Open Access
Issue
J. Space Weather Space Clim.
Volume 4, 2014
Article Number A08
Number of page(s) 11
DOI https://doi.org/10.1051/swsc/2014005
Published online 20 February 2014
  • Aran, A., B. Sanahuja, and D. Lario, Fluxes and fluences of SEP events derived from SOLPENCO, Ann. Geophys., 23, 3047–3053, 2005. [NASA ADS] [CrossRef] [Google Scholar]
  • Battarbee, M., Acceleration of Solar Energetic Particles in coronal shocks through self-generated turbulence, PhD Thesis, University of Turku, Annales Universitatis Turkuensis AI 475, 126 pp, 2013 [Google Scholar]
  • Battarbee, M., T. Laitinen, and R. Vainio, Heavy-ion acceleration and self-generated waves in coronal shocks, A&A, 535, A34, 2011. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
  • Battarbee, M., R. Vainio, T. Laitinen, and H. Hietala, Injection of thermal and suprathermal seed particles in coronal shocks of varying obliquity, A&A, 558, A110, 2013. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
  • Bell, A.R., The acceleration of cosmic rays in shock fronts. I, Mon. Not. R. Astron. Soc., 182, 147–156, 1978. [Google Scholar]
  • Cranmer, S.R., and A.A. van Ballegooijen, On the generation, propagation, and reflection of Alfvén Waves from the solar photosphere to the distant heliosphere, Astrophys. J. Suppl., 156, 265–293, 2005. [NASA ADS] [CrossRef] [Google Scholar]
  • Drury, L. O’C., An introduction to the theory of diffusive shock acceleration of energetic particles in tenuous plasmas, Rep. Prog. Phys., 46, 973–1027, 1983. [NASA ADS] [CrossRef] [Google Scholar]
  • Feynman, J., G. Spitale, J. Wang, and S. Gabriel, Interplanetary proton fluence model–JPL 1991, J. Geophys. Res., 98, 13281–13294, 1993. [CrossRef] [Google Scholar]
  • Horne, R., S. Glauert, N. Meredith, H. Koskinen, R. Vainio, et al., Forecasting the Earth’s radiation belts and modelling solar energetic particle events: Recent results from SPACECAST, J. Space Weather Space Clim., 3, A20, 2013. [CrossRef] [EDP Sciences] [Google Scholar]
  • Lario, D., and R.B. Decker, Estimation of solar energetic proton mission-integrated fluences and peak intensities for missions traveling close to the Sun, Space Weather, 9, S11003, 2011. [CrossRef] [Google Scholar]
  • Lario, D., B. Sanahuja, and A.M. Heras, Energetic particle events: Efficiency of interplanetary shocks as 50 keV < E < 100 MeV proton accelerators, Astrophys. J., 509, 415–434, 1998. [NASA ADS] [CrossRef] [Google Scholar]
  • Lario, D., M.-B. Kallenrode, R.B. Decker, E.C. Roelof, S.M. Krimigis, A. Aran, and B. Sanahuja, Radial and longitudinal dependence of solar 4–13 MeV and 27–37 MeV proton peak intensities and fluences: Helios and IMP 8 observations, Astrophys. J., 653, 1531–1544, 2006. [NASA ADS] [CrossRef] [Google Scholar]
  • Lario, D., A. Aran, N. Agueda, and B. Sanahuja, Radial dependence of proton peak intensities and fluences in SEP events: Influence of the energetic particle transport parameters, Adv. Space Res., 40 (3), 289–294, 2007. [CrossRef] [Google Scholar]
  • Lee, M.A., Coupled hydromagnetic wave excitation and ion acceleration at interplanetary traveling shocks, J. Geophys. Res., 88, 6109–6119, 1983. [NASA ADS] [CrossRef] [Google Scholar]
  • Lee, M.A., Coupled hydromagnetic wave excitation and ion acceleration at an evolving coronal/interplanetary shock, Astrophys. J. Suppl. Ser., 158, 38–67, 2005. [NASA ADS] [CrossRef] [Google Scholar]
