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A general time-dependent stochastic method for solving Parker's transport equation in spherical coordinates

Journal of Geophysical Research: Space Physics, 2010-12, Vol.115 (A12), p.n/a

2010

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Galactic Cosmic-Ray Anistropy During the Forbush Decrease Starting 2013 April 13

Astrophysical journal. Letters, 2018-01, Vol.852 (2), p.L26

2018

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Turbulence transport throughout the heliosphere

Journal of Geophysical Research - Space Physics, 2008-08, Vol.113 (A8), p.A08105-n/a

2008

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Nonlinear Parallel and Perpendicular Diffusion of Charged Cosmic Rays in Weak Turbulence

The Astrophysical journal, 2004-11, Vol.616 (1), p.617-629

2004

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Spectral Properties and Length Scales of Two-dimensional Magnetic Field Models

The Astrophysical journal, 2007-10, Vol.667 (2), p.956-962

2007

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Analytic Forms of the Perpendicular Diffusion Coefficient in Magnetostatic Turbulence

The Astrophysical journal, 2004-04, Vol.604 (2), p.675-686

2004

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GIANT GROUND LEVEL ENHANCEMENT OF RELATIVISTIC SOLAR PROTONS ON 2005 JANUARY 20. I. SPACESHIP EARTH OBSERVATIONS

The Astrophysical journal, 2013-07, Vol.771 (2), p.1-13

2013

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Nonlinear Collisionless Perpendicular Diffusion of Charged Particles

The Astrophysical journal, 2003-06, Vol.590 (1), p.L53-L56

2003

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Parallel and Perpendicular Transport of Heliospheric Cosmic Rays in an Improved Dynamical Turbulence Model

The Astrophysical journal, 2006-05, Vol.642 (1), p.230-243

2006

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Cosmic ray diffusion tensor throughout the heliosphere

Journal of Geophysical Research. A. Space Physics, 2010-03, Vol.115 (A3), p.n/a

2010

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Determination of interplanetary coronal mass ejection geometry and orientation from ground-based observations of galactic cosmic rays

Journal of Geophysical Research - Space Physics, 2009-05, Vol.114 (A5), p.A05109-n/a

2009

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Perpendicular Transport of Charged Particles in Composite Model Turbulence: Recovery of Diffusion

The Astrophysical journal, 2002-10, Vol.578 (2), p.L117-L120

2002

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When do particles follow field lines?

Journal of Geophysical Research - Space Physics, 2009-01, Vol.114 (A1), p.A01102-n/a

2009

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Relativistic Solar Protons on 1989 October 22: Injection and Transport along Both Legs of a Closed Interplanetary Magnetic Loop

The Astrophysical journal, 2006-03, Vol.639 (2), p.1186-1205

2006

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Perpendicular Transport of Energetic Charged Particles in Nonaxisymmetric Two-Component Magnetic Turbulence

The Astrophysical journal, 2008-10, Vol.686 (2), p.1231-1244

2008

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Global Muon Detector Network Used for Space Weather Applications

Space science reviews, 2014-08, Vol.182 (1-4), p.1-18

2014

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Radial evolution of cross helicity in high-latitude solar wind

Geophysical research letters, 2005-03, Vol.32 (6), p.L06103-n/a

2005

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Transport of cross helicity and radial evolution of Alfvénicity in the solar wind

Geophysical research letters, 2004-06, Vol.31 (12), p.L12803-n/a

2004

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Subdiffusive transport of charged particles perpendicular to the large scale magnetic field

Geophysical research letters, 2002-02, Vol.29 (4), p.7-1-7-4

2002

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Drift Effects and the Cosmic Ray Density Gradient in a Solar Rotation Period: First Observation with the Global Muon Detector Network (GMDN)

The Astrophysical journal, 2008-07, Vol.681 (1), p.693-707

2008

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Parallel Diffusion of Charged Particles in Strong Two-dimensional Turbulence

The Astrophysical journal, 2006-03, Vol.640 (1), p.L103-L106

2006

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A calibration neutron monitor: Energy response and instrumental temperature sensitivity

Journal of Geophysical Research - Space Physics, 2008-08, Vol.113 (A8), p.A08101-n/a

2008

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On the Ability of Different Diffusion Theories to Account for Directly Simulated Diffusion Coefficients

The Astrophysical journal, 2007-07, Vol.663 (2), p.1049-1054

2007

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Characteristics of solar proton events associated with ground level enhancements

Journal of Geophysical Research: Space Physics, 2010-10, Vol.115 (A10), p.n/a

2010

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Precursors of the Forbush Decrease on 2006 December 14 Observed with the Global Muon Detector Network (GMDN)

The Astrophysical journal, 2010-06, Vol.715 (2), p.1239-1247

2010

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A general time-dependent stochastic method for solving Parker's transport equation in spherical coordinates

Galactic Cosmic-Ray Anistropy During the Forbush Decrease Starting 2013 April 13

Turbulence transport throughout the heliosphere

Nonlinear Parallel and Perpendicular Diffusion of Charged Cosmic Rays in Weak Turbulence

Spectral Properties and Length Scales of Two-dimensional Magnetic Field Models

Analytic Forms of the Perpendicular Diffusion Coefficient in Magnetostatic Turbulence

GIANT GROUND LEVEL ENHANCEMENT OF RELATIVISTIC SOLAR PROTONS ON 2005 JANUARY 20. I. SPACESHIP EARTH OBSERVATIONS

Nonlinear Collisionless Perpendicular Diffusion of Charged Particles

Parallel and Perpendicular Transport of Heliospheric Cosmic Rays in an Improved Dynamical Turbulence Model

Cosmic ray diffusion tensor throughout the heliosphere

Determination of interplanetary coronal mass ejection geometry and orientation from ground-based observations of galactic cosmic rays

Perpendicular Transport of Charged Particles in Composite Model Turbulence: Recovery of Diffusion

When do particles follow field lines?

Relativistic Solar Protons on 1989 October 22: Injection and Transport along Both Legs of a Closed Interplanetary Magnetic Loop

Perpendicular Transport of Energetic Charged Particles in Nonaxisymmetric Two-Component Magnetic Turbulence

Global Muon Detector Network Used for Space Weather Applications

Radial evolution of cross helicity in high-latitude solar wind

Transport of cross helicity and radial evolution of Alfvénicity in the solar wind

Subdiffusive transport of charged particles perpendicular to the large scale magnetic field

Drift Effects and the Cosmic Ray Density Gradient in a Solar Rotation Period: First Observation with the Global Muon Detector Network (GMDN)

Parallel Diffusion of Charged Particles in Strong Two-dimensional Turbulence

A calibration neutron monitor: Energy response and instrumental temperature sensitivity

On the Ability of Different Diffusion Theories to Account for Directly Simulated Diffusion Coefficients

Characteristics of solar proton events associated with ground level enhancements

Precursors of the Forbush Decrease on 2006 December 14 Observed with the Global Muon Detector Network (GMDN)

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