Sponsor:
The authors want to thank Professor Jesús Ramos from the Massachusetts Institute of Technology, and Dr Jaume Navarro, Dr Gonzalo Sánchez-Arriaga, and Dr Pablo Fajardo from Universidad Carlos III de Madrid for many insightful discussions and comments.This work has been supported by ESA project 4000116180/15/NL/PS. The work of Javier Mauriño has been supported by the UK Royal Academy of Engineering's Engineering Leaders Scholarship (ELAA1516/1/87).
Keywords:
Electric propulsion
,
Plasma thrusters
,
Plasma plumes
,
Kinetic models
,
Collisionless plasma
,
Electron cooling
A paraxial model of an unmagnetized, collisionless plasma plume expanding into vacuum is presented. Electrons are treated kinetically, relying on the adiabatic invariance of their radial action integral for the integration of Vlasov's equation, whereas ions arA paraxial model of an unmagnetized, collisionless plasma plume expanding into vacuum is presented. Electrons are treated kinetically, relying on the adiabatic invariance of their radial action integral for the integration of Vlasov's equation, whereas ions are treated as a cold species. The quasi-2D plasma density, self-consistent electric potential, and electron pressure, temperature, and heat fluxes are analyzed. In particular, the model yields the collisionless cooling of electrons, which differs from the Boltzmann relation and the simple polytropic laws usually employed in fluid and hybrid PIC/fluid plume codes.[+][-]