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Kim, M.-H.Y., De Angelis, G., Cucinotta, F.A., 2011. Probabilistic assessment of radiation risk for astronauts in space missions. Acta Astronaut. 68 (7), 747–759.

Klein, K.-L., Dalla, S., 2017. Acceleration and Propagation of Solar Energetic Particles. Space Sci. Rev. 212 (3–4), 1107–1136.

Kong, X., Guo, F., Giacalone, J., Li, H., Chen, Y., 2017. The Acceleration of High-energy Protons at Coronal Shocks: The Effect of Large-scale Streamer-like Magnetic Field Structures. Astrophys. J. 851 (1), 38.

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Kozarev, K.A., Davey, A., Kendrick, A., Hammer, M., Keith, C., 2017. The Coronal Analysis of SHocks and Waves (CASHeW) framework. J. Space Weather Space Clim. 7, A32.

Kozarev, K.A., Dayeh, M.A., Farahat, A., 2019. Early-stage Solar Energetic Particle Acceleration by Coronal Mass Ejection-driven Shocks with Realistic Seed Spectra. I. Low Corona. Astrophys. J. 871 (1), 65.

Kozarev, K.A., Evans, R.M., Schwadron, N.A., Dayeh, M.A., Opher, M., Korreck, K.E., van der Holst, B., 2013. Global Numerical Modeling of Energetic Proton Acceleration in a Coronal Mass Ejection Traveling through the Solar Corona. Astrophys. J. 778 (1), 43.

Kozarev, K.A., Schwadron, N.A., 2016. A Data-driven Analytic Model for Proton Acceleration by Large-scale Solar Coronal Shocks. Astrophys. J. 831 (2), 120.

Kruglanski, M., Crosby, N., Devos, A., Perry, C., Borries, C., Martini, D., Luntama, J.-P., 07 2016. Services for space mission support within the esa space situational awareness space weather service network.

Krymsky, G.F., 1977. A regular mechanism for the acceleration of charged particles on the front of a shock wave. Soviet Physics-Doklady 234, 1306.

Kühl, P., Heber, B., Gómez-Herrero, R., Malandraki, O., Posner, A., Sierks, H., 2020. The Electron Proton Helium INstrument as an example for a Space Weather Radiation Instrument. J. Space Weather Space Clim. 10, 53.

Lario, D., 2005. Advances in modeling gradual solar energetic particle events. Adv. Space Res. 36 (12), 2279–2288.

Lario, D., Kwon, R.Y., Balmaceda, L., Richardson, I.G., Krupar, V., Thompson, B.J., Cyr, O.C.S., Zhao, L., Zhang, M., 2020. Fast and Wide CMEs without Observed >20 MeV Protons. Astrophys. J. 889 (2), 92.

Lario, D., Sanahuja, B., Heras, A.M., 1998. Energetic Particle Events: Efficiency of Interplanetary Shocks as $50 \text{ keV} < E < 100 \text{ MeV Proton Accelerators.}$ Astrophys. J. 509 (1), 415–434.

Laurenza, M., Alberti, T., Cliver, E.W., 2018. A Short-term ESPERTA-based Forecast Tool for Moderate-to-extreme Solar Proton Events. Astrophys. J. 857 (2), 107.

Laurenza, M., Cliver, E.W., Hewitt, J., Storini, M., Ling, A.G., Balch, C. C., Kaiser, M.L., 2009. A technique for short-term warning of solar energetic particle events based on flare location, flare size, and evidence of particle escape. Space Weather 7 (4), S04008.

Lavasa, E., Giannopoulos, G., Papaioannou, A., Anastasiadis, A., Daglis, I.A., Aran, A., Pacheco, D., Sanahuja, B., 2021. Assessing the Predictability of Solar Energetic Particles with the Use of Machine Learning Techniques. Sol. Phys. 296 (7), 107.

le Roux, J.A., Webb, G.M., 2009. Time-Dependent Acceleration of Interstellar Pickup Ions at the Heliospheric Termination Shock Using a Focused Transport Approach. Astrophys. J. 693 (1), 534–551.

Leblanc, Y., Dulk, G.A., Bougeret, J.-L., 1998. Tracing the Electron Density from the Corona to 1au. Sol. Phys. 183 (1), 165–180.

LeCun, Y., Bengio, Y., 1998. Convolutional networks for images, speech, and time series. In: Arbib, M.A. (Ed.), The Handbook of Brain Theory and Neural Networks. MIT Press, Cambridge, MA, USA, pp. 255–258.

Lee, M.A., Fisk, L.A., 1981. The role of particle drifts in solar modulation. Astrophys. J. 248, 836–844.

Li, G., Jin, M., Ding, Z., Bruno, A., de Nolfo, G.A., Randol, B.M., Mays, L., Ryan, J., Lario, D., 2021. Modeling the 2012 May 17 Solar Energetic Particle Event Using the AWSOM and iPATH Models. Astrophys. J. 919 (2), 146.

Liemohn, M.W., Shane, A.D., Azari, A.R., Petersen, A.K., Swiger, B.M., Mukhopadhyay, A., 2021. RMSE is not enough: Guidelines to robust data-model comparisons for magnetospheric physics. J. Atmos. Solar-Terr. Phys. 218, 105624.

Linker, J.A., Caplan, R.M., Downs, C., Riley, P., Mikic, Z., Lionello, R., Henney, C.J., Arge, C.N., Liu, Y., Derosa, M.L., Yeates, A., Owens, M.J., 2017. The Open Flux Problem. Astrophys. J. 848 (1), 70.

Linker, J.A., Caplan, R.M., Schwadron, N., Gorby, M., Downs, C., Torok, T., Lionello, R., Wijaya, J., 2019. Coupled MHD-Focused Transport Simulations for Modeling Solar Particle Events. J. Phys. Conf. Ser. 1225, 012007.

