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43 papers
A study of the capabilities for inferring atmospheric information from high-spatial-resolution simulations
C. Quintero Noda, E. Khomenko, M. Collados +8
In this work, we study the accuracy that can be achieved when inferring the atmospheric information from realistic numerical magneto-hydrodynamic simulations that reproduce the spa…
Observations of pores and surrounding regions with CO 4.66 μm lines by BBSO/CYRA
Yongliang Song, Xianyong Bai, Xu Yang +6
Solar observations of carbon monoxide (CO) indicate the existence of lower-temperature gas in the lower solar chromosphere. We present an observation of pores, and quiet-Sun, and n…
The Propagation of Coherent Waves Across Multiple Solar Magnetic Pores
S. D. T. Grant, D. B. Jess, M. Stangalini +9
Solar pores are efficient magnetic conduits for propagating magnetohydrodynamic wave energy into the outer regions of the solar atmosphere. Pore observations often contain isolated…
Evaluating Non-LTE Spectral Inversions with ALMA and IBIS
Ryan Hofmann, Kevin Reardon, Ivan Milic +3
We present observations of a solar plage in the millimeter-continuum with the ALMA and in the Ca 8542 and Na 5896 spectral lines with the Interferometric BIdimensional Spectrometer…
DeSIRe: Departure coefficient aided Stokes Inversion based on Response functions
B. Ruiz Cobo, C. Quintero Noda, R. Gafeira +3
Future ground-based telescopes, such as the 4-metre class facilities DKIST and EST, will dramatically improve on current capabilities for simultaneous multi-line polarimetric obser…
The Atmospheric Response to High Nonthermal Electron Beam Fluxes in Solar Flares. II. Hydrogen Broadening Predictions for Solar Flare Observations with the Daniel K. Inouye Solar Telescope
Adam F. Kowalski, Joel C. Allred, Mats Carlsson +5
Red-shifted components of chromospheric emission lines in the hard X-ray impulsive phase of solar flares have recently been studied through their 30 s evolution with the high resol…