Abstract
Bayesian inference techniques, coupled with Markov chain Monte Carlo sampling methods, are used to predict dose-time profiles for energetic solar particle events. Inputs into the predictive methodology are dose and dose-rate measurements obtained early in the event. Surrogate dose values are grouped in hierarchical models to express relationships among similar solar particle events. Models assume nonlinear, sigmoidal growth for dose throughout an event. Markov chain Monte Carlo methods are used to sample from Bayesian posterior predictive distributions for dose and dose rate. Example predictions are provided for the November 8, 2000, and August 12, 1989, solar particle events.
Original language | English |
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Pages (from-to) | 2004-2009 |
Number of pages | 6 |
Journal | IEEE Transactions on Nuclear Science |
Volume | 48 |
Issue number | 6 I |
DOIs | |
State | Published - Dec 2001 |
Event | 2001 Nuclear and Sapce Radiation Effects Conference (NSREC) - Vancouver, BC, Canada Duration: Jul 16 2001 → Jul 20 2001 |
Funding
Manuscript received July 17, 2001. This work was supported in part by the National Aeronautics and Space Administration Graduate Student Researchers Program. J. S. Neal was with the University of Tennessee, Knoxville, TN 37996 USA. He is now with the Nuclear Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831 USA (e-mail: [email protected]). L. W. Townsend is with the Nuclear Engineering Department, University of Tennessee, Knoxville, TN 37996-2300 USA (e-mail: [email protected]). Publisher Item Identifier S 0018-9499(01)10682-9.
Keywords
- Bayesian interface
- Dose prediction
- Solar particle events