000004015 001__ 4015
000004015 005__ 20190131001415.0
000004015 037__ $$aPOSTER-2019-0049
000004015 100__ $$aWest, Matthew
000004015 245__ $$aPost-Flare Loop Signatures
000004015 260__ $$c2018
000004015 269__ $$c2018-08-01
000004015 520__ $$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.
000004015 536__ $$a3ESA-PROBA2SOC/$$c3ESA-PROBA2SOC/$$f3ESA-PROBA2SOC
000004015 594__ $$aNO
000004015 700__ $$aSeaton, Daniel
000004015 700__ $$aPalmerio, Erika
000004015 773__ $$tSHINE meeting, Florida, USA
000004015 8560_ $$fmatthew.west@observatoire.be
000004015 85642 $$ahttp://shinecon.org/shine2018/ViewAbstract.php?idabs=37
000004015 980__ $$aCPOSTER