ECRIS 2024 - Proceedings Management

Simulation of Bremsstrahlung emission in ECRIS and its dependence on the magnetic confinement

TUC2

Sep 17, 2024, 2:00 PM

30m

Main Hall (Welcome Hotel Darmstadt City Center)

Oral Presentation MC3: Fundamental Process and Plasma Studies TUC: Oral Session MC3

Speaker

Andrea Cernuschi (Laboratoire de Physique Subatomique et de Cosmologie)

Description

A Monte Carlo (MC) code dedicated to the electron dynamics in ECRIS was recently completed with a new functionality, allowing to simulate Bremsstrahlung photon emission from the volume interaction of electrons with charged particles inside the plasma. The simulation qualitatively reproduces the experimental anisotropy of the photon spectral temperature previously reported. The effects of variations in the magnetic field minimum Bmin and in the extraction peak on both the electron energy distribution function and the Bremsstrahlung emission are also investigated and reported. The simulation results confirm that only changes in Bmin influences the hot energy tail of the EEDF *. The MC high electron statistics allows studying with unprecedent details the location and mechanism responsible for the hot electrons generation in ECRIS, highlighting the crucial role of Bmin in this process.

Footnotes

• J. Benitez, C. Lyneis, L. Phair, D. Todd, and D. Xie, IEEE Transactions on Plasma Science 45, 1746 (2017).

Funding Agency

This work is supported by Agence Nationale de la Recherche with the contract # 21-ESRE-0018 EQUIPEX+ NEWGAIN.