Pablo Fajardo

Dr. Pablo Fajardo

orcid

Research Focus & Metrics

Academic Career Length

19Years (2008-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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1 March 2012 in Energy Conversion and Management
Verified
Journal Article
Closed access
FPF. Payri
F. Payri
Jose Ramón SerranoJose Ramón Serrano
Jose Ramón Serrano
Pablo FajardoPablo Fajardo
Pablo Fajardo
Miguel A. Reyes-BelmonteMiguel A. Reyes-Belmonte
Miguel A. Reyes-Belmonte
RGR. Gozalbo-Belles
R. Gozalbo-Belles

1 March 2018 in Vacuum
Verified
Journal Article
Closed access
Jaume NavarroJaume Navarro
Jaume Navarro
MWM. Wijnen
M. Wijnen
Pablo FajardoPablo Fajardo
Pablo Fajardo
EAE. Ahedo
E. Ahedo

30 October 2018 in Plasma Sources Science and Technology
Verified
Journal Article
Closed access
PDF file
ADA Domínguez-Vázquez
A Domínguez-Vázquez
FCFilippo Cichocki
Filippo Cichocki
Mario MerinoMario Merino
Mario Merino
Pablo FajardoPablo Fajardo
Pablo Fajardo
EAEduardo Ahedo
Eduardo Ahedo
The expansion of a rarefied axisymmetric plume emitted by a plasma thruster is analyzed and compared with a 3D Cartesian-type and a 2D cylindrical-type simulation code, both based on a particle-in-cell formulation for the heavy species and a simple Boltzmann-type model for the electrons. The first part of the paper discusses the 2D code numerical challenges in the moving of particles, their generation within the cells, and the weighting to the nodes, caused by the radial non-uniformity and the singular and boundary character of the symmetry axis. The second part benchmarks the 2D code against the 3D one for a high-energy, unmagnetized plume with three major species populations (injected neutrals, singly-charged and doubly-charged ions) and three minor species populations (constituted by particles coming from collisional processes, such as the charge-exchange reactions). The excellent agreement found in the results proves that both plume codes are capable of simulating, with a reasonable noise level, heavy particle populations differing by several orders of magnitude in number density. For simulations with a comparable level of accuracy, the 2D code presents a ten-fold gain in computational cost, although the symmetry axis remains its weakest point, due to particle depletion there and the related weighting noise.

1 September 2014 in Energy Conversion and Management
Verified
Journal Article
Open access
JGJosé Galindo
José Galindo
ATA. Tiseira
A. Tiseira
Pablo FajardoPablo Fajardo
Pablo Fajardo
LGLuis Miguel García-Cuevas
Luis Miguel García-Cuevas

10 March 2022 in Journal of Applied Physics
Verified
Journal Article
Open access
PDF file
JPJ. Perales-Díaz
J. Perales-Díaz
ADA. Domínguez-Vázquez
A. Domínguez-Vázquez
Pablo FajardoPablo Fajardo
Pablo Fajardo
EAE. Ahedo
E. Ahedo
FFFarbod Faraji
Farbod Faraji
TATommaso Andreussi
Tommaso Andreussi
Numerical simulations of a magnetically shielded Hall effect thruster with a centrally mounted cathode are performed with an axisymmetric hybrid particle-in-cell/fluid code and are partially validated with experimental data. A full description of the plasma discharge inside the thruster chamber and in the near plume is presented and discussed, with the aim of highlighting those features most dependent on the magnetic configuration and the central cathode. Compared to traditional magnetic configurations, the acceleration region is mainly outside the thruster, whereas high plasma densities and low temperatures are found inside the thruster. Thus, magnetic shielding does not decrease plasma currents to the walls, but reduces significantly the energy fluxes, yielding low heat loads and practically no wall erosion. The injection of neutrals at the central cathode generates a secondary plasma plume that merges with the main one and facilitates much the drift of electrons toward the chamber. Once inside, the magnetic topology is efficient in channeling electron current away from lateral walls. Current and power balances are analyzed to assess performances in detail.