Non-local thermodynamic equilibrium inversions from a 3D magnetohydrodynamic chromospheric model
Open Access
- 22 June 2012
- journal article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 543, A34
- https://doi.org/10.1051/0004-6361/201218825
Abstract
No abstract availableThis publication has 24 references indexed in Scilit:
- SCATTERING POLARIZATION IN THE Ca II INFRARED TRIPLET WITH VELOCITY GRADIENTSThe Astrophysical Journal, 2012
- THE FORMATION OF THE Hα LINE IN THE SOLAR CHROMOSPHEREThe Astrophysical Journal, 2012
- MODEL SELECTION FOR SPECTROPOLARIMETRIC INVERSIONSThe Astrophysical Journal, 2012
- A high-resolution three-dimensional model of the solar photosphere derived from Hinode observationsAstronomy & Astrophysics, 2011
- Non-equilibrium calcium ionisation in the solar atmosphereAstronomy & Astrophysics, 2011
- The solar chromosphere at high resolution with IBISAstronomy & Astrophysics, 2009
- Spectropolarimetric Inversions of the Caii8498 and 8542 A Lines in the Quiet SunThe Astrophysical Journal, 2007
- Simulation of Quiet‐Sun Waves in the CaiiInfrared TripletThe Astrophysical Journal, 2006
- An Hermitian Method for the Solution of Polarized Radiative Transfer ProblemsThe Astrophysical Journal, 1998
- Linearization versus Preconditioning: Which Approach Is Best for Solving Multilevel Transfer Problems?The Astrophysical Journal, 1997