2 citations · 4 across the 2 of their papers we have counts for
4 papers
Transport properties of Keplerian flows in extended local domains with no imposed field
Farrukh Nauman, Martin E. Pessah
We compare transport statistics of elongated incompressible shearing boxes for different Reynolds and magnetic Prandtl numbers, and , and aspect ratios, . We find…
Exploring helical dynamos with machine learning
Farrukh Nauman, Joonas Nättilä
We use ensemble machine learning algorithms to study the evolution of magnetic fields in magnetohydrodynamic (MHD) turbulence that is helically forced. We perform direct numerical…
The effects of large scale magnetic fields around young protostars and their disks
Michael Kuffmeier, Farrukh Nauman
We study the evolution of magnetic fields in accretion flows around six different sink particles in a global star formation simulation. Using the adaptive mesh refinement capabilit…
Quantifying the Imprecision of Accretion Theory and Implications for Multi-Epoch Observations of Protoplanetary Discs
Eric G. Blackman, Farrukh Nauman, Richard G. Edgar
If accretion disc emission results from turbulent dissipation, then axisymmetric accretion theory must be used as a mean field theory: turbulent flows are at most axisymmetric only…