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Solar Physics|September 14, 2022
Interferometric Imaging, and Beam-Formed Study of a Moving Type-IV Radio Burst with LOFARHongyu Liu, Pietro Zucca, Kyung-Suk Cho, et al.Solar Physics|April 20, 2018
A Fixed-point Scheme for the Numerical Construction of Magnetohydrostatic Atmospheres in Three DimensionsS A Gilchrist, D C Braun, G BarnesSolar Physics|November 1, 2021
Can Multi-threaded Flux Tubes in Coronal Arcades Support a Magnetohydrodynamic Avalanche?J Threlfall, J Reid, A W HoodSolar Physics|July 20, 2022
Searching for a Solar Source of Magnetic-Field Switchbacks in Parker Solar Probe's First EncounterD de Pablos, T Samanta, S T Badman, et al.Solar Physics|July 27, 2022
First Hard X-Ray Imaging Results by Solar Orbiter STIXPaolo Massa, Andrea F Battaglia, Anna Volpara, et al.Solar Physics|July 2, 2019
On the Performance of Multi-Instrument Solar Flare Observations During Solar Cycle 24Ryan O Milligan, Jack IrelandSolar Physics|March 7, 2022
Sky Brightness Evaluation at Concordia Station, Dome C, Antarctica, for Ground-Based Observations of the Solar CoronaAlessandro Liberatore, Gerardo Capobianco, Silvano Fineschi, et al.Solar Physics|February 15, 2020
Probabilistic Solar Wind and Geomagnetic Forecasting Using an Analogue Ensemble or "Similar Day" ApproachM J Owens, P Riley, T S HorburySolar Physics|April 1, 2020
Particle Acceleration Due to Coronal Non-null Magnetic ReconnectionJames Threlfall, Thomas Neukirch, Clare Elizabeth ParnellSolar Physics|October 31, 2022
A Statistical Comparison of EUV Brightenings Observed by SO/EUI with Simulated Brightenings in Nonpotential SimulationsKrzysztof Barczynski, Karen A Meyer, Louise K Harra, et al.Pageof 12