2019-07-31T09:06:05.000Z http://sot.lmsal.com Mr. Sam Freeland Lockheed Martin Solar and Astrophysics Laboratory (LMSAL) http://www.lmsal.com Lockheed Martin Advanced Tech Center, 3251 Hanover Rd, O/ADBS, B/252, Palo Alto, CA 94304 null null HINODE SOT Demoto Yasuda DeRosa (RCO) 0 Synoptic Sun Center DC, SYN DC, SYN 19 19 26 327 163 2015-03-04T18:04:30.000Z 2015-03-04T18:04:53.000Z 19 26 Synoptic Synoptic BFI NFI (revised: small, no mask, Na D cont.) Sunspots often show bright fan loops in the AIA 171 channel, and these are clearly seen in upper transition region lines of EIS where they exhibit downflows of 10-40 km/s. Sunspot plumes are identified as redshifted features seen in transition region lines, and are particularly clearly seen in the IRIS O IV lines, which show velocities of 70-100 km/s. Sunspot plumes are usually narrower than fan loops, but are found in the same locations so they may represent one stage in the evolution of the strands that compose fan loops. This IHOP will take coordinated observations between Hinode and IRIS to investigate the relationship between sunspot plumes and fan loops. ivo://sot.lmsal.com/VOEvent#2015-03-04T18:04:00Z