Modeling the solar cosmic ray event of 13 December 2006 using ground level neutron monitor data

[1]  Victor Yanke,et al.  Modeling ground level enhancements: Event of 20 January 2005 , 2007 .

[2]  Helen A. Mavromichalaki,et al.  Solar cosmic rays during the extremely high ground level enhancement on 23 February 1956 , 2005 .

[3]  P. Evenson,et al.  Relativistic solar neutrons and protons on 28 October 2003 , 2005 .

[4]  Lev I. Dorman,et al.  * * * * * 20% conference discount * * * * * Cosmic Rays in the Earth's Atmosphere and Underground , 2004 .

[5]  M. Shea,et al.  The October 22, 1989, solar cosmic ray enhancement: An analysis of the anisotropy and spectral characteristics , 1997 .

[6]  S. Xue,et al.  The Ground Level Enhancement of September 29, 1989 , 1991 .

[7]  M. Shea,et al.  Detection of 0.5–15 GEV solar protons on 29 September 1989 at Australian stations , 1991 .

[8]  Nikolai A. Tsyganenko,et al.  GLOBAL QUANTITATIVE MODELS OF THE GEOMAGNETIC-FIELD IN THE CISLUNAR MAGNETOSPHERE FOR DIFFERENT DISTURBANCE LEVELS , 1987 .

[9]  M. Shea,et al.  Possible evidence for a rigidity-dependent release of relativistic protons from the solar corona , 1982 .

[10]  C. Plainaki,et al.  Application of the NM-BANGLE model to GLE70 , 2008 .

[11]  G. Bazilevskaya,et al.  The GLE of December 13, 2006 according to the ground level and balloon observations , 2008 .

[12]  C. Plainaki,et al.  Ground level enhancement of the solar cosmic rays on January 20, 2005. , 2005 .

[13]  A. G. Fenton,et al.  The Ground-level Enhancements of 1989 September 29 and October 22 , 1993, Publications of the Astronomical Society of Australia.

[14]  N. Tsyganenko.  A magnetospheric magnetic field model with a warped tail current sheet , 1989 .