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The Pencil Code, a modular MPI code for partial differential equations and particles: multipurpose and multiuser-maintained
The Pencil Code is a highly modular physics-oriented simulation code that can be adapted
to a wide range of applications. It is primarily designed to solve partial differential equations …
to a wide range of applications. It is primarily designed to solve partial differential equations …
Numerical evidence for a small-scale dynamo approaching solar magnetic Prandtl numbers
Magnetic fields on small scales are ubiquitous in the Universe. Although they can often be
observed in detail, their generation mechanisms are not fully understood. One possibility is …
observed in detail, their generation mechanisms are not fully understood. One possibility is …
Data-driven simulations of magnetic field evolution in active region 11429: Magneto-frictional method using pencil code
Coronal magnetic fields evolve quasi-statically over long timescales and dynamically over
short timescales. As of now there exist no regular measurements of coronal magnetic fields …
short timescales. As of now there exist no regular measurements of coronal magnetic fields …
Dust growth by accretion of molecules in supersonic interstellar turbulence
We show that the growth rate of dust grains in cold molecular clouds is enhanced by the
high degree of compressibility of a turbulent, dilute gas. By means of high-resolution (1024 …
high degree of compressibility of a turbulent, dilute gas. By means of high-resolution (1024 …
Constraining the inner boundaries of COCONUT through plasma β and Alfvén speed
Context. Space weather modelling has been gaining importance due to our increasing
dependency on technology sensitive to space weather effects, such as satellite services, air …
dependency on technology sensitive to space weather effects, such as satellite services, air …
Granulation and Convectional Driving on Stellar Surfaces
J Tschernitz, PA Bourdin - The Astrophysical Journal Letters, 2025 - iopscience.iop.org
Surface convection is important for the presence of magnetic activity at stars. So far, this
convection is thought to be a result of heating from below, where convection cells rise and …
convection is thought to be a result of heating from below, where convection cells rise and …
Investigating numerical stability by scaling heat conduction in a 1D hydrodynamic model of the solar atmosphere
Context. Numerical models of the solar atmosphere are widely used in solar research and
provide insights into unsolved problems such as the heating of coronal loops. A prerequisite …
provide insights into unsolved problems such as the heating of coronal loops. A prerequisite …
Coagulation of inertial particles in supersonic turbulence
Coagulation driven by supersonic turbulence is primarily an astrophysical problem because
coagulation processes on Earth are normally associated with incompressible fluid flows at …
coagulation processes on Earth are normally associated with incompressible fluid flows at …