-626 km cross-sections. Observed Doppler velocities are suggestive of siphon flows, gradually changing from -10 km s(-1) at one end to 20 km s(-1) at the other end of the loops. Nonthermal velocities of 15 similar to 25 km s(-1) were determined. Magnetic cancellation with a rate of 10(15) Mx s(-1) is found at the blueshifted footpoints. These physical properties suggest that these loops are impulsively heated by magnetic reconnection, and the siphon flows play an important role in the energy redistribution. The second group corresponds to two footpoints rooted in mixed-magnetic-polarity regions, where magnetic cancellation with a rate of 10(15) Mx s(-1) and explosive-event line profiles with enhanced wings of up to 200 km s(-1) were observed. In the third group, interaction between two cool loop systems is observed. Evidence for magnetic reconnection between the two loop systems is reflected in the explosive-event line profiles and magnetic cancellation with a rate of 3 x 10(15) Mx s(-1) observed in the corresponding area. The IRIS has provided opportunity for in-depth investigations of cool transition region loops. Further numerical experiments are crucial for understanding their physics and their roles in the coronal heating processes.