OOIR: Observatory of International Research

Papers

(The H4-Index of Solar Physics is 20. 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 2021-09-01 to 2025-09-01.)

Article	Citations
The Possible Cause of Most Intense Geomagnetic Superstorm of the 21st Century on 20 November 2003	80
Spatial and Temporal Variations of 2 – 10 MeV nuc−1 He/H in Gradual Solar Energetic Particle Events	57
Fabry–Pérot Interferometer-Based Tunable Narrow-Band Imager for Solar Chromospheric Observation: First Results	45
Numerical Simulation of Longitudinal Oscillation of Filament Based on Smoothed Particle Hydrodynamics (SPH) Method	40
Rate of Change of Large-Scale Solar-Wind Structure	36
Nonlinear Generation of Fluting Perturbations by Kink Mode in a Twisted Magnetic Tube	34
On the Possibility of Measuring Solar Flattening from Photometry Measurements Taken during Solar Eclipses Seen from the Earth’s Surface or Earth Orbit	32
Interplanetary Scintillation Observations of Solar-Wind Disturbances During Cycles 23 and 24	29
A Critical Comment on “Can Solar Cycle 25 Be a New Dalton Minimum?”	27
Accelerating Multiframe Blind Deconvolution via Deep Learning	27
Mysteries of the 17 May 2012 Solar Event Responsible for GLE71. I. CME Development and the Role of Disturbances Excited by Eruptions	27
Correction to: Kanzelhöhe Observatory: Instruments, Data Processing and Data Products	26
Bošković’s Spherical Trigonometric Solution for Determining the Axis and Rate of Solar Rotation by Observing Sunspots in 1777	24
Photometric Comparison of Metis and LASCO-C2 Polarized Brightness Images	23
Differential Rotation of Long-Lived Sunspot Groups in Solar Cycles 22 – 24 Determined by Watukosek Solar Observatory Data	23
CME-Flare Association and the Role of Reconnection in CME Acceleration	23
Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind	23
Solar Filament Segmentation Based on Improved U-Nets	22
Avalanching Together: A Model for Sympathetic Flaring	22
The Mean Temperatures of CME-Related Dimming Masses	21
Data-Driven Reconstruction of a Low-Order Dynamo Model from Sunspot Data	20