Publication type: Refereed

  • Publication
    Induced Massive Star Formation in the Trifid Nebula?
    Not Available
  • Publication
    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...
  • Publication
    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...
  • Publication
    Inference of horizontal velocity fields from the induction equation in the solar atmosphere: I. Analytical and numerical solutions in 2D
    Context. Spectroscopic and spectropolarimetric observations, which rely on the Doppler effect, only provide access to the line-of-sight component of the solar...
  • Publication
    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...
  • Publication
    Inference of magnetic fields in the very quiet Sun
    Context. Over the past 20 yr, the quietest areas of the solar surface have revealed a weak but extremely dynamic magnetism occurring at small scales (
  • Publication
    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...
  • Publication
    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...
  • Publication
    Inferring chromospheric velocities in an M3.2 flare using He I 1083.0 nm and Ca II 854.2 nm
    Aims. Our aim was to study the chromospheric line-of-sight (LOS) velocities during the GOES M3.2 flare (SOL2013-05-17T08:43) using simultaneous high-resolution...