Context. Halo bias links the statistical properties of the spatial distribution of dark matter (DM) halos to those of the underlying DM field, providing...
Inelastic e+Mg collision data and its impact on modelling stellar and supernova spectra
Results of calculations for inelastic e+Mg effective collision strengths for the lowest 25 physical states of Mg i (up to 3s6p1P), and thus 300 transitions...
Inference of electric currents in the solar photosphere
Context. Despite their importance, routine and direct measurements of electric currents, j, in the solar atmosphere have generally not been possible. Aims: We...
Inference of magnetic field strength and density from damped transverse coronal waves
A classic application of coronal seismology uses transverse oscillations of waveguides to obtain estimates of the magnetic field strength. The procedure...
Inference of Solar Magnetic Field Parameters from Data with Limited Wavelength Sampling
We investigate the diagnostic potential of polarimetric measurements with filtergraph instruments. Numerical simulations are used to explore the possibility of...
Inference of the chromospheric magnetic field orientation in the Ca ii 8542 Å line fibrils
Context. Solar chromospheric fibrils, as observed in the core of strong chromospheric spectral lines, extend from photospheric field concentrations suggesting...