Inference of physical parameters in solar prominence threads
We consider magnetohydrodynamics models and observations of transverse oscillations in prominence threads to obtain information on their physical properties...
Inference of Solar Vector Magnetic Fields with Filtergraph Instruments
We investigate the diagnostic potential of polarimetric measurements with filtergraph instruments. Numerical simulations are used to explore the possibility of...
Inferring Plasma Flows In The Solar Photosphere & Chromosphere Using Deep Learning And Surface Observations
Direct measurements of plasma motions are limited to the line-of-sight component at the Sun's surface. Multiple tracking and inversion methods were developed to...
Inferring stellar population properties from HST+JWST photometry using Normalizing Flows
Spectral energy distributions (SEDs) encode information about the stellar populations within galaxies. By investigating the properties of these stars, such as...
Influence of Coronal EUV Irradiance on the Stokes Profiles of the He I 10830 Å Multiplet
One of the most useful spectral windows for spectropolarimetric investigations of the solar chromosphere is the one provided by the spectral lines of the He I...
Influence of longitudinal structure in the fast modes of prominence threads
Recent high-resolution observations have pointed out that prominences are made of small threads (also named fibrils) piled up to form the body of the prominence...
Influence of the Paschen-Back effect on the results of polarimetric inversions of the He I 10830 Å triplet
The He I triplet at 10830 Å has a great potential for determining the magnetic field vector in the upper chromosphere. The triplet is Zeeman sensitive (Landé...