Adapts FLASH code for MHD rigid body simulations to model non-magnetized planet-stellar wind interactions and examine viscosity influence on flow patterns.
Bourrier, et al., Astron
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
physics.space-ph 1years
2019 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Simulating the interaction of a non-magnetized planet with the stellar wind produced by a sun-like star using the FLASH Code
Adapts FLASH code for MHD rigid body simulations to model non-magnetized planet-stellar wind interactions and examine viscosity influence on flow patterns.