6948 20240326143854.0 POSTER-2024-0059 Gorman, J. Diffuse Quiet Solar Corona 2024 2024-04-09 The 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 STCE Solar Orbiter EUI corona Chitta, L.P. Peter, H. Berghmans, D. Auchère, F. Aznar Cuadrado, R. Teriaca, L. Solanki, S.K. Verbeeck, C. Kraaikamp, E. Stegen, K. Gissot, S. Joint Solar Orbiter, Parker Solar Probe, and DKIST Meeting david.berghmans@ksb-orb.be https://eclipse2024sa.com CPOSTER