| Issue |
J. Space Weather Space Clim.
Volume 14, 2024
Topical Issue - CMEs, ICMEs, SEPs: Observational, Modelling, and Forecasting Advances
|
|
|---|---|---|
| Article Number | 15 | |
| Number of page(s) | 9 | |
| DOI | https://doi.org/10.1051/swsc/2024012 | |
| Published online | 28 May 2024 | |
- Afanasiev A, Battarbee M, Vainio R. 2015. Self-consistent Monte Carlo simulations of proton acceleration in coronal shocks: Effect of anisotropic pitch-angle scattering of particles. A&A 584: A81. https://doi.org/10.1051/0004-6361/201526750. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Afanasiev A, Vainio R, Trotta D, Nyberg S, Talebpour Sheshvan N, Hietala H, Dresing N. 2023. Self-consistent modeling of the energetic storm particle event of November 10, 2012. A&A 679: A111. https://doi.org/10.1051/0004-6361/202346220. [CrossRef] [EDP Sciences] [Google Scholar]
- Axford WI, Leer E, Skadron G. 1977. The acceleration of cosmic rays by shock waves. In: Proc. of 15th International Cosmic Ray Conference, vol. 11, Plovdiv, Bulgaria, August 13–26, 1977. Bulgarian Academy of Sciences, pp. 132–137. [Google Scholar]
- Bell AR. 1978. The acceleration of cosmic rays in shock fronts – I. Mon Not R Astron Soc 182: 147–156. https://doi.org/10.1093/mnras/182.2.147. [CrossRef] [Google Scholar]
- Berezhko EG, Taneev SN. 2016. Particle acceleration and Alfvén wave generation by an interplanetary shock. Astron Lett 42(2): 126–135. https://doi.org/10.1134/S1063773716010011. [CrossRef] [Google Scholar]
- Bieber JW, Matthaeus WH, Smith CW, Wanner W, Kallenrode M-B, Wibberenz G. 1994. Proton and electron mean free paths: The palmer consensus revisited. A&A 420: 294. https://doi.org/10.1086/173559. [Google Scholar]
- Blandford RD, Ostriker JP. 1978. Particle acceleration by astrophysical shocks. Astrophys J 221: L29–L32. https://doi.org/10.1086/182658. [CrossRef] [Google Scholar]
- Decker RB. 1988. Computer modeling of test particle acceleration at oblique shocks. Space Sci Rev 48(3–4): 195–262. https://doi.org/10.1007/BF00226009. [CrossRef] [Google Scholar]
- Desai M, Giacalone J. 2016. Large gradual solar energetic particle events. Living Rev Sol Phys 13(1): 3. https://doi.org/10.1007/s41116-016-0002-5. [CrossRef] [Google Scholar]
- Ding Z, Li G, Mason G, Poedts S, Kouloumvakos A, Ho G, Wijsen N, Wimmer-Schweingruber RF, Rodríguez-Pacheco J.. 2024. Modelling two energetic storm particle events observed by Solar Orbiter using the combined EUHFORIA and iPATH models. A&A 681: A92. https://doi.org/10.1051/0004-6361/202347506. [CrossRef] [EDP Sciences] [Google Scholar]
- Ding Z, Wijsen N, Li G, Poedts S. 2022. Modeling the 2020 November 29 solar energetic particle event using EUHFORIA and iPATH models. A&A 668: A71. https://doi.org/10.1051/0004-6361/202244732. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Drury LO. 1983. Review article: An introduction to the theory of diffusive shock acceleration of energetic particles in tenuous plasmas. Rep Prog Phys 46(8): 973–1027. https://doi.org/10.1088/0034-4885/46/8/002. [CrossRef] [Google Scholar]
- Fraschetti F. 2021. Effect of acceleration and escape of energetic particles on spectral steepening at shocks. Astrophys J 909(1): 42. https://doi.org/10.3847/1538-4357/abd699. [CrossRef] [Google Scholar]
- Gordon BE, Lee MA, Möbius E, Trattner KJ. 1999. Coupled hydromagnetic wave excitation and ion acceleration at interplanetary traveling shocks and Earth’s bow shock revisited. J Geophys Res Space Phys 104(A12): 28263–28278. https://doi.org/10.1029/1999JA900356. [CrossRef] [Google Scholar]
- Hu J, Li G, Ao X, Zank GP, Verkhoglyadova O. 2017. Modeling particle acceleration and transport at a 2-D CME-driven shock. J Geophys Res (Space Phys) 122(11): 10938–10963. https://doi.org/10.1002/2017JA024077. [Google Scholar]
