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Coupling between magnetic reconnection, energy release, and particle acceleration in the X17.2 2003 October 28 solar flare
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Magnetic Reconnection Flux during Two Flares on September 6, 2017
Characterising solar magnetic reconnection in confined and eruptive flares
Kanniah Balamuralikrishna, John Y. H. Soo, Norhaslinda Mohamed Tahrin and Abdul Halim Abdul Aziz Astrophysics and Space Science 368(11) (2023) https://doi.org/10.1007/s10509-023-04251-w
High-Energy Emissions Observed in the Impulsive Phase of the 2001 August 25 Eruptive Flare
Correlated Spatio-temporal Evolution of Extreme-Ultraviolet Ribbons and Hard X-Rays in a Solar Flare
S. J. Naus, J. Qiu, C. R. DeVore, S. K. Antiochos, J. T. Dahlin, J. F. Drake and M. Swisdak The Astrophysical Journal 926(2) 218 (2022) https://doi.org/10.3847/1538-4357/ac4028
Invited Review: Short-term Variability with the Observations from the Helioseismic and Magnetic Imager (HMI) Onboard the Solar Dynamics Observatory (SDO): Insights into Flare Magnetism
Study of reconnection rates and light curves in solar flares from low and mid chromosphere
G Sindhuja, Nandita Srivastava, A M Veronig and W Pötzi Monthly Notices of the Royal Astronomical Society 482(3) 3744 (2019) https://doi.org/10.1093/mnras/sty2887
The Scientific Foundation of Space Weather
Lucie M. Green, Tibor Török, Bojan Vršnak, Ward Manchester and Astrid Veronig Space Sciences Series of ISSI, The Scientific Foundation of Space Weather 67 113 (2019) https://doi.org/10.1007/978-94-024-1588-9_5
On the Relation between Flare and CME during GLE-SEP and Non-GLE-SEP Events
Reconnection Fluxes in Eruptive and Confined Flares and Implications for Superflares on the Sun
Johannes Tschernitz, Astrid M. Veronig, Julia K. Thalmann, Jürgen Hinterreiter and Werner Pötzi The Astrophysical Journal 853(1) 41 (2018) https://doi.org/10.3847/1538-4357/aaa199
Multi-instrument view on solar eruptive events observed with the Siberian Radioheliograph: From detection of small jets up to development of a shock wave and CME
Dependence of Coronal Mass Ejection Properties on Their Solar Source Active Region Characteristics and Associated Flare Reconnection Flux
Sanchita Pal, Dibyendu Nandy, Nandita Srivastava, Nat Gopalswamy and Suman Panda The Astrophysical Journal 865(1) 4 (2018) https://doi.org/10.3847/1538-4357/aada10
The Acceleration Process of a Solar Quiescent Filament in the Inner Corona
H. Q. Song, Y. Chen, J. Qiu, C. X. Chen, J. Zhang, X. Cheng, Y. D. Shen and R. S. Zheng The Astrophysical Journal Letters 857(2) L21 (2018) https://doi.org/10.3847/2041-8213/aabcc3
The 26 December 2001 Solar Eruptive Event Responsible for GLE63. II. Multi-Loop Structure of Microwave Sources in a Major Long-Duration Flare
S. N. Kuznetsov, V. G. Kurt, B. Yu. Yushkov, et al. Astrophysics and Space Science Library, The Coronas-F Space Mission 400 301 (2014) https://doi.org/10.1007/978-3-642-39268-9_10
A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. II. CMEs, Shock Waves, and Drifting Radio Bursts
A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. I. Unusual History of an Eruptive Filament
Relations between Strong High-Frequency Microwave Bursts and Proton Events
Victor V. Grechnev, Nataliya S. Meshalkina, Ilya M. Chertok and Valentin I. Kiselev Publications of the Astronomical Society of Japan 65(sp1) S4 (2013) https://doi.org/10.1093/pasj/65.sp1.S4
Initiation of Coronal Mass Ejections by Sunspot Rotation
Magnetic Flux of EUV Arcade and Dimming Regions as a Relevant Parameter for Early Diagnostics of Solar Eruptions – Sources of Non-recurrent Geomagnetic Storms and Forbush Decreases
Gamma-Ray and High-Energy-Neutron Measurements on CORONAS-F during the Solar Flare of 28 October 2003
Sergei N. Kuznetsov, Victoria G. Kurt, Boris Y. Yushkov, Karel Kudela and Vladimir I. Galkin Solar Physics 268(1) 175 (2011) https://doi.org/10.1007/s11207-010-9669-2
OBSERVATIONS OF CHROMOSPHERIC FLARE RE-BRIGHTENINGS
Dynamics and energetics of the thermal and nonthermal components in the solar flare of January 20, 2005, based on data from hard electromagnetic radiation detectors onboard the CORONAS-F satellite