2014-10-20T20:14:27.000Z http://sot.lmsal.com Ted Tarbell LMSAL http://lmsal.com 3251 Hanover Rd, O/ADBS, B/252, Palo Alto, CA, 94304 +1-650-424-2400 tarbell@lmsal.com Hinode SOT Arikawa Arikawa DeRosa(RCO) 267 267 null HOP267 (coronal plumes) LO LO Loops 16 819 -389 0 0 2014-10-18T22:04:00.000Z 2014-10-19T01:59:35.000Z 819 -389 Fan loop footpoints AR mode Case 2 (AR medium) Ca and Na V/I 3 min, G band 60 min, BFI Full FOV 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.