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Large-scale Magnetic Structure Formation in 3D-MHD Turbulence
Shiva Kumar Malapaka, Wolf-Christian Müller
The inverse cascade of magnetic helicity in 3D-MHD turbulence is believed to be one of the processes responsible for large scale magnetic structure formation in astrophysical syste…
Modeling Statistical Properties of Solar Active Regions through DNS of 3D-MHD Turbulence
Shiva Kumar. Malapaka, Wolf-Christian Mueller
Statistical properties of the Sun's photospheric turbulent magnetic field, especially those of the Active Regions (ARs), have been studied using the line-of-sight data from magneto…
Role of helicities for the dynamics of turbulent magnetic fields
Wolf-Christian Müller, Shiva Kumar. Malapaka
Investigations of the inverse cascade of magnetic helicity are conducted with pseudospectral, three-dimensional direct numerical simulations of forced and decaying incompressible m…