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@inproceedings{pidatella:ecris2020-tuyzo01, author = {A. Pidatella and A. Galatà and D. Mascali and B. Mishra and E. Naselli and G. Torrisi}, title = {{Advancements in Self-Consistent Modeling of Time- and Space-Dependent Phenomena in ECRIS Plasma}}, booktitle = {Proc. ECRIS'20}, % booktitle = {Proc. 24th International Workshop on ECR Ion Sources (ECRIS'20)}, pages = {78--83}, eid = {TUYZO01}, language = {english}, keywords = {plasma, electron, ECR, ECRIS, cyclotron}, venue = {East Lansing, MI, USA}, series = {International Workshop on ECR Ion Sources}, number = {24}, publisher = {JACoW Publishing, Geneva, Switzerland}, month = {07}, year = {2022}, issn = {2222-5692}, isbn = {978-3-95450-226-4}, doi = {10.18429/JACoW-ECRIS2020-TUYZO01}, url = {https://jacow.org/ecris2020/papers/tuyzo01.pdf}, abstract = {{Resonant interaction with microwave radiation in ECRIS plasma leads to a strongly anisotropic electron energy distribution function (EEDF), given as a combination of two to three electron populations, with anisotropy that might trigger kinetic instabilities. At the INFN, further efforts have been paid to improve and update self-consistent 3D numerical codes for plasma electrons kinetics. Progresses have opened several perspectives. It is now possible to derive a space-resolved EEDF, providing local information on electron properties. Also, the code has been updated to provide reaction rates of electromagnetic emissions, including X-ray fluorescence. Estimates of the local ion charge state distribution is potentially possible, and first evaluations are ongoing. Dealing with fast-transient mechanisms, such as electromagnetic emission via the electron-cyclotron MASER instability, the code is now updated for locally evaluating the EEDF anisotropy. We will present the collected results, which we believe to have a relevant impact both on the ECRIS plasma physics and on the INFN’s PANDORA project that plans to use ECR plasmas for fundamental studies in Nuclear and AstroNuclear Physics.}}, }