GM
Giancarlo Mattia
Max Planck Institute for Astronomy, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Astrophysical Phenomena and Observations · Computational Fluid Dynamics and Aerodynamics
Employment
-
MPIA Postdoc2024 - Present
-
Istituto Nazionale di Fisica Nucleare, Sezione di Firenze Postdoctoral Researcher2022 - 2024
Education
Education history is unavailable.
Projects & Funding
Projects & funding information is unavailable.
Publications (19)
- A robust super-time-stepping scheme for Ohmic and ambipolar diffusion Save
- Role of Magnetic Reconnection in Blazar Variability Using Numerical Simulation Save
- PyPLUTO: a data analysis Python package for the PLUTO code Save
- Multidimensional half-moment multigroup radiative transfer Save
- Relativistic reconnection with effective resistivity Save
- PyPLUTO: a data analysis Python package for the PLUTO code Save
- Magnetic dissipation in short gamma-ray-burst jets Save
- A fourth-order accurate finite volume scheme for resistive relativistic MHD Save
- A 4th-order accurate finite volume method for ideal classical and special relativistic MHD based on pointwise reconstructions Save
- Amplification and Dissipation of Magnetic Fields in Accreting Compact Objects Save
- Resistive relativistic MHD simulations of astrophysical jets Save
- A comparison of approximate non-linear Riemann solvers for Relativistic MHD Save
- Exploring the disk-jet connection in NGC 315 Save
- Jets from Accretion Disk Dynamos: Consistent Quenching Modes for Dynamo and Resistivity Save
- Magnetohydrodynamic Accretion-Ejection: Jets Launched by a Nonisotropic Accretion-disk Dynamo. I. Validation and Application of Selected Dynamo Tensorial Components Save
- Magnetohydrodynamic Accretion-Ejection: Jets Launched by a Nonisotropic Accretion-disk Dynamo. II. A Dynamo Tensor Defined by the Disk Coriolis Number Save
- A constrained transport method for the solution of the resistive relativistic MHD equations Save
- A Particle Module for the PLUTO Code. I. An Implementation of the MHD-PIC Equations Save
- Linear wave wave propagation for resistive relativistic magnetohydrodynamics Save