HanleRT-TIC
HanleRT-TIC is a numerical code for solving the problem of the generation and transfer of polarized radiation in one-dimensional (1D and 1.5D) model atmospheres for realistic atomic models. HanleRT-TIC also allows for the solution of the inversion problem with its Tenerife Inversion Code (TIC) module. The code can take into account atomic and scattering polarization, quantum interference among energy levels pertaining to a given atomic term, partial frequency redistribution effects due to the photon coherence in scattering processes, the impact of dynamics, and the impact of magnetic fields via the joint action of the Hanle and Zeeman effects (incomplete Paschen-Back regime).
References
- del Pino Alemán, T., Casini, R., Manso Sainz, R. (2016), Magnetic Diagnostics of the Solar Chromosphere with the Mg II h-k Lines, The Astrophysical Journal, 830, L24
- del Pino Alemán, T., Trujillo Bueno, J., Casini, R., Manso Sainz, R. (2020), The Magnetic Sensitivity of the Resonance and Subordinate Lines of Mg II in the Solar Chromosphere, The Astrophysical Journal, 891, 91
- Li, H., del Pino Alemán, T., Trujillo Bueno, J., Casini, R. (2022), TIC: A Stokes inversion code for scattering polarization with partial frequency redistribution and arbitrary magnetic fields, The Astrophysical Journal, 933, 145
Download
The code is freely available to the community, hosted at GitLab. The latest version of HanleRT-TIC can be found at https://gitlab.com/TdPA/hanlert-tic, and the latest version of the documentation at https://tdpa.gitlab.io/hanlert-tic/.