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Núñez, M., 2022. Evaluation of the UMASEP-10 Version 2 Tool for Predicting All >10 MeV SEP Events of Solar Cycles 22, 23 and 24. Universe 8 (1), 35.

Núñez, M., Paul-Pena, D., 2020. Predicting >10 MeV SEP Events from Solar Flare and Radio Burst Data. Universe 6 (10), 161.

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Malandraki, O.E., Crosby, N.B. (Eds.), Jan. 2018. Solar Particle Radiation Storms Forecasting and Analysis: The HESPERIA HORIZON 2020 Project and Beyond. Vol. 444 of Astrophysics and Space Science Library.

Manchester, W.B., I., Gombosi, T.I., De Zeeuw, D.L., Sokolov, I.V., Roussev, I.I., Powell, K.G., Kóta, J., Tóth, G., Zurbuchen, T.H., Apr. 2005. Coronal Mass Ejection Shock and Sheath Structures Relevant to Particle Acceleration. Astrophys. J. 622 (2), 1225–1239.

Manchester, W.B., I., van der Holst, B., Lavraud, B., Jun. 2014. Flux rope evolution in interplanetary coronal mass ejections: the 13 May 2005 event. Plasma Phys. Control. Fusion 56 (6), 064006.

Manchester, W.B., I., van der Holst, B., Tóth, G., Gombosi, T.I., 2012. The Coupled Evolution of Electrons and Ions in Coronal Mass Ejection-driven shocks. Astrophys. J. 756 (1), 81.

Manchester, Ward, I., Van Der Holst, B., 2017. The Interaction of Coronal Mass Ejections with Alfvénic Turbulence. J. Phys. Conf. Ser. 900, 012015.

Manchester, Ward B., I., Vourlidas, A., Tóth, G., Lugaz, N., Roussev, I. I., Sokolov, I.V., Gombosi, T.I., De Zeeuw, D.L., Opher, M., 2008. Three-dimensional MHD Simulation of the 2003 October 28 Coronal Mass Ejection: Comparison with LASCO Coronagraph Observations. Astrophys. J. 684 (2), 1448–1460.

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Marsh, M.S., Dalla, S., Kelly, J., Laitinen, T., 2013. Drift-induced Perpendicular Transport of Solar Energetic Particles. Astrophys. J. 774 (1), 4.

Martens, P.C., Angryk, R.A., Aug. 2018. Data Handling and Assimilation for Solar Event Prediction. In: Foullon, C., Malandraki, O.E. (Eds.), Space Weather of the Heliosphere: Processes and Forecasts. Vol. 335. pp. 344–347.

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Mays, M.L., Taktakishvili, A., Pulkkinen, A., MacNeice, P.J., Rastätter, L., Odstrcil, D., Jian, L.K., Richardson, I.G., LaSota, J.A., Zheng, Y., Kuznetsova, M.M., 2015. Ensemble Modeling of CMEs Using the WSA-ENLIL+Cone Model. Sol. Phys. 290 (6), 1775–1814.

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Mikić, Z., Linker, J.A., Schnack, D.D., Lionello, R., Tarditi, A., 1999. Magnetohydrodynamic modeling of the global solar corona. Phys. Plasmas 6 (5), 2217–2224.

Millward, G., Biesecker, D., Pizzo, V., de Koning, C.A., 2013. An operational software tool for the analysis of coronagraph images: Determining CME parameters for input into the WSA-Enlil heliospheric model. Space Weather 11 (2), 57–68.

Miteva, R., Samwel, S.W., Krupar, V., 2017. Solar energetic particles and radio burst emission. J. Space Weather Space Clim. 7, A37.

Müller-Mellin, R., Kunow, H., Fleißner, V., Pehlke, E., Rode, E., Röschmann, N., Scharnberg, C., Sierks, H., Rusznyak, P., McKenna-Lawlor, S., Elendt, I., Sequeiros, J., Meziat, D., Sanchez, S., Medina, J., Del Peral, L., Witte, M., Marsden, R., Henrion, J., 1995. COSTEP - Comprehensive Suprathermal and Energetic Particle Analyser. Sol. Phys. 162 (1–2), 483–504.

National Science & Technology Council, 2019. National Space Weather Strategy and Action Plan. URL: https://trumpwhitehouse.archives.gov/wp-content/uploads/2019/03/National-Space-Weather-Strategy-and-Action-Plan-2019.pdf.

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Núñez, M., 2015. Real-time prediction of the occurrence and intensity of the first hours of >100 MeV solar energetic proton events. Space Weather 13 (11), 807–819.

Núñez, M., 2022. Evaluation of the UMASEP-10 Version 2 Tool for Predicting All >10 MeV SEP Events of Solar Cycles 22, 23 and 24. Universe 8 (1), 35.

Núñez, M., Paul-Pena, D., 2020. Predicting >10 MeV SEP Events from Solar Flare and Radio Burst Data. Universe 6 (10), 161.

Núñez, M., Reyes-Santiago, P.J., Malandraki, O.E., 2017. Real-time prediction of the occurrence of GLE events. Space Weather 15 (7), 861–873.

Odstrcil, D., 2003. Modeling 3-d solar wind structure. Advances in Space Research 32 (4), 497–506, heliosphere at Solar Maximum. URL: https://www.sciencedirect.com/science/article/pii/S0273117703003326.

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Pacheco, D., 2019. Analysis and modelling of the solar energetic particle radiation environment in the inner heliosphere in preparation for Solar Orbiter. Ph.D. thesis, Universitat de Barcelona, Barcelona, Spain. URL: http://hdl.handle.net/10803/667033.

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