Results 101 to 110 of about 1,535,639 (228)
Modeling multiphase plasma in the corona: prominences and rain
Living Reviews in Solar PhysicsWe review major achievements in our understanding of multiphase coronal plasma, where cool-dense and hot-tenuous matter coexists, brought about by advances in modeling and theory, inspired by observations.
Rony Keppens, Yuhao Zhou, Chun Xia
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Ultra-high charge electron acceleration for nuclear applications
Fundamental Plasma PhysicsUltra-intense laser-plasma wakefield accelerator possess several superior properties compared with the traditional radio-frequency accelerators. These characteristics include femtosecond duration, micro-source size, and ultra-dense beam density, result ...
Liming Chen +8 more
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Dynamics, thermodynamics, and fine structure of virtual erupting filaments
Astronomy & AstrophysicsContext. It is not fully understood why some solar filaments erupt, whereas others do not. Filaments that erupt typically undergo a slow rise, followed by an acceleration phase; this transition requires further investigation.
Donné D. +3 more
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Free–Free Gaunt Factors for Atmospheres of Accreting Pulsars Observable with X-Ray Space Missions
The Astrophysical JournalFree–free Gaunt factors for X-ray absorption by hot plasma in the presence of a strong magnetic field are reported. Modified formulae are used for application to the nonlocal thermodynamic equilibrium conditions found in accreting pulsar atmospheres ...
Parisee S. Shirke
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Center for Astrophysics Colloquia, 1999
, 2018 Public lectures given at the Harvard-Smithsonian Center for Astrophysics as part of their CfA Colloquium series. Originally recorded on videotape and audio cassette in 1999 and converted to digital files by EverPresent in 2017.
Harvard-Smithsonian Center for Astrophysics (5986331) +1 more
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Whistler–Alfvén Turbulence in a Nonneutral Ultrarelativistic Pair Plasma
The Astrophysical JournalThe large-scale dynamics of most conventional space and astrophysical plasmas are predominantly governed by Alfvén modes, which are low-frequency magnetohydrodynamic modes existing in magnetized media.
Stanislav Boldyrev, Mikhail Medvedev
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The usage of numerical code FLASH in plasma astrophysics
, 2013 My diploma thesis is focused on the use of numerical computer codes for simulation in plasma astrophysics. They will learn the basic characteristics of the Sun, a closer focus on the solar corona and the solar corona heating problem.
BROŽ, Jaroslav
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The Astrophysical JournalA forefront research question is how energy evolves in weakly collisional plasmas for which departures from local thermodynamic equilibrium (LTE) are significant.
M. Hasan Barbhuiya +9 more
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ISRN Astronomy and Astrophysics
, 2011 SRN Astronomy and Astrophysics is a peer-reviewed, open access journal that publishes original research articles as well as review articles in all areas of astronomy and ...
CAPUZZO DOLCETTA, Roberto Angelo
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Gamma Ray Astrophysics with CTA: Introduction to the School [PDF]
, 2017 Gamma Ray Astrophysics with CTA ...
VERCELLONE, STEFANO
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