Towards the Modelling of the Second Solar Spectrum

dc.creatorBueno, J. Trujillo
dc.date2007-10-29
dc.date.accessioned2026-07-07T08:39:13Z
dc.date.available2026-07-07T08:39:13Z
dc.descriptionThis paper addresses the modelling issue of the linearly-polarized solar limb spectrum, which is due to scattering processes and it offers a rich diagnostic potential for exploring solar magnetic fields via the Hanle effect. However, this so-called second solar spectrum is full of mysterious spectral features, which cannot be understood with simplified polarization transfer theories, thus suggesting that the underlying scattering physics is more complex than previously thought. In this paper we argue that the physical understanding of the second solar spectrum requires the consideration of scattering processes in multilevel atomic models, taking fully into account the transfer of atomic polarization among all the levels involved. The consideration of lower-level atomic polarization leads to non-linear and non-local coupled sets of equations, even for the two-level model atom case considered in this paper. The unknowns of the problem are the irreducible tensor components of the atomic density matrix whose self-consistent values have first to be obtained to be able to calculate the emergent Stokes profiles. To solve numerically this non-LTE problem of the second kind we present some iterative methods that are very suitable for developing a general multilevel scattering polarization code. We demonstrate that there exists metastable-level atomic polarization in the solar chromosphere, which suggests that the solution to some recently-formulated "paradoxes" is to be found by carefully revising our current ideas about the chromospheric magnetic field.
dc.description24 pages, 6 figures
dc.identifierhttps://arxiv.org/abs/0710.5421
dc.identifierhttp://arxiv.org/abs/0710.5421
dc.identifierPublished in 1999 in the book Solar Polarization, edited by K.N. Nagendra and J.O. Stenflo. Kluwer Academic Publishers, 1999. (Astrophysics and Space Science Library ; Vol. 243), p. 73-96
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/140995
dc.subjectAstrophysics
dc.titleTowards the Modelling of the Second Solar Spectrum
dc.typetext

Files

Collections