Micropinch formation dynamics in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>X</mml:mi></mml:math> pinches
High temporal resolution x-ray streak camera studies of micropinch formation in Cu hybrid x pinches reveal key plasma conditions. Analysis of Ne-like Cu lines indicate an average electron temperature of about 200 eV and 4.5×10^{28}m^{-3} electron density. The spectra suggest that the electron temperature jumps to about 1 keV, inferred from the continuum and the postcontinuum line emission that includes Li-like Cu lines. There is no sign of a rapid temperature change or a substantial surge in radiation emission during the 200 ps precontinuum x-ray burst, suggesting that the radiative collapse process does not play a major role in micropinch formation. Two-dimensional extended Magnetohydrodynamic (MHD) simulations, coupled to a collisional-radiative spectral analysis code, suggest the significance of the rapid radial implosion of high-temperature, low-density plasma, the axial outflow, and the dynamic plasma pressure in micropinch formation.
Authors
- D. A. Hammer (ORCID: https://orcid.org/0000-0002-6618-0580)
- Ahmed Elshafiey (ORCID: https://orcid.org/0000-0002-7373-9303)
- N. G. Chalmers (ORCID: https://orcid.org/0000-0002-1212-3142)
Institutions
- Los Alamos National Laboratory (US)
- Cornell University (US)
Publication Details
- Journal
- Physical review. E
- Published
- 2024-09-26
- DOI
- https://doi.org/10.1103/physreve.110.l033202
- Primary Topic
- Magnetic properties of thin films
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- U.S. Department of Energy
- National Nuclear Security Administration
- Sandia National Laboratories
- Los Alamos National Laboratory