0000000000389859

AUTHOR

Tiago M. D. Pereira

showing 1 related works from this author

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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