000003473 001__ 3473
000003473 005__ 20180129172145.0
000003473 037__ $$aPOSTER-2018-0036
000003473 100__ $$aWest, Matthew
000003473 245__ $$aFurther Exploration Of Post-Flare Giant Arches
000003473 260__ $$c2017
000003473 269__ $$c2017-08-05
000003473 520__ $$aRecent observations from the SWAP EUV imager on-board PROBA2 and SXI X-ray observations from the GOES satellite have shown that post-flare giant arches and regular post-flare loops are one and the same thing. However, it is still not clear how certain loop systems are able to sustain prolonged growth to heights of approximately 400000 km (>0.5 solar-radii). In this presentation we further explore the energy deposition rate above post-flare loop systems through high-energy RHESSI observations. We also explore the difference between the growth of different loop systems through an epoch analysis, and the difference between their on-disk and on-limb signatures.
000003473 536__ $$a3ESA_PROBA2SOC/$$c3ESA_PROBA2SOC/$$f3ESA_PROBA2SOC
000003473 594__ $$aNO
000003473 700__ $$aSeaton, Daniel
000003473 700__ $$aDennis, Brian
000003473 700__ $$aFeng, Li
000003473 700__ $$aPalmerio, Erika
000003473 773__ $$tESPM-15, Budapest, Hungary
000003473 8560_ $$fmatthew.west@observatoire.be
000003473 85642 $$ahttp://astro.elte.hu/ESPM-15/subindex.php?lang=en&page=sciprogramme
000003473 980__ $$aCPOSTER