  • Li, G., G.P. Zank, and W.K.M. Rice, Energetic particle acceleration and transport at coronal mass ejection-driven shocks, J. Geophys. Res., 108, 1082, 2013. [CrossRef] [Google Scholar]
  • Ng, C.K., and D.V. Reames, Focused interplanetary transport of approximately 1 MeV solar energetic protons through self-generated Alfvén waves, Astrophys. J., 424, 1032–1048, 1994. [NASA ADS] [CrossRef] [Google Scholar]
  • Ng, C.K., and D.V. Reames, Shock acceleration of solar energetic protons: The first 10 minutes, Astrophys. J., 686, L123–L126, 2008. [NASA ADS] [CrossRef] [Google Scholar]
  • Pomoell, J., and R. Vainio, Influence of solar wind heating formulations on the properties of shocks in the corona, Astrophys. J., 745, 151, 2012. [NASA ADS] [CrossRef] [Google Scholar]
  • Pomoell, J., R. Vainio, and R. Kissmann, MHD simulation of the evolution of shock structures in the solar corona: implications for coronal shock acceleration, Astrophys. Space Sci. Trans., 7, 387–394, 2011. [NASA ADS] [CrossRef] [Google Scholar]
  • Reames, D.V., Particle acceleration at the Sun and in the heliosphere, Space Sci. Res., 90, 413–491, 1999. [Google Scholar]
  • Reames, D.V., and C.K. Ng, Streaming-limited intensities of solar energetic particles, Astrophys. J., 504, 1002–1005, 1998. [NASA ADS] [CrossRef] [Google Scholar]
  • Rice, W.K.M., G.P. Zank, and G. Li, Particle acceleration and coronal mass ejection driven shocks: Shocks of arbitrary strength, J. Geophys. Res., 108, 1369, 2003. [CrossRef] [Google Scholar]
  • Vainio, R., On the generation of Alfvén waves by solar energetic particles, A&A, 406, 735–740, 2003. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
  • Vainio, R., and T. Laitinen, Monte Carlo simulations of coronal diffusive shock acceleration in self-generated turbulence, Astrophys. J., 658, 622–630, 2007. [NASA ADS] [CrossRef] [Google Scholar]
  • Vainio, R., and T. Laitinen, Simulations of coronal shock acceleration in self-generated turbulence, J. Atmos. Sol. Terr. Phys., 70, 467–474, 2008. [NASA ADS] [CrossRef] [Google Scholar]
  • Vainio, R., N. Agueda, A. Aran, and D. Lario, Modeling of solar energetic particles in interplanetary space. In: Space Weather, J., Lilensten, Editor, Astrophys. Space Sci. Lib, 344, Springer: Dordrecht, 27–38, 2007. [CrossRef] [Google Scholar]
  • Verkhoglyadova, O.P., G. Li, G.P. Zank, Q. Hu, and R.A. Mewaldt, Using the path code for modeling gradual SEP events in the inner heliosphere, Astrophys. J., 693, 894–900, 2009. [CrossRef] [Google Scholar]
  • Verkhoglyadova, O.P., G. Li, G.P. Zank, Q. Hu, C.M.S. Cohen, R.A. Mewaldt, G.M. Mason, D.K. Haggerty, T.T. von Rosenvinge, and M.D. Looper, Understanding large SEP events with the PATH code: Modeling of the 13 December 2006 SEP event, J. Geophys. Res., 115, A12103, 2010. [NASA ADS] [CrossRef] [Google Scholar]
  • Verkhoglyadova, O.P., G. Li, X. Ao, and G.P. Zank, Radial dependence of peak proton and iron fluxes in solar energetic particle events: Application of the PATH code, Astrophys. J., 757, 75, 2012. [CrossRef] [Google Scholar]
  • Zank, G.P., W.K.M. Rice, and C.C. Wu, Particle acceleration and coronal mass ejection driven shocks: A theoretical model, J. Geophys. Res., 105, 25079–25096, 2000. [NASA ADS] [CrossRef] [Google Scholar]

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.