Search results for "Plasma density"

showing 2 items of 2 documents

The role of radiative losses in the late evolution of pulse-heated coronal loops/strands

2012

Radiative losses from optically thin plasma are an important ingredient for modeling plasma confined in the solar corona. Spectral models are continuously updated to include the emission from more spectral lines, with significant effects on radiative losses, especially around 1 MK. We investigate the effect of changing the radiative losses temperature dependence due to upgrading of spectral codes on predictions obtained from modeling plasma confined in the solar corona. The hydrodynamic simulation of a pulse-heated loop strand is revisited comparing results using an old and a recent radiative losses function. We find significant changes in the plasma evolution during the late phases of plas…

Physics010504 meteorology & atmospheric sciencesFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsCoronal loopPlasma01 natural sciencesSpectral lineComputational physicsPulse (physics)Cooling rateSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceSun: X-rays gamma rays Sun: corona Sun: UV radiation Sun: activity radiation mechanisms: thermal hydrodynamicsPhysics::Plasma Physics0103 physical sciencesPhysics::Space PhysicsRadiative transferX-rays gamma rays Sun: corona Sun: UV radiation Sun: activity radiation mechanisms: thermal hydrodynamics [Sun]010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPlasma density
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Fe Kα and Hydrodynamic Loop Model Diagnostics for a Large Flare on II Pegasi

2008

The observation by the Swift X-ray Telescope of the Fe K alpha_1, alpha_2 doublet during a large flare on the RS CVn binary system II Peg represents one of only two firm detections to date of photospheric Fe K alpha from a star other than our Sun. We present models of the Fe K alpha equivalent widths reported in the literature for the II Peg observations and show that they are most probably due to fluorescence following inner shell photoionisation of quasi-neutral Fe by the flare X-rays. Our models constrain the maximum height of flare the to 0.15 R_* assuming solar abundances for the photospheric material, and 0.1 R_* and 0.06 R_* assuming depleted photospheric abundances ([M/H]=-0.2 and […

PhysicsAstronomy and AstrophysicsAstrophysicslaw.inventionLuminosityLoop (topology)TelescopeSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary SciencelawPEG ratioK-alphaHydrodynamics Plasmas Stars: Coronae X-Rays: StarsBinary systemPlasma densityFlareThe Astrophysical Journal
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