A parameter-free dynamic alternative to hyper-viscosity for coupled transport equations: Application to the simulation of 3D squall lines using spectral elements

2015 ◽  
Vol 283 ◽  
pp. 360-373 ◽  
Author(s):  
Simone Marras ◽  
Francis X. Giraldo
2017 ◽  
Vol 75 (5) ◽  
pp. 1047-1073 ◽  
Author(s):  
Arnd Scheel ◽  
Angela Stevens

2010 ◽  
Vol 6 (S275) ◽  
pp. 313-314
Author(s):  
Florencia L. Vieyro ◽  
Gustavo E. Romero

AbstractWe present a model for high-energy flares in accreting black holes based on the injection in a magnetized corona of a non-thermal population of relativistic particles. Coupled transport equations are solved for all species of particles and the electromagnetic and neutrino output is predicted for the case of Galactic black holes.


2021 ◽  
Author(s):  
Xiaojun Yao ◽  
Weiyao Ke ◽  
Yingru Xu ◽  
Steffen A. Bass ◽  
Berndt Mueller

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