000003547 001__ 3547
000003547 005__ 20180816180805.0
000003547 037__ $$aPOSTER-2018-0042
000003547 100__ $$aWest, Matthew
000003547 245__ $$aPost-Flare Loop Signatures
000003547 260__ $$c2018
000003547 269__ $$c2018-08-03
000003547 520__ $$aRecent observations from the SWAP EUV imager onboard 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, with the former being a sub-set of post-flare loops that are able to maintain their growth to great heights over longer periods. However, it is still not clear how certain loop systems are able to sustain this growth to heights that can exceed half a solar radii (> 400000 km). In this presentation we further explore the energy deposition rate in post-flare loop systems, combined with an epoch analysis of the irradiance light curves generated by the initial flare and subsequent decline in emission generated from the post-flare loop systems.
000003547 536__ $$aPROBA2/$$cPROBA2/$$fPROBA2
000003547 594__ $$aNO
000003547 700__ $$aSeaton, Daniel
000003547 700__ $$aPalmerio, Erika
000003547 773__ $$tSHINE Florida USA
000003547 8560_ $$fmatthew.west@observatoire.be
000003547 980__ $$aCPOSTER