We present, in this two-part article, an extensive study on the influence
that the magnitudes of the applied electric (E) and magnetic (B) fields have on
a collisionless plasma discharge of xenon, krypton, and argon in a 2D
radial-azimuthal configuration with perpendicular orientation of the fields.
The dependency of the behavior and the underlying processes of ExB discharges
on the strength of electromagnetic field and ion mass has not yet been studied
in depth and in a manner that can distinguish the role of each individual
factor. This has been, on the one hand, due to the significant computational
cost of conventional high-fidelity particle-in-cell (PIC) codes that do not
allow for extensive simulations over a broad parameter space within practical
timeframes. On the other hand, the experimental efforts have been limited, in
part, by the measurements' spatial and temporal resolution. In this sense, the
notably reduced computational cost of the reduced-order PIC scheme enables to
numerically cast light on the parametric variations in various aspects of the
physics of ExB discharges, such as high resolution spatial-temporal mappings of
the plasma instabilities. In part I of the article, we focus on the effects of
the E-field intensity. We demonstrate that the intensity of the field
determines two distinct plasma regimes, which are characterized by different
dominant instability campaigns. At relatively low E-field magnitudes, the
Modified Two Stream Instability (MTSI) is dominant, whereas, at relatively high
E-field magnitudes, the MTSI is mitigated, and the Electron Cyclotron Drift
Instability (ECDI) becomes dominant. These two regimes are identified for all
studied propellants. Consequent to the change in the plasma regime, the radial
distribution of the axial electron current density and the electron temperature
anisotropy vary.Comment: 20 pages, 16 figure