We present the Tenerife Inversion Code (TIC), which has been developed to infer the magnetic and plasma properties of the solar chromosphere and transition region via full-Stokes inversion of polarized spectral lines. The code is based on the HanleRT forward engine, which takes into account many of the physical mechanisms that are critical for a proper modeling of the Stokes profiles of spectral lines originating in the tenuous and highly dynamic plasmas of the chromosphere and transition region: quantum level population imbalance and interference (atomic polarization), frequency coherence effects in polarized resonance scattering (partial frequency redistribution), and the impact of arbitrary magnetic fields on the atomic polarization and ...
Magnetic fields are responsible for a multitude of Solar phenomena, including such destructive event...
Abstract Since the early 1970s, inversion techniques have become the most useful tool for inferring ...
The long-standing paradox of the linear polarization signal of the Na i D1 line was recently resolve...
Inversion techniques (ITs) allow us to infer the magnetic, dynamic, and thermal properties of the so...
The Mg II h and k lines are among the strongest in the near-ultraviolet solar spectrum and their lin...
We investigate the diagnostic potential of the spectral lines at 850 nm for understanding the magnet...
Future ground-based telescopes, such as the 4-metre class facilities DKIST and EST, will dramaticall...
A major remaining challenge for heliophysics is to decipher the magnetic structure of the chromosphe...
This paper highlights very recent advances concerning the identification of new mechanisms that intr...
In order to obtain empirical information on the magnetism of the solar transition region we need to ...
Thomson scattered photospheric light is the dominant constituent of the lower solar corona's spectra...
Is it physically feasible to perform the chromospheric diagnosis using spatial maps of scattering po...
The new CRISP filter at the Swedish 1-m Solar Telescope provides opportunities for observing the sol...
Observational astrophysics started when spectroscopy could be applied to astronomy. Similarly, obser...
This paper identifies spectral lines from X-ray to infrared wavelengths which are optimally suited t...
Magnetic fields are responsible for a multitude of Solar phenomena, including such destructive event...
Abstract Since the early 1970s, inversion techniques have become the most useful tool for inferring ...
The long-standing paradox of the linear polarization signal of the Na i D1 line was recently resolve...
Inversion techniques (ITs) allow us to infer the magnetic, dynamic, and thermal properties of the so...
The Mg II h and k lines are among the strongest in the near-ultraviolet solar spectrum and their lin...
We investigate the diagnostic potential of the spectral lines at 850 nm for understanding the magnet...
Future ground-based telescopes, such as the 4-metre class facilities DKIST and EST, will dramaticall...
A major remaining challenge for heliophysics is to decipher the magnetic structure of the chromosphe...
This paper highlights very recent advances concerning the identification of new mechanisms that intr...
In order to obtain empirical information on the magnetism of the solar transition region we need to ...
Thomson scattered photospheric light is the dominant constituent of the lower solar corona's spectra...
Is it physically feasible to perform the chromospheric diagnosis using spatial maps of scattering po...
The new CRISP filter at the Swedish 1-m Solar Telescope provides opportunities for observing the sol...
Observational astrophysics started when spectroscopy could be applied to astronomy. Similarly, obser...
This paper identifies spectral lines from X-ray to infrared wavelengths which are optimally suited t...
Magnetic fields are responsible for a multitude of Solar phenomena, including such destructive event...
Abstract Since the early 1970s, inversion techniques have become the most useful tool for inferring ...
The long-standing paradox of the linear polarization signal of the Na i D1 line was recently resolve...