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Cited by in F6Publishing
For: Kahler SW, Ling AG. Forecasting Solar Energetic Particle (SEP) events with Flare X-ray peak ratios. J Space Weather Space Clim 2018;8:A47. [DOI: 10.1051/swsc/2018033] [Cited by in Crossref: 9] [Cited by in F6Publishing: 9] [Article Influence: 2.3] [Reference Citation Analysis]
Number Citing Articles
1 Kahler SW, Ling AG. A Comparison of Solar X-Ray Flare Timescales and Peak Temperatures with Associated Coronal Mass Ejections. ApJ 2022;934:175. [DOI: 10.3847/1538-4357/ac7e56] [Reference Citation Analysis]
2 Miteva R, Samwel SW. M-Class Solar Flares in Solar Cycles 23 and 24: Properties and Space Weather Relevance. Universe 2022;8:39. [DOI: 10.3390/universe8010039] [Cited by in Crossref: 3] [Cited by in F6Publishing: 2] [Article Influence: 3.0] [Reference Citation Analysis]
3 Papaioannou A, Vainio R, Raukunen O, Jiggens P, Aran A, Dierckxsens M, Mallios SA, Paassilta M, Anastasiadis A. The probabilistic solar particle event forecasting (PROSPER) model. J Space Weather Space Clim 2022;12:24. [DOI: 10.1051/swsc/2022019] [Cited by in Crossref: 2] [Cited by in F6Publishing: 2] [Article Influence: 2.0] [Reference Citation Analysis]
4 Aminalragia-giamini S, Raptis S, Anastasiadis A, Tsigkanos A, Sandberg I, Papaioannou A, Papadimitriou C, Jiggens P, Aran A, Daglis IA. Solar Energetic Particle Event occurrence prediction using Solar Flare Soft X-ray measurements and Machine Learning. J Space Weather Space Clim 2021;11:59. [DOI: 10.1051/swsc/2021043] [Cited by in Crossref: 1] [Cited by in F6Publishing: 1] [Article Influence: 1.0] [Reference Citation Analysis]
5 Lavasa E, Giannopoulos G, Papaioannou A, Anastasiadis A, Daglis IA, Aran A, Pacheco D, Sanahuja B. Assessing the Predictability of Solar Energetic Particles with the Use of Machine Learning Techniques. Sol Phys 2021;296. [DOI: 10.1007/s11207-021-01837-x] [Cited by in Crossref: 2] [Cited by in F6Publishing: 6] [Article Influence: 2.0] [Reference Citation Analysis]
6 Steyn R, Strauss DT, Effenberger F, Pacheco D. The soft X-ray Neupert effect as a proxy for solar energetic particle injection: A proof-of-concept physics-based forecasting model. J Space Weather Space Clim 2020;10:64. [DOI: 10.1051/swsc/2020067] [Cited by in Crossref: 3] [Cited by in F6Publishing: 4] [Article Influence: 1.5] [Reference Citation Analysis]
7 Kahler SW, Ling AG. The Role of Peak Temperatures in Solar X-Ray Flare Associations with CME Speeds and Widths and in Flare Size Distributions. ApJ 2020;901:63. [DOI: 10.3847/1538-4357/abae5e] [Cited by in Crossref: 1] [Cited by in F6Publishing: 1] [Article Influence: 0.5] [Reference Citation Analysis]
8 Chakraborty S, Morley SK. Probabilistic prediction of geomagnetic storms and the K p index. J Space Weather Space Clim 2020;10:36. [DOI: 10.1051/swsc/2020037] [Cited by in Crossref: 8] [Cited by in F6Publishing: 6] [Article Influence: 4.0] [Reference Citation Analysis]
9 Ling AG, Kahler SW. Peak Temperatures of Large Solar X-Ray Flares and Associated CME Speeds and Widths. ApJ 2020;891:54. [DOI: 10.3847/1538-4357/ab6f6c] [Cited by in Crossref: 1] [Cited by in F6Publishing: 3] [Article Influence: 0.5] [Reference Citation Analysis]