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• W2508272616 abstract "Turbulent magnetic fields permeate our universe, impacting a wide range of astronomical phenomena across all cosmic scales. A clear example is the magnetic field that threads the interstellar medium (ISM), which impacts the motion of cosmic rays through that medium. Understanding the structure of magnetic within the ISM and how it relates to the physical quantities that characterize it can thus inform our analysis of particle transport within these regions. Toward that end, we probe the structure of magentic through the use of Lyapunov exponents for a suite of isotropic and nonisotropic Alfvenic profiles. Our results provide a means of calculating a turbulence lengthscale that can then be connected to how cosmic rays propagate through magentically turbulent environments, and we perform such an analysis for molecular cloud environments." @default.
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• W2508272616 date "2016-09-02" @default.
• W2508272616 modified "2023-10-17" @default.
• W2508272616 title "Assessing the Structure of Isotropic and Anisotropic Turbulent Magnetic Fields" @default.
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• W2508272616 doi "https://doi.org/10.1088/1538-3873/128/968/104301" @default.
• W2508272616 hasPublicationYear "2016" @default.
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