000004009 001__ 4009
000004009 005__ 20190130225626.0
000004009 037__ $$aCTALK-2019-0067
000004009 100__ $$aWest, Matthew
000004009 245__ $$aSH23C-3323: Epoch Analysis of Post Flare Loop Systems
000004009 260__ $$c2018
000004009 269__ $$c2018-12-11
000004009 520__ $$aThe length of post-flare/eruptive loop systems are intrinsically connected to the underlying magnetic field structure. In this work we present results of an epoch analysis used to compare the signatures of post flare-loops observed during the period when the STEREO satellites were in quadrature with the Sun-Earth line (SDO-AIA-HMI / PROBA2-SWAP). By choosing events that occurred near disc centre from the perspective of Earth, we can see the growth in profile from the perspective of STEREO EUVI, whilst obtaining magnetic field information from HMI. In this work we present correlations between the different phases of the loop growth, together with magnetic complexity, loop growth (height/speed) and flare magnitude.
000004009 536__ $$a3ESA-PROBA2SOC/$$c3ESA-PROBA2SOC/$$f3ESA-PROBA2SOC
000004009 594__ $$aNO
000004009 700__ $$aPalmerio, Erika
000004009 773__ $$tAGU Washington DC
000004009 8560_ $$fmatthew.west@observatoire.be
000004009 85642 $$ahttps://agu.confex.com/agu/fm18/meetingapp.cgi/Paper/440019
000004009 906__ $$aContributed
000004009 980__ $$aCTALKCONT