58 citations · 228 across the 30 of their papers we have counts for
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Dynamics of Alfvén waves in partially ionized astrophysical plasmas
Dastgeer Shaikh
We develop a two dimensional, self-consistent, compressible fluid model to study evolution of Alfvenic modes in partially ionized astrophysical and space plasmas. The partially ion…
3D Hall MHD Modeling of Solar Wind Plasma Spectra
Dastgeer Shaikh, G. P. Zank
We present fully self consistent 3D simulations of compressible Hall MHD plasma that describe spectral features relevant to the solar wind plasma. We find that a spectru…
Whistler Wave Turbulence in Solar Wind Plasma
Dastgeer Shaikh, G. P. Zank
Whistler waves are present in solar wind plasma. These waves possess characteristic turbulent fluctuations that are characterized typically by the frequency and length scales that…
Self-consistent Simulations of Plasma-Neutral in a Partially Ionized Astrophysical Turbulent Plasma
Dastgeer Shaikh, G. P. Zank
A local turbulence model is developed to study energy cascades in the heliosheath and outer heliosphere (OH) based on self-consistent two-dimensional fluid simulations. The model d…
Density Spectrum in the Solar Wind Plasma
Dastgeer Shaikh, G. P. Zank
The density fluctuation spectrum in the solar wind reveals a Kolmogorov-like scaling with a spectral slope of -5/3 in wavenumber space. The energy transfer process in the magnetize…
Turbulent Density Spectrum in Solar Wind Plasma
Dastgeer Shaikh, G. P. Zank
The density fluctuation spectrum in the solar wind reveals a Kolmogorov-like scaling with a spectral slope of -5/3 in wavenumber space. The energy transfer process in the magnetize…