103 citations · 248 across the 10 of their papers we have counts for
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Large-Scale High-Lundquist Number Reduced MHD Simulations of the Solar Corona Using GPU Accelerated Machines
L. Lin, C. S. Ng, A. Bhattacharjee
We have recently carried out a computational campaign to investigate a model of coronal heating in three-dimensions using reduced magnetohydrodynamics (RMHD). Our code is built on…
Generalizations of a Nonlinear Fluid Model for Void Formation in Dusty Plasmas
C. S. Ng, A. Bhattacharjee, S. Hu +2
New developments in the theory and numerical simulation of a recently proposed one-dimensional nonlinear time-dependent fluid model [K. Avinash, A. Bhattacharjee, and S. Hu, Phys.…
A Constrained Tectonics Model for Coronal Heating
C. S. Ng, A. Bhattacharjee
An analytical and numerical treatment is given of a constrained version of the tectonics model developed by Priest, Heyvaerts, & Title [2002]. We begin with an initial uniform magn…
Kolmogorov versus Iroshnikov-Kraichnan spectra: Consequences for ion heating in the solar wind
C. S. Ng, A. Bhattacharjee, D. Munsi +2
Whether the phenomenology governing MHD turbulence is Kolmogorov or Iroshnikov-Kraichnan (IK) remains an open question, theoretically as well as observationally. The ion heating pr…
High-Lundquist Number Scaling in Three-Dimensional Simulations of Parker's Model of Coronal Heating
C. S. Ng, L. Lin, A. Bhattacharjee
Parker's model is one of the most discussed mechanisms for coronal heating and has generated much debate. We have recently obtained new scaling results in a two-dimensional (2D) ve…
Fast magnetic reconnection in laser-produced plasma bubbles
W. Fox, A. Bhattacharjee, K. Germaschewski
Recent experiments have observed magnetic reconnection in high-energy-density, laser-produced plasma bubbles, with reconnection rates observed to be much higher than can be explain…