Atomic Scattering Polarization. Observations, Modeling, Predictions

Bibcode
2015IAUS..305..127B
DOI
10.1017/S1743921315004652
Trujillo Bueno, J.; Del Pino Alemán, T.; Belluzzi, L.
Bibliographical reference

Proceedings of the International Astronomical Union, Volume 305, pp. 127-135

Advertised on:
10
2015
Number of authors
3
IAC number of authors
2
Citations
0
Refereed citations
0
Description
This paper highlights very recent advances concerning the identification of new mechanisms that introduce polarization in spectral lines, which turn out to be key for understanding some of the most enigmatic scattering polarization signals of the solar visible spectrum. We also show a radiative transfer prediction on the scattering polarization pattern across the Mg ii h & k lines, whose radiation can only be observed from space.
Related projects
Project Image
Magnetism, Polarization and Radiative Transfer in Astrophysics

Magnetic fields pervade all astrophysical plasmas and govern most of the variability in the Universe at intermediate time scales. They are present in stars across the whole Hertzsprung-Russell diagram, in galaxies, and even perhaps in the intergalactic medium. Polarized light provides the most reliable source of information at our disposal for the

Tanausú del
Pino Alemán
In progress
Type
Non-refereed
Radiative transfer
Magnetic fields
Solar Physics (FS)

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