Solar Physics

Papers
(The H4-Index of Solar Physics is 17. The table below lists those papers that are above that threshold based on CrossRef citation counts [max. 250 papers]. The publications cover those that have been published in the past four years, i.e., from 2022-08-01 to 2026-08-01.)
ArticleCitations
Nonlinear Generation of Fluting Perturbations by Kink Mode in a Twisted Magnetic Tube101
The Solar Aspect System of the Hard X-ray Imager Onboard ASO-S78
Avalanching Together: A Model for Sympathetic Flaring50
Observations of Switchback Chains in a Twin-CME Event31
The Solar Origin of an Intense Geomagnetic Storm on 1 December 2023: Successive Slipping and Eruption of Multiple Magnetic Flux Ropes31
Accelerating Multiframe Blind Deconvolution via Deep Learning30
Bošković’s Spherical Trigonometric Solution for Determining the Axis and Rate of Solar Rotation by Observing Sunspots in 177729
Interplanetary Scintillation Observations of Solar-Wind Disturbances During Cycles 23 and 2429
Photometric Comparison of Metis and LASCO-C2 Polarized Brightness Images24
The Mean Temperatures of CME-Related Dimming Masses24
On the Possibility of Measuring Solar Flattening from Photometry Measurements Taken during Solar Eclipses Seen from the Earth’s Surface or Earth Orbit24
Shock Signatures of the Successive Type-II Solar Radio Bursts at Meter Wavelength23
Data-Driven Reconstruction of a Low-Order Dynamo Model from Sunspot Data23
CME-Flare Association and the Role of Reconnection in CME Acceleration22
Differential Rotation of Long-Lived Sunspot Groups in Solar Cycles 22 – 24 Determined by Watukosek Solar Observatory Data22
The Possible Cause of Most Intense Geomagnetic Superstorm of the 21st Century on 20 November 200321
A Critical Comment on “Can Solar Cycle 25 Be a New Dalton Minimum?”18
On the Relation Between Upflow Velocities and Coronal Non-thermal Velocities as Measured by Hinode/EIS17
Analog-Based Forecasting of Solar Cycles Using Dynamic Time Warping and Residual Bootstrapping: Real-Time Application to Cycle 2517
Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind17
Mysteries of the 17 May 2012 Solar Event Responsible for GLE71. I. CME Development and the Role of Disturbances Excited by Eruptions17
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