000006948 001__ 6948
000006948 005__ 20240326143854.0
000006948 037__ $$aPOSTER-2024-0059
000006948 100__ $$aGorman, J.
000006948 245__ $$aDiffuse Quiet Solar Corona
000006948 260__ $$c2024
000006948 269__ $$c2024-04-09
000006948 520__ $$aThe quiet Sun corona imaged at 1 MK mostly consists of diffuse emission that lacks the spatial structuring seen in coronal loops or bright points. These diffuse regions, despite having a total intensity comparable to a bright point, have only very small intensity fluctuations. Data are inconsistent with driver being power-law-like distribution of discrete heating events
000006948 594__ $$aSTCE
000006948 6531_ $$aSolar Orbiter
000006948 6531_ $$aEUI
000006948 6531_ $$acorona 
000006948 700__ $$aChitta, L.P.
000006948 700__ $$aPeter, H.
000006948 700__ $$aBerghmans, D.
000006948 700__ $$aAuchère, F.
000006948 700__ $$aAznar Cuadrado, R.
000006948 700__ $$aTeriaca, L.
000006948 700__ $$aSolanki, S.K.
000006948 700__ $$aVerbeeck, C.
000006948 700__ $$aKraaikamp, E.
000006948 700__ $$aStegen, K.
000006948 700__ $$aGissot, S.
000006948 773__ $$tJoint Solar Orbiter, Parker Solar Probe, and DKIST Meeting
000006948 8560_ $$fdavid.berghmans@ksb-orb.be
000006948 85642 $$ahttps://eclipse2024sa.com
000006948 980__ $$aCPOSTER