Search results for "Sun: transition region"

showing 3 items of 3 documents

Investigating the Response of Loop Plasma to Nanoflare Heating Using RADYN Simulations

2018

We present the results of 1D hydrodynamic simulations of coronal loops that are subject to nanoflares, caused by either in situ thermal heating or nonthermal electron (NTE) beams. The synthesized intensity and Doppler shifts can be directly compared with Interface Region Imaging Spectrograph (IRIS) and Atmospheric Imaging Assembly (AIA) observations of rapid variability in the transition region (TR) of coronal loops, associated with transient coronal heating. We find that NTEs with high enough low-energy cutoff (EC) deposit energy in the lower TR and chromosphere, causing blueshifts (up to approximately 20 kilometers per second) in the IRIS Si IV lines, which thermal conduction cannot repro…

Electron density010504 meteorology & atmospheric sciencesFOS: Physical sciencesAstrophysicsElectron01 natural sciencesSun: activity0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsSun: transition region010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSun: coronaAstronomy and AstrophysicsPlasmaCoronal loopAstronomy and AstrophysicThermal conductionNanoflaresIntensity (physics)Astrophysics - Solar and Stellar Astrophysicsline: profileSpace and Planetary SciencePhysics::Space PhysicsThe Astrophysical Journal
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MHD modeling of coronal loops: the transition region throat

2014

The expansion of coronal loops in the transition region may considerably influence the diagnostics of the plasma emission measure. The cross sectional area of the loops is expected to depend on the temperature and pressure, and might be sensitive to the heating rate. The approach here is to study the area response to slow changes in the coronal heating rate, and check the current interpretation in terms of steady heating models. We study the area response with a time-dependent 2D MHD loop model, including the description of the expanding magnetic field, coronal heating and losses by thermal conduction and radiation from optically thin plasma. We run a simulation for a loop 50 Mm long and qu…

PhysicsMagnetohydrodynamics (MHD)Sun: coronaMagnetohydrodynamics (MHD); Sun: corona; Sun: magnetic fields; Sun: transition region; Astronomy and Astrophysics; Space and Planetary ScienceFOS: Physical sciencesAstronomy and AstrophysicsPlasmaAstrophysicsMechanicsCoronal loopRadiationThermal conductionMagnetic fieldLoop (topology)corona Sun: magnetic fields Sun: transition region magnetohydrodynamics (MHD) [Sun]Settore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceSun: corona Sun: magnetic fields Sun: transition region magnetohydrodynamics (MHD)MagnetohydrodynamicsCurrent (fluid)Sun: transition regionSun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)
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A fast multi-dimensional magnetohydrodynamic formulation of the transition region adaptive conduction (TRAC) method

2021

We have demonstrated that the Transition Region Adaptive Conduction (TRAC) method permits fast and accurate numerical solutions of the field-aligned hydrodynamic equations, successfully removing the influence of numerical resolution on the coronal density response to impulsive heating. This is achieved by adjusting the parallel thermal conductivity, radiative loss, and heating rates to broaden the transition region (TR), below a global cutoff temperature, so that the steep gradients are spatially resolved even when using coarse numerical grids. Implementing the original 1D formulation of TRAC in multi-dimensional magnetohydrodynamic (MHD) models would require tracing a large number of magne…

Sun: flaresMagnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencescorona [Sun]Field lineNDASFOS: Physical scienceschromosphere [Sun]Astrophysics01 natural sciencestransition region [Sun]0103 physical sciencesRadiative transferQB AstronomyMagnetohydrodynamic driveflares hydrodynamics [Sun]Sun: transition region010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QC0105 earth and related environmental sciencescomputer.programming_languageQBPhysicsSun: coronaSun: chromosphereAstronomy and AstrophysicsTRACCoronal loopThermal conductionComputational physicsMagnetic fieldQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceHydrodynamicsMagnetohydrodynamicscomputerSettore FIS/06 - Fisica Per Il Sistema Terra E Il Mezzo Circumterrestre
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