23 citations as recorded by crossref.

1. The Energetic Particle Detector J. Rodríguez-Pacheco et al. 10.1051/0004-6361/201935287
2. Modeling proton intensity gradients and radiation dose equivalents in the inner heliosphere using EMMREM: May 2003 solar events M. Dayeh et al. 10.1029/2009SW000566
3. LONGITUDINAL AND RADIAL DEPENDENCE OF SOLAR ENERGETIC PARTICLE PEAK INTENSITIES:STEREO,ACE,SOHO,GOES, ANDMESSENGEROBSERVATIONS D. Lario et al. 10.1088/0004-637X/767/1/41
4. Modeling and forecasting solar energetic particle events at Mars: the event on 6 March 1989 A. Aran et al. 10.1051/0004-6361:20077233
5. Variation of Proton Flux Profiles with the Observer’s Latitude in Simulated Gradual SEP Events R. Rodríguez-Gasén et al. 10.1007/s11207-013-0442-1
6. A theoretical perspective on particle acceleration by interplanetary shocks and the Solar Energetic Particle problem O. Verkhoglyadova et al. 10.1016/j.physrep.2014.10.004
7. Space Radiation and Plasma Effects on Satellites and Aviation: Quantities and Metrics for Tracking Performance of Space Weather Environment Models Y. Zheng et al. 10.1029/2018SW002042
8. Propagation of Solar Energetic Particles in Three-dimensional Interplanetary Magnetic Fields: Radial Dependence of Peak Intensities H. He et al. 10.3847/1538-4357/aa7574
9. Capability of Geomagnetic Storm Parameters to Identify Severe Space Weather N. Balan et al. 10.3847/1538-4357/ab5113
10. RADIAL DEPENDENCE OF PEAK PROTON AND IRON ION FLUXES IN SOLAR ENERGETIC PARTICLE EVENTS: APPLICATION OF THE PATH CODE O. Verkhoglyadova et al. 10.1088/0004-637X/757/1/75
11. Comparing proton fluxes of central meridian SEP events with those predicted by SOLPENCO A. Aran et al. 10.1016/j.asr.2007.08.003
12. Assessing the Predictability of Solar Energetic Particles with the Use of Machine Learning Techniques E. Lavasa et al. 10.1007/s11207-021-01837-x
13. Radial dependence of proton peak intensities and fluences in SEP events: Influence of the energetic particle transport parameters D. Lario et al. 10.1016/j.asr.2007.01.057
14. Validating the proton prediction system (PPS) S. Kahler et al. 10.1016/j.jastp.2006.06.009
15. What causes the variability in the properties of energetic storm particle (ESP) events? M. Dayeh et al. 10.1088/1742-6596/1100/1/012008
16. Solar energetic particles in the inner heliosphere: status and open questions A. Anastasiadis et al. 10.1098/rsta.2018.0100
17. Radial and Longitudinal Dependence of Solar 4–13 MeV and 27–37 MeV Proton Peak Intensities and Fluences:HeliosandIMP 8Observations D. Lario et al. 10.1086/508982
18. Review of Solar Energetic Particle Prediction Models K. Whitman et al. 10.1016/j.asr.2022.08.006
19. Why should the latitude of the observer be considered when modeling gradual proton events? An insight using the concept of cobpoint R. Rodríguez-Gasén et al. 10.1016/j.asr.2010.03.021
20. Advancing interplanetary magnetohydrodynamic models through solar energetic particle modelling A. Niemela et al. 10.1051/0004-6361/202347116
21. Dynamics of the Earth’s Particle Radiation Environment R. Vainio et al. 10.1007/s11214-009-9496-7
22. Forecasting the Earth’s radiation belts and modelling solar energetic particle events: Recent results from SPACECAST R. Horne et al. 10.1051/swsc/2013042
23. A semi-analytical foreshock model for energetic storm particle events inside 1 AU R. Vainio et al. 10.1051/swsc/2014005