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Cited article:

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Effects of Global Geomagnetic Field Variations Over the Past 100,000 Years on Cosmogenic Radionuclide Production Rates in the Earth's Atmosphere

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High-Resolution Spectral and Anisotropy Characteristics of Solar Protons During the GLE N∘73 on 28 October 2021 Derived with Neutron-Monitor Data Analysis

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Fluences of solar energetic particles for last three GLE events: Comparison of different reconstruction methods

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Advances in Space Research 70 (9) 2585 (2022)
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Diurnal anisotropy of polar neutron monitors: Dome C looks poleward

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Advances in Space Research 70 (9) 2618 (2022)
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The probabilistic solar particle event forecasting (PROSPER) model

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Characteristic Features of Solar Cosmic Rays in the 21st–24th Solar-Activity Cycles According to Data from Catalogs of Solar Proton Events

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Geomagnetism and Aeronomy 61 (1) 6 (2021)
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High‐Altitude Polar NM With the New DAQ System as a Tool to Study Details of the Cosmic‐Ray Induced Nucleonic Cascade

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Application of the Verified Neutron Monitor Yield Function for an Extended Analysis of the GLE # 71 on 17 May 2012

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World grid of cosmic ray vertical cut-off rigidity for the last decade

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GLE # 67 Event on 2 November 2003: An Analysis of the Spectral and Anisotropy Characteristics Using Verified Yield Function and Detrended Neutron Monitor Data

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Current status and possible extension of the global neutron monitor network

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Minor Ground Level Enhancements in the Solar Cosmic Rays in the 24th Solar Activity Cycle

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Solar energetic particles in the inner heliosphere: status and open questions

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Journal of Space Weather and Space Climate 9 E1 (2019)
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Onset Time of the GLE 72 Observed at Neutron Monitors and its Relation to Electromagnetic Emissions

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First Analysis of Ground-Level Enhancement (GLE) 72 on 10 September 2017: Spectral and Anisotropy Characteristics

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An Anisotropic Cosmic-Ray Enhancement Event on 07-June-2015: A Possible Origin

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The Ground‐Level Enhancement Event of September 2017 and Other Large Solar Energetic Particle Events of Cycle 24

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GLE and Sub-GLE Redefinition in the Light of High-Altitude Polar Neutron Monitors

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