000006973 001__ 6973
000006973 005__ 20240416120710.0
000006973 037__ $$aPOSTER-2024-0066
000006973 100__ $$aBerghmans, D.
000006973 245__ $$aEUI High Resolution Observations of Decayless Oscillations
000006973 260__ $$c2024
000006973 269__ $$c2024-04-08
000006973 520__ $$aDecayless oscillations are routinely observed with AIA and now also with HRIEUV. Co-observations EUI & AIA detect the same decayless oscillations, confirming that they are of solar origin. Decayless oscillations are different from flare-induced oscillations as they do not dampen during their lifetime and they are independent of flares. In fact the driver is unknown. These oscillations have been interpreted as kink-waves and the ratio between the loop length and the period tends to be in the order of 1 Mm/s, suggestive of the coronal Alfvén speed.
000006973 594__ $$aSTCE
000006973 6531_ $$aSolar Orbiter
000006973 6531_ $$aEUI
000006973 6531_ $$awaves
000006973 700__ $$aLim, D.
000006973 700__ $$aPetrova, E.
000006973 700__ $$aZhong, S.
000006973 700__ $$aShrivastav, A.K.
000006973 700__ $$aMandal, S.
000006973 700__ $$aKraaikamp, E.
000006973 700__ $$aVerbeeck, C.
000006973 700__ $$aStegen, K.
000006973 700__ $$aZhukov, A.
000006973 700__ $$aGissot, S.
000006973 700__ $$aVan Doorsselaere, T.
000006973 773__ $$tJoint Solar Orbiter, Parker Solar Probe, and DKIST Meeting, San Antonio, Texas
000006973 8560_ $$fdavid.berghmans@ksb-orb.be
000006973 85642 $$ahttps://eclipse2024sa.com
000006973 8564_ $$s2808615$$uhttp://publi2-as.oma.be/record/6973/files/posterFinal.pdf
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000006973 980__ $$aCPOSTER