Evidence for anisotropic non-Maxwellian velocity distributions in the solar transition region
astro-ph.SR
Submitted: 2026-05-04
Updated: 2026-09-15
Comments: 9 pages, 5 figures, accepted for publication in ApJ Letters
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The Interface Region Imaging Spectrograph (IRIS)
- Why Is Non-thermal Line Broadening of Spectral Lines in The Lower Transition Region of the Sun Independent of Spatial Resolution?
- Non-Maxwellian analysis of the transition-region line profiles observed by the Interface Region Imaging Spectrograph
- RHESSI Microflare Statistics II. X-ray Imaging, Spectroscopy & Energy Distributions
- Accelerated electrons observed down to <7 keV in a NuSTAR solar microflare
- Evidence of Non-Thermal Particles in Coronal Loops Heated Impulsively by Nanoflares
- IRIS observations of short-term variability in moss associated with transient hot coronal loops
- A Statistical Study of IRIS Observational Signatures of Nanoflares and Non-thermal Particles
- High Resolution Observations of the Low Atmospheric Response to Small Coronal Heating Events in an Active Region Core
- Center-to-limb variations in coronal hole and quiet Sun regions obtained with IRIS spectroscopic observations
- Investigating the response of loop plasma to nanoflare heating using RADYN simulations
- HST/STIS High Resolution Echelle Spectra of alpha Centauri A (G2 V)
- Ultraviolet Spectroscopy of Rapidly-Rotating Solar-Mass Stars: Emission Line Redshifts as a Test of the Solar-Stellar Connection
- On the Nature of Nonthermal Broadening of Spectral Lines Observed by IRIS
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