23 citations as recorded by crossref.

1. Testing the impact of coronal mass ejections on cosmic-ray intensity modulation with algorithm selected Forbush decreases O. Okike et al. 10.1093/mnras/staa4002
2. What determines the observational magnitudes of Forbush events on Earth: A critique of the traditional manual method O. Okike 10.1093/mnras/stz3123
3. Precursory Signals of Forbush Decreases Not Connected with Shock Waves D. Lingri et al. 10.1007/s11207-022-01951-4
4. Empirical implications of location-dependent cosmic ray diurnal anisotropy on small-amplitude Forbush decreases O. Okike & F. Menteso 10.1140/epjp/s13360-024-05191-2
5. Effect of solar wind disturbances on small-amplitude simultaneous Forbush events during solar cycle 23 C. Ugwu et al. 10.1016/j.asr.2024.09.011
6. A Way of Detecting Local Muon-Flux Anisotropies with the Matrix-Form Data of the URAGAN Hodoscope M. Dobrovolsky et al. 10.3103/S1062873819050125
7. A New Method for Predicting Non‐Recurrent Geomagnetic Storms C. Wang et al. 10.1029/2023SW003522
8. On the variation of small-amplitude Forbush decreases with solar-geomagnetic parameters C. Ugwu et al. 10.1007/s10509-024-04310-w
9. The amplitude and phase distributions of cosmic ray variation at different conditions of Forbush decrease S. Shalaby et al. 10.1016/j.rinp.2022.106076
10. Cosmic ray − global lightning causality O. Okike & A. Umahi 10.1016/j.jastp.2019.04.002
11. The Frequency‐Domain Characterization of Cosmic Ray Intensity Variations Before Forbush Decreases Associated With Geomagnetic Storms Q. Ye et al. 10.1029/2021SW002863
12. Automated detection of simultaneous/non-simultaneous Forbush decreases and the associated cosmic ray phenomena O. Okike 10.1016/j.jastp.2020.105460
13. The implications of the superposed effect of cosmic ray diurnal anisotropy on weak Forbush Events at Apatity and Moscow Neutron Monitors F. Menteso et al. 10.1007/s10509-024-04358-8
14. A comparison of catalogues of Forbush decreases identified from individual and a network of neutron monitors: a critical perspective O. Okike et al. 10.1093/mnras/stab680
15. Analysis of Ground Level Enhancement Events of 1989 September 29; 2001 April 15 and 2005 January 20 R. Ugwoke et al. 10.1088/1674-4527/ac8b58
16. DOUBLE-EXPONENTIAL FITTING FUNCTION FOR EVALUATION OF COSMIC-RAY-INDUCED NEUTRON FLUENCE RATE IN ARBITRARY LOCATIONS H. Li et al. 10.1093/rpd/ncx047
17. First measurements of periodicities and anisotropies of cosmic ray flux observed with a water-Cherenkov detector at the Marambio Antarctic base N. Santos et al. 10.1016/j.asr.2022.11.041
18. Investigation of the rigidity and sensitivity dependence of neutron monitors for cosmic ray modulation using algorithm-selected Forbush decreases O. Okike & O. Nwuzor 10.1093/mnras/staa370
19. The Empirical Implication of Conducting a Chree Analysis Using Data from Isolated Neutron Monitors O. Okike & A. Umahi 10.1007/s11207-019-1405-y
20. Diurnal anisotropy of polar neutron monitors: Dome C looks poleward A. Gil et al. 10.1016/j.asr.2021.12.010
21. Amplitude of the Observational Forbush Decreases in the Presence of Cosmic Ray Diurnal Anisotropy During High Solar Activity in 1972 O. Okike & J. Alhassan 10.1007/s11207-021-01855-9
22. Chree Method of Analysis: A Critique of Its Application to Forbush Events Selection Criteria and Timing O. Okike 10.3847/1538-4357/ab32db
23. Amplitude of the Usual Cosmic Ray Diurnal and Enhanced Anisotropies: Implications for the Observed Magnitude, Timing, and Ranking of Forbush Decreases O. Okike 10.3847/1538-4357/abfe60