- Kocharov LG, Torsti J, Vainio R, Kovaltsov GA. 1996. Propagation of solar cosmic rays: Diffusion versus focused diffusion. Sol Phys 165(1): 205–208. https://doi.org/10.1007/BF00149100. [CrossRef] [Google Scholar]
- Krymskii GF. 1977. A regular mechanism for the acceleration of charged particles on the front of a shock wave. Akad Nauk SSSR Dokl 234: 1306–1308. [Google Scholar]
- Lee MA. 1983. Coupled hydromagnetic wave excitation and ion acceleration at interplanetary traveling shocks. J Geophys Res Space Phys 88(A8): 6109–6120. https://doi.org/10.1029/JA088iA08p06109. [CrossRef] [Google Scholar]
- Li G, Zank GP, Rice WKM. 2005. Acceleration and transport of heavy ions at coronal mass ejection-driven shocks. J Geophys Res Space Phys 110(A6): A06104. https://doi.org/10.1029/2004JA010600. [Google Scholar]
- Ng CK, Reames DV. 2008. Shock acceleration of solar energetic protons: The first 10 minutes. Astrophys J 686(2): L123. https://doi.org/10.1086/592996. [CrossRef] [Google Scholar]
- Palmer ID. 1982. Transport coefficients of low-energy cosmic rays in interplanetary space. Rev Geophys Space Phys 20: 335–351. https://doi.org/10.1029/RG020i002p00335. [CrossRef] [Google Scholar]
- Reames DV. 2023. How do shock waves define the space-time structure of gradual solar energetic particle events?. Space Sci Rev 219(1): 14. https://doi.org/10.1007/s11214-023-00959-x. [CrossRef] [Google Scholar]
- Rice WKM, Zank GP, Li G. 2003. Particle acceleration and coronal mass ejection driven shocks: Shocks of arbitrary strength. J Geophys Res (Space Phys) 108(A10): 1369. https://doi.org/10.1029/2002JA009756. [Google Scholar]
- Roelof EC. 1969. Propagation of solar cosmic rays in the interplanetary magnetic field. In: Lectures in High-Energy Astrophysics, Ögelman H, Wayland JR (Eds.), Scientific and Technical Information Division, Office of Technology Utilization, NASA, Washington, DC, p. 111. [Google Scholar]
- Ruffolo D. 1995. Effect of adiabatic deceleration on the focused transport of solar cosmic rays. Astrophys J 442: 861. https://doi.org/10.1086/175489. [CrossRef] [Google Scholar]
- Vainio R. 2006. Acceleration of SEPs: Role of CME-associated shocks and turbulence. In: Washington DC American Geophysical Union Geophysical Monograph Series, vol. 165, pp. 253–262. https://doi.org/10.1029/165GM24. [Google Scholar]
- Vainio R, Desorgher L, Heynderickx D, Storini M, Flückiger E, et al. 2009. Dynamics of the Earth’s particle radiation environment. Space Sci Rev 147(3–4): 187–231. https://doi.org/10.1007/s11214-009-9496-7. [CrossRef] [Google Scholar]
- Vainio R, Kocharov L, Laitinen T. 2000. Interplanetary and interacting protons accelerated in a parallel shock wave. Astrophys J 528(2): 1015–1025. https://doi.org/10.1086/308202. [CrossRef] [Google Scholar]
- Vainio R, Laitinen T. 2007. Monte Carlo simulations of coronal diffusive shock acceleration in self-generated turbulence. Astrophys J 658(1): 622–630. https://doi.org/10.1086/510284. [CrossRef] [Google Scholar]
- Vainio R, Pönni A, Battarbee M, Koskinen HEJ, Afanasiev A, Laitinen T. 2014. A semi-analytical foreshock model for energetic storm particle events inside 1 AU. J Space Weather Space Clim 4: A08. https://doi.org/10.1051/swsc/2014005. [CrossRef] [EDP Sciences] [Google Scholar]
- Wijsen N, Aran A, Scolini C, Lario D, Afanasiev A, Vainio R, Sanahuja B, Pomoell J, Poedts S. 2022. Observation-based modelling of the energetic storm particle event of 14 July 2012. A&A 659: A187. https://doi.org/10.1051/0004-6361/202142698. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Wijsen N, Lario D, Sánchez-Cano B, Jebaraj IC, Dresing N, et al. 2023. The effect of the ambient solar wind medium on a CME-driven shock and the associated gradual solar energetic particle event. Astrophys J 950(2): 172. https://doi.org/10.3847/1538-4357/acd1ed. [CrossRef] [Google Scholar]
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