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Extreme-ultraviolet Fine Structure and Variability Associated with Coronal Rain Revealed by Solar Orbiter/EUI HRIEUV and SPICE

P. Antolin,A. Dolliou,F. Auchere,L. P. Chitta,S. Parenti,D. Berghmans,R. Aznar Cuadrado,K. Barczynski,S. Gissot,L. Harra, Z. Huang,M. Janvier,E. Kraaikamp,D. M. Long,S. Mandal,H. Peter,L. Rodriguez,U. Schuehle,P. J. Smith,S. K. Solanki,K. Stegen,L. Teriaca,C. Verbeeck,M. J. West,A. N. Zhukov,T. Appourchaux,G. Aulanier,E. Buchlin,F. Delmotte, J. M. Gilles,M. Haberreiter,J. -P. Halain,K. Heerlein,J. -F. Hochedez,M. Gyo,S. Poedts,P. Rochus

ASTRONOMY & ASTROPHYSICS（2023）

Cited 1|Views17
Key words
Sun,corona,transition region,activity,filaments,prominences,magnetohydrodynamics (MHD),instabilities
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