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101
Application of radiative fluid dynamics scaled from the laboratory to astrophysics
Published 2015Thesis -
102
Scalable Codes for Precision Calculations of Properties of Complex Atomic Systems
Published 2021-04-01“…High precision atomic data are indispensable for studies of fundamental symmetries, tests of fundamental physics postulates, developments of atomic clocks, ultracold atom experiments, astrophysics, plasma science, and many other fields of research. …”
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103
Simulations of the small-scale turbulent dynamo
Published 2004“…The primary focus is on the case of large magnetic Prandtl numbers Prm, which is relevant for hot low-density astrophysical plasmas. A Prm parameter scan is given for the model case of viscosity-dominated (low Reynolds number) turbulence. …”
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104
Astrophysical gyrokinetics: turbulence in pressure-anisotropic plasmas at ion scales and beyond
Published 2018“…Our theory provides a foundation for determining how pressure anisotropy affects turbulent fluctuation spectra, the differential heating of particle species and the ratio of parallel and perpendicular phase mixing in space and astrophysical plasmas.…”
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105
Relativistic Collisionless Shocks in Inhomogeneous Magnetized Plasmas
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106
Pitch-angle Anisotropy Imprinted by Relativistic Magnetic Reconnection
Published 2023-01-01Get full text
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107
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108
An Exactly Energy-conserving Electromagnetic Particle-in-cell Method in Curvilinear Coordinates
Published 2024-01-01Get full text
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109
Dynamic Formation of a Transient Jet from Arched Magnetized Laboratory Plasma
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110
Database NORAD-Atomic-Data for Atomic Processes in Plasma
Published 2020-10-01“…It contains large sets of parameters for the dominant atomic processes in astrophysical plasmas, such as, (i) photo-excitation, (ii) photoionization, (iii) electron–ion recombination, (iv) electron–impact excitations. …”
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111
Global Electron Thermodynamics in Radiatively Inefficient Accretion Flows
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112
Studying astrophysical collisionless shocks with counterstreaming plasmas from high power lasers
Published 2012“…Because of the low density of astrophysical plasmas, the mean free path due to Coulomb collisions is typically very large. …”
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113
SPECTROSCOPIC DIAGNOSIS IN ELECTRONIC TEMPERATURE OF PHOTOIONISE PLASMAS
Published 2015-08-01“…These lines appear clearly in the spectra of astrophysical plasmas. As helium-like ion, we chose two, the oxygen O<sup>6+</sup> (Z=8) and neon Ne<sup>8+ </sup>(Z=10). …”
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114
Estimating intermittency significance by means of surrogate data: implications for solar wind turbulence
Published 2023-06-01“…Introduction: Intermittency is a property of turbulent astrophysical plasmas, such as the solar wind, that implies irregularity and fragmentation, leading to non-uniformity in the transfer rate of energy carried by nonlinear structures from large to small scales. …”
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115
The Origin of Persistently Nonthermal Solar Wind Electrons: the Steady Electron Runaway Model's Demonstration of Dreicer Bifurcation using Measured and Ion–Electron Coulomb Drag
Published 2023-01-01“…This documentation quantitatively establishes Coulomb runaway physics as the missing determinant of the ubiquitous nonthermal solar wind eVDF. Astrophysical plasmas, like stellar winds, are unavoidably inhomogeneous, requiring ${{\mathbb{E}}}_{\parallel }$ to enforce quasi-neutrality. …”
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116
Production of energetic protons, deuterons, and neutrons up to 60 MeV via disruption of a current-carrying plasma column at 3 MA
Published 2020-01-01“…Acceleration of ions to multi-MeV energies is investigated in various plasma devices to better understand processes in astrophysical plasmas and to develop efficient accelerators for a variety of applications. …”
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117
Isochoric generation and spectroscopic diagnosis of high energy-density systems
Published 2020“…</p> <p>This thesis describes a set of experiments to isochorically generate and characterise WDM and HED systems relevant to astrophysical plasmas and Inertial Confinement Fusion. The focus of this work is on using measured X-ray Emission Spectroscopy or Resonant Inelastic X-ray Scattering (RIXS) spectra to bound the conditions present in the laser target, and using Single Photon Counting informed techniques to maximise the signal/noise in recovered spectra. …”
Thesis -
118
Time-dependent Photoionization Modeling of Warm Absorbers in Active Galactic Nuclei
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119
Electron Heating by Magnetic Pumping and Whistler-mode Waves
Published 2024-01-01Get full text
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120
A New Covariant Formalism for Kinetic Plasma Simulations in Curved Spacetimes
Published 2023-01-01Get full text
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