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SDR, EVC, and SDREVC: Limitations and Extensions

by Ulmer, S. , Killian, C. , Widmann, E. , Murtagh, D.J. , Malbrunot, C. , Costantini, G. , Tajima, M. , Breuker, H. , Nanda, A. , Leali, M. , Amsler, C. , Zmeskal, J. , Matsuda, Y. , Maero, G. , Migliorati, S. , Chesnevskaya, S. , Kraxberger, V. , Simon, M.C. , Hunter, E.D. , Rheinfrank, S. , Toso, V. , Mäckel, V. , Kuroda, N. , Giammarchi, M. , Yamazaki, Y. , Higaki, H. , Romé, M. , Gosta, G. , Lanz, A. , Mascagna, V. , Nowak, L. , Bumbar, M. , Weiser, A. , Ferragut, R. , Gligorova, A. , Venturelli, L. , Parnefjord Gustafsson, F.

in Charged particles / Compressive strength / Electrodes / Evaporative cooling / Magnetic fields / Magnetic mirrors / Non-Neutral Plasmas: Achievements and Perspectives / Plasma / Plasma density / Plasma physics / Radiation / Space charge

2023

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2023

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2023

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Journal Article

SDR, EVC, and SDREVC: Limitations and Extensions

Ulmer, S.,

Killian, C.,

Widmann, E.,

Murtagh, D.J.,

Malbrunot, C.,

Costantini, G.,

Tajima, M.,

Breuker, H.,

Nanda, A.,

Leali, M.,

Amsler, C.,

Zmeskal, J.,

Matsuda, Y.,

Maero, G.,

Migliorati, S.,

Chesnevskaya, S.,

Kraxberger, V.,

Simon, M.C.,

Hunter, E.D.,

Rheinfrank, S.,

Toso, V.,

Mäckel, V.,

Kuroda, N.,

Giammarchi, M.,

Yamazaki, Y.,

Higaki, H.,

Romé, M.,

Gosta, G.,

Lanz, A.,

Mascagna, V.,

Nowak, L.,

Bumbar, M.,

Weiser, A.,

Ferragut, R.,

Gligorova, A.,

Venturelli, L.,

Parnefjord Gustafsson, F.

2023

Overview

Methods for reducing the radius, temperature and space charge of a non-neutral plasma are usually reported for conditions which approximate an ideal Penning Malmberg trap. Here, we show that (i) similar methods are still effective under surprisingly adverse circumstances: we perform strong drive regime (SDR) compression and SDREVC in a strong magnetic mirror field using only 3 out of 4 rotating wall petals. In addition, we demonstrate (ii) an alternative to SDREVC, using e-kick instead of evaporative cooling (EVC) and (iii) an upper limit for how much plasma can be cooled to $T<20\\ \\mathrm {K}$ using EVC. This limit depends on the space charge, not on the number of particles or the plasma density.

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Publisher

Cambridge University Press

Subject

Charged particles

/ Compressive strength

/ Electrodes

/ Evaporative cooling

/ Magnetic fields

/ Magnetic mirrors

/ Non-Neutral Plasmas: Achievements and Perspectives