Accurate free—free Gaunt factors for astrophysical plasmas [PDF]
, 1998 Ralph S. Sutherland
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Level populations for Be-sequence ions in astrophysical plasmas [PDF]
, 1984 F. P. Keenan +4 more
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Relativistic Astrophysical Plasmas
Kakuyūgō kenkyū, 1989 Selected theoretical topics in high energy astrophysics are discussed. Firstly an account is given of accretion disks around a massive black hole and radiation processes in hot thermal plasmas. Then recent studies on the effects of electron-positron pairs in relativistic thermal plasmas are summarized.
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Wave Propagation in Anisotropic Magnetically Quantized Ion Plasma with Trapped Electron and Positron
East European Journal of PhysicsThis study examines the effects of magnetically quantized degenerate trapped electrons and positrons on small-amplitude ion acoustic shock waves (IAShWs) in a pair ion plasma using the Zakharov-Kuznetsov Burger (ZKB) equation.
Balaram Pradhan +2 more
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Dielectronic recombination rates in astrophysical plasmas [PDF]
, 2010 P. Quarati +3 more
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Investigating the Role of Inward Alfvén Waves and Structures in the Slow Solar Wind
The Astrophysical JournalThe solar wind dynamics are thought to be governed by counter-propagating Alfvén waves. Alfvén waves generate a turbulent cascade through nonlinear couplings between shearing wave packets. However, imbalances, structures, and intermittency complicate the
Michael Terres, Gang Li
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Lower-hybrid oscillations in a cold magnetized electron-positron-ion plasma
AIP Advances, 2018 In this paper, we obtain the dispersion relation for the lower-hybrid oscillations/waves in a cold magnetized electron-positron-ion (e-p-i) plasma. It is found that the frequency of the lower-hybrid oscillations in an e-p-i plasma is approximate 1/3 ...
Prabal Singh Verma
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Benchmarking calculations of excitation energies and transition properties with spectroscopic accuracy of highly charged ions used for the fusion plasma and astrophysical plasma [PDF]
, 2023 Chunyu Zhang +7 more
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The Astrophysical JournalWe report the first experimental detection of a reflected Alfvén wave from an Alfvén-speed gradient under conditions similar to those in coronal holes. The experiments were conducted in the Large Plasma Device at the University of California, Los Angeles.
Sayak Bose +8 more
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Atomic spectra and oscillator strengths for astrophysical and laboratory plasmas: ASOS-12 [PDF]
, 2017 B. Barbuy, P. Beiersdörfer, Tomas Brage
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