Development and Application of Stochastic Methods for Radiation Belt Simulations

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dc.contributor.advisorChan, Anthony A
dc.contributor.committeeMemberWolf, Richard A
dc.contributor.committeeMemberDugan, Brandon
dc.creatorZheng, Liheng
dc.date.accessioned2016-02-05T21:29:41Z
dc.date.available2016-02-05T21:29:41Z
dc.date.created2015-12
dc.date.issued2015-09-04
dc.date.submittedDecember 2015
dc.date.updated2016-02-05T21:29:41Z
dc.description.abstractThis thesis describes a method for modeling radiation belt electron diffusion, which solves the radiation belt Fokker-Planck equation using its equivalent stochastic differential equations, and presents applications of this method to investigating drift shell splitting effects on radiation belt electron phase space density. The theory of the stochastic differential equation method of solving Fokker-Planck equations is formulated in this thesis, in the context of the radiation belt electron diffusion problem, and is generalized to curvilinear coordinates to enable calculation of the electron phase space density as a function of adiabatic invariants M, K and L. Based on this theory, a three-dimensional radiation belt electron model in adiabatic invariant coordinates, named REM (for Radbelt Electron Model), is constructed and validated against both known results from other methods and spacecraft measurements. Mathematical derivations and the essential numerical algorithms that constitute REM are presented in this thesis. As the only model to date that can solve the fully three-dimensional diffusion problem, REM is used to study the effects of drift shell splitting, which gives rise to M-L and K-L off-diagonal terms in the radiation belt diffusion tensor. REM simulation results suggest that drift shell splitting reduces outer radiation belt electron phase space density enhancements during electron injection events. Plots of the phase space density sources, which are unique products of the stochastic differential equation method, and theoretical analysis further reveal that this reduction effect is caused by a change of the phase space location of the source to smaller $L$ shells, and has a limit corresponding to two-dimensional local diffusion on a curved surface in the (M,K,L) phase space.
dc.format.mimetypeapplication/pdf
dc.identifier.citationZheng, Liheng. "Development and Application of Stochastic Methods for Radiation Belt Simulations." (2015) Diss., Rice University. <a href="https://hdl.handle.net/1911/88411">https://hdl.handle.net/1911/88411</a>.
dc.identifier.urihttps://hdl.handle.net/1911/88411
dc.language.isoeng
dc.rightsCopyright is held by the author, unless otherwise indicated. Permission to reuse, publish, or reproduce the work beyond the bounds of fair use or other exemptions to copyright law must be obtained from the copyright holder.
dc.subjectradiation belt
dc.subjectelectron diffusion
dc.subjectFokker-Planck equation
dc.subjectstochastic differential equation
dc.subjectmodeling
dc.titleDevelopment and Application of Stochastic Methods for Radiation Belt Simulations
dc.typeThesis
dc.type.materialText
thesis.degree.departmentPhysics and Astronomy
thesis.degree.disciplineNatural Sciences
thesis.degree.grantorRice University
thesis.degree.levelDoctoral
thesis.degree.majorSpace Physics
thesis.degree.nameDoctor of Philosophy
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