Astrophysical: Radiative transfer

  • Talk
    Physical properties of asteroid surfaces 1: Introduction to asteroid UV-VIS-NIR spectrometry
    Series: XXVIII Canary Islands Winter School of Astrophysics: Solar System Exploration Topic: Physical Properties of Asteroid Surfaces Lecture 1: Introduction to...
  • Talk
    Physical properties of asteroid surfaces 2: Novel spectrometric modeling
    Series: XXVIII Canary Islands Winter School of Astrophysics: Solar System Exploration Topic: Physical Properties of Asteroid Surfaces Lecture 2: Novel...
  • Publication
    Physical Properties of the Solar Magnetic Photosphere under the MISMA Hypothesis. I. Description of the Inversion Procedure
    The paper describes an automatic inversion code to recover microstructured magnetic atmospheres (MISMAs) by fitting Stokes profiles. These solar model...
  • Publication
    Physical Properties of the Solar Magnetic Photosphere under the MISMA Hypothesis. II. Network and Internetwork Fields at the Disk Center
    This paper is the second in a series that models photospheric magnetic structures in terms of atmospheres having optically thin fluctuations of magnetic field...
  • Talk
    Planetary Atmospheres 2: Radiative Transfer, Composition, and Clouds
    Series: XXVIII Canary Islands Winter School of Astrophysics: Solar System Exploration Topic: Planetary Atmospheres. Lecture 2: Radiative transfer, composition...
  • Publication
    Polarized resonance line transfer in a spherically symmetric medium with angle-dependent partial frequency redistribution
    In a stellar atmosphere, the resonance line polarization arises from scattering of limb-darkened radiation field by atoms. This spectral line polarization gets...
  • Publication
    PORTA: A three-dimensional multilevel radiative transfer code for modeling the intensity and polarization of spectral lines with massively parallel computers
    The interpretation of the intensity and polarization of the spectral line radiation produced in the atmosphere of the Sun and of other stars requires solving a...
  • Publication
    Probing 3D and NLTE models using APOGEE observations of globular cluster stars
    Context. Hydrodynamical (or 3D) and non-local thermodynamic equilibrium (NLTE) effects are known to affect abundance analyses. However, there are very few...
  • Publication
    Probing downflows in solar magnetic elements: the Fe II test
    In an attempt to assess the physical realism of the plage flux tube model derived by Bellot Rubio, Ruiz Cobo & Collados (cite{brc}, cite{bellot}) we extend its...