Experimental analysis of self-organized structure and transport on the magnetospheric plasma device RT-1

Dipole plasma exhibits strong heterogeneities in field strength, density, temperature and other parameters, while maintaining a holistic balance. Our study of the internal structures reveals the fundamental self-organizing mechanisms operating in their simplest realization (as commonly observed in astronomical systems). Three new findings are reported from the RT-1 experiment. The creation of a high-energy electron core (similar to the radiation belts in planetary magnetospheres) is observed for the first time in a laboratory system. High-energy electrons (3–15 keV), produced by electron cyclotron heating, accumulate in a ‘belt’ located in the low-density region (high-beta value ~1 is obtained by increasing the high-energy component up to 70% of the total electrons). The dynamical process of the ‘up-hill diffusion’ (a spontaneous mechanism of creating density gradient) has been analyzed by perturbing the density by gas injection. The spontaneous density formation in the laboratory magnetosphere elucidates the self-organized plasma transport relevant to a planetary magnetosphere. The coherence-imaging spectroscopy visualized the two-dimensional profiles of ion temperature and flow velocity in the ion cyclotron resonance frequency heating. The ion temperature and flow were enhanced globally, and particularly along the magnetic field lines near the levitation magnet. These results advance our understanding of transport and self-organization not only in dipole plasmas, but in general magnetic confinement systems relevant to fusion plasmas.

[1]  J. Howard,et al.  Coherence-imaging spectroscopy for 2D distribution of ion temperature and flow velocity in a laboratory magnetosphere. , 2018, The Review of scientific instruments.

[2]  I. Yamada,et al.  Nd:YAG laser Thomson scattering diagnostics for a laboratory magnetosphere. , 2018, The Review of scientific instruments.

[3]  A. Fukuyama,et al.  Ion cyclotron resonance heating system in the RT-1 magnetospheric plasma , 2017 .

[4]  A. Fukuyama,et al.  Increase in Ion Temperature by Slow Wave Heating in Magnetosphere Plasma Device RT-1 , 2016 .

[5]  Jinil Chung,et al.  Spectro-polarimetrc optical systems for imaging plasma internal fields, structures and flows , 2015 .

[6]  M. Nishiura,et al.  Observation of particle acceleration in laboratory magnetosphere , 2015, 1507.03692.

[7]  Z. Yoshida,et al.  Improved beta (local beta >1) and density in electron cyclotron resonance heating on the RT-1 magnetosphere plasma , 2015 .

[8]  Y. Ogawa,et al.  Direct observation of transition to electron Bernstein waves from electromagnetic mode by three mode-conversion scenarios in the dipole confinement torus plasma , 2015 .

[9]  D. Gurnett,et al.  The plasma density distribution in the inner region of Saturn's magnetosphere , 2013 .

[10]  H. Saitoh,et al.  Generalized two-fluid equilibria: Understanding RT-1 experiments and beyond , 2010 .

[11]  P. Woskov,et al.  Turbulent inward pinch of plasma confined by a levitated dipole magnet , 2010 .

[12]  S. Mizumaki,et al.  Construction and Operation of an Internal Coil Device, RT-1, with a High-Temperature Superconductor , 2009 .

[13]  M. Mauel,et al.  Production and study of high-beta plasma confined by a superconducting dipole magneta) , 2006 .

[14]  S. Mizumaki,et al.  First Plasma in the RT-1 Device , 2006 .

[15]  J. Howard Vector tomography applications in plasma diagnostics , 1996 .

[16]  S. Yoshikawa Experiments on plasma confinement in internal-ring devices , 1973 .