Predicting dose-time profiles of solar energetic particle events using Bayesian forecasting methods

John S. Neal, Lawrence W. Townsend

Research output: Contribution to journalConference articlepeer-review

15 Scopus citations

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 languageEnglish
Pages (from-to)2004-2009
Number of pages6
JournalIEEE Transactions on Nuclear Science
Volume48
Issue number6 I
DOIs
StatePublished - Dec 2001
Event2001 Nuclear and Sapce Radiation Effects Conference (NSREC) - Vancouver, BC, Canada
Duration: Jul 16 2001Jul 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

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