000004013 001__ 4013
000004013 005__ 20190131000613.0
000004013 037__ $$aCTALK-2019-0070
000004013 100__ $$aWest, Matthew
000004013 245__ $$aRHESSI SWAP Post-Flare Giant Arch Signatures
000004013 260__ $$c2018
000004013 269__ $$c2018-07-20
000004013 520__ $$aRecent observations from the SWAP EUV imager on board PROBA2, AIA on SDO 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 greater than half a solar radii (> 400000 km). In this presentation we further explore the energy deposition rate above post flare loop systems through high energy RHESSI observations, combined with evidence of supra arcade down flows, indicating ongoing sustained magnetic reconnection.
000004013 536__ $$a3ESA-PROBA2SOC/$$c3ESA-PROBA2SOC/$$f3ESA-PROBA2SOC
000004013 594__ $$aNO
000004013 700__ $$aSeaton , Daniel
000004013 700__ $$aPalmerio, Erika
000004013 700__ $$aDennis, Brian
000004013 700__ $$aSavage, Sabrina
000004013 700__ $$aFeng, Li
000004013 773__ $$tCOSPAR, Pasadena, USA
000004013 8560_ $$fmatthew.west@observatoire.be
000004013 85642 $$ahttps://www.cospar-assembly.org/abstractcd/COSPAR-18/abstracts/E2.2-0009-18.pdf
000004013 906__ $$aContributed
000004013 980__ $$aCTALKCONT