Results 121 to 130 of about 1,149,927 (208)

Back reaction of the untwisting solar corona scars sunspots. [PDF]

Sci Adv
Xing C, Cheng X, Aulanier G, Ding M.
europepmc   +1 more source

Potential Solar Precursors to Magnetic Switchbacks. [PDF]

Space Sci Rev
Tripathi D, Madjarska MS, Karpen J, Velli M, Froment C, Pariat E, Patsourakos S, Raouafi NE, Rouillard AP, Sterling AC, Tziotziou K, Wyper PF.   +11 more
europepmc   +1 more source

Investigating the Relationship Between Physical Properties and Spatial Irregularities at Coronal Hole Boundaries. [PDF]

Sol Phys
Ngampoopun N, Long DM, Green LM, Yardley SL, James AW, Mason EI, Heinemann SG, Uritsky VM.   +7 more
europepmc   +1 more source

Evolution of Open Magnetic Flux and Heliospheric Current Sheet-Associated Streamer Wind Across Multiple Solar Cycles. [PDF]

Sol Phys
MacTaggart JR, Zhao L, Lepri ST, Fisk LA, Nakhleh AJ.   +4 more
europepmc   +1 more source

The EUV Late-Phase: Statistical Results from 15 Years of Solar Dynamics Observatory Observations. [PDF]

Sol Phys
Greatorex HJ, O'Hare AN, Bekker S, Campbell RJ, Keane DC, Milligan RO.   +5 more
europepmc   +1 more source

Propagating slow-mode shocks discovered in dynamical solar flare loops. [PDF]

Nat Commun
Ye J, Shen C, Raymond JC, Cai Q, Mei Z, Hu J, Chen Y, Li Y, Lin J.   +8 more
europepmc   +1 more source

Revealing Flare Energetics and Dynamics with SDO EVE Solar Extreme Ultraviolet Spectral Irradiance Observations. [PDF]

Sol Phys
Woods TN, Chamberlin PC, Jones A, Mason JP, Qian L, Warren HP, Woodraska D, Borelli R, Eparvier FG, Gonzalez G.   +9 more
europepmc   +1 more source

High-frequency magnetohydrodynamic waves with substantial energy in the solar polar corona. [PDF]

Natl Sci Rev
Gao Y, Tian H, Morton R, Van Doorsselaere T, Lim D, Guo M, He J, Hou Z.   +7 more
europepmc   +1 more source

MUSE EUV spectroscopy of a kink-unstable coronal loops system

Turbulent photospheric motions drive the solar magnetic field to twist and tangle, making magnetic stresses continuously grow in the corona. Thin magnetic flux tubes can become kink-unstable and magnetic energy can be released through impulsive and ...
Antonino Petralia, Alan W. Hood, Gabriele Cozzo, Costanza Argiroffi, Fabio Reale, Juan Martinez-Sykora, Bart de Pontieu, Paolo Pagano, Jack Reid, Paola Testa   +9 more
core  

The Behaviour of the EUV Corona Before Flares in Regions with High Free Magnetic Energy. [PDF]

Sol Phys
Harra L, Kusano K, Zhu Y, Barczynski K, De-Sassi A, Stiefel MZ, Kontogiannis I, West MJ, Brooks DH.   +8 more
europepmc   +1 more source