Fig. 35.
![EIS has measured relatively narrow temperature distributions for many 1 MK loops. The top panel shows an EIS 195.119 Å raster over an active region, which has been sharpened to help identify the loops. The bottom panel shows the DEM computed from observations of 12 emission lines in a small segment of the loop. The emission lines range in temperature from Si vii to Fe xvi. [Adapted from Warren et al. (2008) by permission of the AAS.] (Color online)](https://oup.silverchair-cdn.com/oup/backfile/Content_public/Journal/pasj/71/5/10.1093_pasj_psz084/2/pasj_71_5_r1_f29.jpeg?Expires=1750066856&Signature=v81s7kZxzbrGUnjABG~b8Hocu~Q2PDfWhXo3oblgzmH8Q-VRkk20dQX4IKe2JMKwBiYo4~U5Wsvx177JYzhsjqA9DAi02900pfnQLA8slcSCVn25rbla4TpcyQvD5gOYkwYkKCtyWcz1hr6ykT97NShTWjSYFfCirvHRY02qv7SR8tpPPbTVteavlGiYDYO-Kv2Ooz2n4ontC-bAtiRW8oVc8--ZzY-CG2ou9xgynclXbZMWxracSrwnpZC6RiLCHcOOU-hy-f-cgOoxQcMUdMDARnOYXf6UfAGzUVEFbfMz8aMHXmXrzKzFNnnLYyc0aakBzB-NXFyvTEvbr1DT2g__&Key-Pair-Id=APKAIE5G5CRDK6RD3PGA)
EIS has measured relatively narrow temperature distributions for many 1 MK loops. The top panel shows an EIS 195.119 Å raster over an active region, which has been sharpened to help identify the loops. The bottom panel shows the DEM computed from observations of 12 emission lines in a small segment of the loop. The emission lines range in temperature from Si vii to Fe xvi. [Adapted from Warren et al. (2008) by permission of the AAS.] (Color online)
