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Corona and upper transition region(radi<strong>at</strong>ion+conduction+solar wind)QuietActiveTemper<strong>at</strong>ure (K)6 .10 6 Vernazza & Reeves d<strong>at</strong>aDeere et alSRPM 10014 .10 62 . 10 6Temper<strong>at</strong>ure (K)6 . 10 6 AR Vernazza & Reeves d<strong>at</strong>aAR Deere et alSRPM 10154 .10 62 .10 65 .10 9 1 .10 10 1.5 .10 10 2 .10 10 2.5 .10 105 .10 9 1 .10 10 1.5 .10 10 2 .10 10 2.5 .10 10Height (cm)Height (cm)The temper<strong>at</strong>ure reaches a maximum value (local energy dissip<strong>at</strong>ionis essential) and decreases again in the heliosphere. DEM cannothandle this behavior. <strong>Solar</strong> wind and coronal holes are fe<strong>at</strong>ures toconsider. In active regions, groups of hot loops are the key fe<strong>at</strong>ure.
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