PITCH-ANGLE SCATTERING OF ENERGETIC CHARGED PARTICLES IN NEARLY CONSTANT MAGNITUDE MAGNETIC TURBULENCE

We use a method developed by Roberts. that optimizes the phase angles of an ensemble of plane waves with amplitudes determined from a Kolmogorov-like power spectrum, to construct magnetic field vector fluctuations having nearly constant magnitude and large variances in its components. This is a repr...

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Main Authors: Sun, P., Jokipii, J. R., Giacalone, J.
Other Authors: Univ Arizona, Lunar & Planetary Lab
Language:en
Published: IOP PUBLISHING LTD 2016
Subjects:
Online Access:http://hdl.handle.net/10150/621389
http://arizona.openrepository.com/arizona/handle/10150/621389
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spelling ndltd-arizona.edu-oai-arizona.openrepository.com-10150-6213892016-11-20T03:00:29Z PITCH-ANGLE SCATTERING OF ENERGETIC CHARGED PARTICLES IN NEARLY CONSTANT MAGNITUDE MAGNETIC TURBULENCE Sun, P. Jokipii, J. R. Giacalone, J. Univ Arizona, Lunar & Planetary Lab diffusion magnetic fields solar wind turbulence We use a method developed by Roberts. that optimizes the phase angles of an ensemble of plane waves with amplitudes determined from a Kolmogorov-like power spectrum, to construct magnetic field vector fluctuations having nearly constant magnitude and large variances in its components. This is a representation of the turbulent magnetic field consistent with that observed in the solar wind. Charged-particle pitch-angle diffusion coefficients are determined by integrating the equations of motion for a large number of charged particles moving under the influence of forces from our predefined magnetic field. We tested different cases by varying the kinetic energy of the particles (E-p) and the turbulent magnetic field variance (sigma(2)(B)). For each combination of E-p and sigma(2)(B), we tested three different models: (1) the so-called "slab" model, where the turbulent magnetic field depends on only one spatial coordinate and has significant fluctuations in its magnitude (b=root delta B-x(2)(z)+ delta B-y(2)(z) + B-0(2)); (2) the slab model optimized with nearly constant magnitude b; and. (3) the slab model turbulent magnetic field with nearly constant magnitude plus a "variance-conserving" adjustment. In the last case, this model attempts to conserve the variance of the turbulent components (sigma(2)(Bx) + sigma(2)(By)), which is found to decrease during the optimization with nearly constant magnitude. We found that there is little or no effect on the pitch-angle diffusion coefficient D mu mu between. models 1 and 2. However, the result from model 3. is significantly different. We also introduce a new method to accurately determine the pitch-angle diffusion coefficients as a function of mu. 2016-08-03 Article PITCH-ANGLE SCATTERING OF ENERGETIC CHARGED PARTICLES IN NEARLY CONSTANT MAGNITUDE MAGNETIC TURBULENCE 2016, 827 (1):16 The Astrophysical Journal 1538-4357 10.3847/0004-637X/827/1/16 http://hdl.handle.net/10150/621389 http://arizona.openrepository.com/arizona/handle/10150/621389 The Astrophysical Journal en http://stacks.iop.org/0004-637X/827/i=1/a=16?key=crossref.4a24fa0dcb1b34abebc8365e102a7f20 © 2016. The American Astronomical Society. All rights reserved. IOP PUBLISHING LTD
collection NDLTD
language en
sources NDLTD
topic diffusion
magnetic fields
solar wind
turbulence
spellingShingle diffusion
magnetic fields
solar wind
turbulence
Sun, P.
Jokipii, J. R.
Giacalone, J.
PITCH-ANGLE SCATTERING OF ENERGETIC CHARGED PARTICLES IN NEARLY CONSTANT MAGNITUDE MAGNETIC TURBULENCE
description We use a method developed by Roberts. that optimizes the phase angles of an ensemble of plane waves with amplitudes determined from a Kolmogorov-like power spectrum, to construct magnetic field vector fluctuations having nearly constant magnitude and large variances in its components. This is a representation of the turbulent magnetic field consistent with that observed in the solar wind. Charged-particle pitch-angle diffusion coefficients are determined by integrating the equations of motion for a large number of charged particles moving under the influence of forces from our predefined magnetic field. We tested different cases by varying the kinetic energy of the particles (E-p) and the turbulent magnetic field variance (sigma(2)(B)). For each combination of E-p and sigma(2)(B), we tested three different models: (1) the so-called "slab" model, where the turbulent magnetic field depends on only one spatial coordinate and has significant fluctuations in its magnitude (b=root delta B-x(2)(z)+ delta B-y(2)(z) + B-0(2)); (2) the slab model optimized with nearly constant magnitude b; and. (3) the slab model turbulent magnetic field with nearly constant magnitude plus a "variance-conserving" adjustment. In the last case, this model attempts to conserve the variance of the turbulent components (sigma(2)(Bx) + sigma(2)(By)), which is found to decrease during the optimization with nearly constant magnitude. We found that there is little or no effect on the pitch-angle diffusion coefficient D mu mu between. models 1 and 2. However, the result from model 3. is significantly different. We also introduce a new method to accurately determine the pitch-angle diffusion coefficients as a function of mu.
author2 Univ Arizona, Lunar & Planetary Lab
author_facet Univ Arizona, Lunar & Planetary Lab
Sun, P.
Jokipii, J. R.
Giacalone, J.
author Sun, P.
Jokipii, J. R.
Giacalone, J.
author_sort Sun, P.
title PITCH-ANGLE SCATTERING OF ENERGETIC CHARGED PARTICLES IN NEARLY CONSTANT MAGNITUDE MAGNETIC TURBULENCE
title_short PITCH-ANGLE SCATTERING OF ENERGETIC CHARGED PARTICLES IN NEARLY CONSTANT MAGNITUDE MAGNETIC TURBULENCE
title_full PITCH-ANGLE SCATTERING OF ENERGETIC CHARGED PARTICLES IN NEARLY CONSTANT MAGNITUDE MAGNETIC TURBULENCE
title_fullStr PITCH-ANGLE SCATTERING OF ENERGETIC CHARGED PARTICLES IN NEARLY CONSTANT MAGNITUDE MAGNETIC TURBULENCE
title_full_unstemmed PITCH-ANGLE SCATTERING OF ENERGETIC CHARGED PARTICLES IN NEARLY CONSTANT MAGNITUDE MAGNETIC TURBULENCE
title_sort pitch-angle scattering of energetic charged particles in nearly constant magnitude magnetic turbulence
publisher IOP PUBLISHING LTD
publishDate 2016
url http://hdl.handle.net/10150/621389
http://arizona.openrepository.com/arizona/handle/10150/621389
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