000006996 001__ 6996
000006996 005__ 20240715085634.0
000006996 037__ $$aCTALK-2024-0121
000006996 100__ $$aMandal, S.
000006996 245__ $$aStereoscopic analysis of coronal loop morphology and dynamics
000006996 260__ $$c2024
000006996 269__ $$c2024-06-25
000006996 520__ $$aCoronal loops are some of the most easily recognizable features within the solar corona. Despite years of research, some aspects of these arched structures are still not well understood, such as the loop's cross-section and its variation along its length. In a recent study, we conducted a stereoscopic analysis of the morphology and dynamics of a coronal loop using high resolution images from two different spacecraft - the High Resolution Imager (HRI) of the Extreme Ultraviolet Imager on board the Solar Orbiter, and the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory. Our findings suggest that the observed loop exhibits similar widths in both datasets, indicating that the cross-sectional shape of the loop is circular. Additionally, the loop maintained a uniform width along its entire length, which supports the idea that coronal loops do not show expansions. Moreover, this loop's highly unusual dynamics make this a fascinating case study. I will discuss the implications of these results on our understanding of loop formations, particularly from the perspective of the 'coronal veil' hypothesis.
000006996 594__ $$aSTCE
000006996 6531_ $$acorona
000006996 6531_ $$aEUV
000006996 6531_ $$aSolar Orbiter
000006996 700__ $$aPeter, H.
000006996 700__ $$aKlimchuk, J. A.
000006996 700__ $$aSolanki, S. K.
000006996 700__ $$aChitta, L. P.
000006996 700__ $$aCuadrado, R. A.
000006996 700__ $$aSchuhle, U.
000006996 700__ $$aTerrace, L.
000006996 700__ $$aBerghmans, D.
000006996 773__ $$t11th Coronal Loop Workshop
000006996 8560_ $$fdavid.berghmans@ksb-orb.be
000006996 85642 $$ahttps://meetings.iac.es/clw11/
000006996 85642 $$ahttps://cloud.iac.es/index.php/s/85rPTtiz558od7a
000006996 906__ $$aContributed
000006996 980__ $$aCTALKCONT