Parametric sensitivity of electron scattering effects by electrostatic electron cyclotron harmonic waves

It is well known that ECH waves can effectively precipitate hundreds of eV to tens of keV electrons into the upper atmosphere, resulting in the production of diffuse aurora. To deepen our outstanding of the contributions of ECH waves to diffuse aurora, in this study we perform a detailed analysis of the sensitivity of ECH wave-induced electron scattering to ambient magnetic field intensity, total electron density and density ratio between hot and cold electrons. Our results show that for various parameter sets, ECH waves can cause the precipitation loss of diffuse auroral electrons at energies of 100 eV to several keV and are capable of accelerating 100 eV to keV electrons at intermediate pitch angle, therefore contributing to the formation of butterfly pitch angle distribution. We also find that the variations of background parameters significantly change the magnitude of diffusion coefficients and resonant pitch angle range of &lt; ~1 keV electrons, while the scattering efficiency of &gt; ~1 keV electrons is almost unaffected. For &lt; ~1 keV electrons, an increase of magnetic field intensity or density ratio between hot and cold electrons weakens the electron scattering efficiency and narrows the resonant region to lower pitch angles, while an increase of total electron density plays an opposite role. In addition, the momentum diffusion can be stronger than pitch angle diffusion at large pitch angles for &lt; ~1 keV electrons, while it can be negligible at higher energies. <br>