Elucidating the collimation of laboratory plasma jets using soft x-ray interferometry

2009 ◽  
Author(s):  
M. A. Purvis ◽  
J. Grava ◽  
J. Filevich ◽  
D. P. Ryan ◽  
S. J. Moon ◽  
...  
Keyword(s):  
Author(s):  
Sun Jin-ren ◽  
Wang Chen ◽  
Fang Zhi-heng ◽  
Wang Wei ◽  
Xiong Jun ◽  
...  
Keyword(s):  

2021 ◽  
Vol 28 (8) ◽  
pp. 082703
Author(s):  
J. T. Banasek ◽  
S. V. R. Rocco ◽  
W. M. Potter ◽  
E. S. Lavine ◽  
C. E. Seyler ◽  
...  

2020 ◽  
Vol 27 (6) ◽  
pp. 062708
Author(s):  
J. T. Banasek ◽  
S. V. R. Rocco ◽  
W. M. Potter ◽  
E. S. Lavine ◽  
B. R. Kusse ◽  
...  

1990 ◽  
Vol 115 ◽  
pp. 21-31
Author(s):  
W. H. Goldstein

AbstractPrecision spectroscopy of solar plasmas has historically been the goad for advances in calculating the atomic physics and dynamics of highly ionized atoms. Recent efforts to understand the laboratory plasmas associated with magnetic and inertial confinement fusion, and with X-ray laser research, have played a similar role. Developments spurred by laboratory plasma research are applicable to the modeling of high-resolution spectra from both solar and cosmic X-ray sources, such as the photo-ionized plasmas associated with accretion disks. Three of these developments in large scale atomic modeling are reviewed: a new method for calculating large arrays of collisional excitation rates, a sum rule based method for extending collisional-radiative models and modeling the effects of autoionizing resonances, and a detailed level accounting calculation of resonant excitation rates in FeXVII.


2008 ◽  
Vol 4 (S259) ◽  
pp. 201-210
Author(s):  
Fernando Moreno-Insertis

AbstractMagnetized plasma is emerging continually from the solar interior into the atmosphere. Magnetic flux emergence events and their consequences in the solar atmosphere are being observed with high space, time and spectral resolution by a large number of space missions in operation at present (e.g. SOHO, Hinode, Stereo, Rhessi). The collision of an emerging and a preexisting magnetic flux system in the solar atmosphere leads to the formation of current sheets and to field line reconnection. Reconnection under solar coronal conditions is an energetic event; for the field strengths, densities and speeds involved in the collision of emerging flux systems, the reconnection outflows lead to launching of high-speed (hundreds of km/s), high-temperature (107 K) plasma jets. Such jets are being observed with the X-Ray and EUV detectors of ongoing satellite missions. On the other hand, the spectacular increase in computational power in recent years permits to carry out three-dimensional numerical experiments of the time evolution of flux emerging systems and the launching of jets with a remarkable degree of detail.In this review, observation and modeling of the solar X-Ray jets are discussed. A two-decade long computational effort to model the magnetic flux emergence events by different teams has led to numerical experiments which explain, even quantitatively, many of the observed features of the X-ray jets. The review points out that, although alternative mechanisms must be considered, flux emergence is a prime candidate to explain the launching of the solar jets.


2008 ◽  
Vol 78 (1) ◽  
Author(s):  
Jonathan Grava ◽  
Michael A. Purvis ◽  
Jorge Filevich ◽  
Mario C. Marconi ◽  
Jorge J. Rocca ◽  
...  

Solar Physics ◽  
1994 ◽  
Vol 155 (1) ◽  
pp. 203-206 ◽  
Author(s):  
H. Aurass ◽  
K. -L. Klein ◽  
P. C. H. Martens

2014 ◽  
Vol 81 (2) ◽  
Author(s):  
S. C. Hsu ◽  
A. L. Moser ◽  
E. C. Merritt ◽  
C. S. Adams ◽  
J. P. Dunn ◽  
...  

We describe a laboratory plasma physics experiment at Los Alamos National Laboratory that uses two merging supersonic plasma jets formed and launched by pulsed-power-driven railguns. The jets can be formed using any atomic species or mixture available in a compressed-gas bottle and have the following nominal initial parameters at the railgun nozzle exit: ne ≈ ni ~ 1016 cm−3, Te ≈ Ti ≈ 1.4 eV, Vjet ≈ 30–100 km/s, mean charge $\bar{Z}$ ≈ 1, sonic Mach number Ms ≡ Vjet/Cs > 10, jet diameter = 5 cm, and jet length ≈20 cm. Experiments to date have focused on the study of merging-jet dynamics and the shocks that form as a result of the interaction, in both collisional and collisionless regimes with respect to the inter-jet classical ion mean free path, and with and without an applied magnetic field. However, many other studies are also possible, as discussed in this paper.


2015 ◽  
Vol 91 (1) ◽  
Author(s):  
Peter Schrafel ◽  
Kate Bell ◽  
John Greenly ◽  
Charles Seyler ◽  
Bruce Kusse

2010 ◽  
Vol 81 (3) ◽  
Author(s):  
Michael A. Purvis ◽  
Jonathan Grava ◽  
Jorge Filevich ◽  
Duncan P. Ryan ◽  
Stephen J. Moon ◽  
...  

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