output
20012026
most citedChandra HETGS Multi-Phase Spectroscopy of the Young Magnetic O Star theta^1 Orionis C

200 citations

13 papers

physics.plasm-ph2026

X-ray spectroscopy of hot dense plasmas using LLNL's upgraded Titan 2 short-pulse laser

A. J. Fairchild, D. T. Bishel, T. Cordova +10

We are developing an experimental platform at Lawrence Livermore National Laboratory's Jupiter Laser Facility to characterize X-ray emission from highly charged ions in the high-de…

physics.plasm-ph2021★ 20 cited

A feasibility study of using X-ray Thomson Scattering to diagnose the in-flight plasma conditions of DT cryogenic implosions

H. Poole, D. Cao, R. Epstein +9

The design of inertial confinement fusion (ICF) ignition targets requires radiation-hydrodynamics simulations with accurate models of the fundamental material properties (i.e., equ…

physics.atom-ph2016★ 24 cited

Comment on "Large enhancement in high-energy photoionization of Fe XVII and missing continuum plasma opacity"

C. Blancard, J. Colgan, Ph. Cossé +12

Recent R-matrix calculations claim to produce a significant enhancement in the opacity of Fe XVII due to atomic core excitations [S. N. Nahar & A.K. Pradhan, Phys. Rev. Letters 116…

astro-ph.SR2014★ 31 cited

Control and diagnosis of temperature, density, and uniformity in x-ray heated iron/magnesium samples for opacity measurements

T. Nagayama, J. E. Bailey, G. Loisel +5

Experimental tests are in progress to evaluate the accuracy of the modeled iron opacity at solar interior conditions, in particular to better constrain the solar abundance problem…

physics.plasm-ph2012★ 20 cited

One-dimensional radiation-hydrodynamic simulations of imploding spherical plasma liners with detailed equation-of-state modeling

J. S. Davis, S. C. Hsu, I. E. Golovkin +2

This work extends the one-dimensional radiation-hydrodynamic imploding spherical argon plasma liner simulations of T. J. Awe et al. [Phys. Plasmas 18, 072705 (2011)] by using a det…

astro-ph2006★ 58 cited

Wind signatures in the X-ray emission line profiles of the late O supergiant Orionis

David H. Cohen, Maurice A. Leutenegger, Kevin T. Grizzard +3

X-ray line profile analysis has proved to be the most direct diagnostic of the kinematics and spatial distribution of the very hot plasma around O stars. In this paper we apply sev…