Titlebook: Study on Magnetohydrodynamic Turbulence and Its Astrophysical Applications; Siyao Xu Book 2019 Springer Nature Singapore Pte Ltd. 2019 gam

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Study on Magnetohydrodynamic Turbulence and Its Astrophysical Applications978-981-13-7515-6Series ISSN 2190-5053 Series E-ISSN 2190-5061

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MHD Turbulence in a Partially Ionized Medium,e extends over a remarkably large range of spatial scales and participates in key astrophysical processes happening in different ranges of scales. A significant progress has been achieved in the understanding of the magnetohydrodynamic (MHD) turbulence since the turn of the century, and this enables

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Interpretation of the Structure Function of Rotation Measure in the Interstellar Medium,ts spectral slope is inconsistent with the standard Kolmogorov scaling. This motivates us to examine the statistical analysis on RM fluctuations. The correlations of RM constructed by Lazarian and Pogosyan (ApJ 818:178, 2016 [.]) are demonstrated to be adequate in explaining the observed features of

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Scatter Broadening of Pulsars and Implications on the Interstellar Medium Turbulence,located in the Galactic plane. Correspondingly, we consider the Galactic distribution of electron density fluctuations consisting of not only a Kolmogorov density spectrum but also a short-wave-dominated density spectrum with the density structure formed at small scales due to shocks. The resulting

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On the Origin of the Scatter Broadening of Fast Radio Burst Pulses and Astrophysical Implications,r host galaxies. To account for the observed millisecond pulses caused by scatter broadening, we examine a variety of possible models of electron density fluctuations in both the IGM and the host galaxy medium. We find that a short-wave-dominated power-law spectrum of density, which may arise in hig

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