An Iterative OLA Method for Inversion of Solar Spectropolarimetric Data. I. Single- and Multiple-variable Inversions of Thermodynamic Quantities

This paper describes an adaptation of the Optimally Localized Averaging (OLA) inversion technique, originally developed for geo- and helioseismological applications, to the interpretation of solar spectroscopic data. It focuses on inverting the thermodynamical properties of the solar atmosphere, ass...

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Main Authors: Piyush Agrawal, Mark P. Rast, Basilio Ruiz Cobo
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/aca536
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author Piyush Agrawal
Mark P. Rast
Basilio Ruiz Cobo
author_facet Piyush Agrawal
Mark P. Rast
Basilio Ruiz Cobo
author_sort Piyush Agrawal
collection DOAJ
description This paper describes an adaptation of the Optimally Localized Averaging (OLA) inversion technique, originally developed for geo- and helioseismological applications, to the interpretation of solar spectroscopic data. It focuses on inverting the thermodynamical properties of the solar atmosphere, assuming that the atmosphere and radiation field are in local thermodynamic equilibrium (LTE). We leave inversions of magnetic field and non-LTE inversions for future work. The advantage with the OLA method is that it computes solutions that are optimally depth resolved with minimal crosstalk error between variables. Additionally, the method allows for direct assessment of the vertical resolution of the inverted solutions. The primary challenges faced when adapting the method to spectroscopic inversions originate with the possible large-amplitude differences between the atmospheric model used to initiate the inversion and the underlying atmosphere it aims to recover, necessitating the development of an iterative scheme. Here, we describe the iterative OLA method we have developed for both single and multivariable inversions and demonstrate its performance on simulated data and synthesized spectra. We note that, when carrying out multivariable inversions, employing response function amplification factors can address the inherent spectral sensitivity bias that makes it hard to invert for less spectrally sensitive variables. The OLA method can, in most cases, reliably invert as well as or better than the frequently employed Stokes Inversion based on Response functions (SIR) scheme, but some difficulties remain. In particular, the method struggles to recover large-scale offsets in the atmospheric stratification. We propose future strategies to improve this aspect.
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spelling doaj.art-7bba354b19724b0997cd7753d37741f72023-09-03T09:58:12ZengIOP PublishingThe Astrophysical Journal1538-43572023-01-01944111110.3847/1538-4357/aca536An Iterative OLA Method for Inversion of Solar Spectropolarimetric Data. I. Single- and Multiple-variable Inversions of Thermodynamic QuantitiesPiyush Agrawal0https://orcid.org/0000-0001-6514-8944Mark P. Rast1https://orcid.org/0000-0002-9232-9078Basilio Ruiz Cobo2https://orcid.org/0000-0001-9550-6749Department of Astrophysical and Planetary Sciences, University of Colorado , Boulder, CO, USA ; piyush.agrawal@colorado.edu; Laboratory for Atmospheric and Space Physics, University of Colorado , Boulder, CO, USA ; mark.rast@lasp.colorado.edu; Southwest Research Institute , Boulder, CO 80302, USADepartment of Astrophysical and Planetary Sciences, University of Colorado , Boulder, CO, USA ; piyush.agrawal@colorado.edu; Laboratory for Atmospheric and Space Physics, University of Colorado , Boulder, CO, USA ; mark.rast@lasp.colorado.eduInstituto de Astrofisica de Canarias , La Laguna, Tenerife, E-38200, Spain ; basilio.ruiz@iac.es; Departamento de Astrofísica, Univ. de La Laguna , La Laguna, Tenerife, E-38205, SpainThis paper describes an adaptation of the Optimally Localized Averaging (OLA) inversion technique, originally developed for geo- and helioseismological applications, to the interpretation of solar spectroscopic data. It focuses on inverting the thermodynamical properties of the solar atmosphere, assuming that the atmosphere and radiation field are in local thermodynamic equilibrium (LTE). We leave inversions of magnetic field and non-LTE inversions for future work. The advantage with the OLA method is that it computes solutions that are optimally depth resolved with minimal crosstalk error between variables. Additionally, the method allows for direct assessment of the vertical resolution of the inverted solutions. The primary challenges faced when adapting the method to spectroscopic inversions originate with the possible large-amplitude differences between the atmospheric model used to initiate the inversion and the underlying atmosphere it aims to recover, necessitating the development of an iterative scheme. Here, we describe the iterative OLA method we have developed for both single and multivariable inversions and demonstrate its performance on simulated data and synthesized spectra. We note that, when carrying out multivariable inversions, employing response function amplification factors can address the inherent spectral sensitivity bias that makes it hard to invert for less spectrally sensitive variables. The OLA method can, in most cases, reliably invert as well as or better than the frequently employed Stokes Inversion based on Response functions (SIR) scheme, but some difficulties remain. In particular, the method struggles to recover large-scale offsets in the atmospheric stratification. We propose future strategies to improve this aspect.https://doi.org/10.3847/1538-4357/aca536Radiative transferSpectropolarimetryHelioseismologySolar physics
spellingShingle Piyush Agrawal
Mark P. Rast
Basilio Ruiz Cobo
An Iterative OLA Method for Inversion of Solar Spectropolarimetric Data. I. Single- and Multiple-variable Inversions of Thermodynamic Quantities
The Astrophysical Journal
Radiative transfer
Spectropolarimetry
Helioseismology
Solar physics
title An Iterative OLA Method for Inversion of Solar Spectropolarimetric Data. I. Single- and Multiple-variable Inversions of Thermodynamic Quantities
title_full An Iterative OLA Method for Inversion of Solar Spectropolarimetric Data. I. Single- and Multiple-variable Inversions of Thermodynamic Quantities
title_fullStr An Iterative OLA Method for Inversion of Solar Spectropolarimetric Data. I. Single- and Multiple-variable Inversions of Thermodynamic Quantities
title_full_unstemmed An Iterative OLA Method for Inversion of Solar Spectropolarimetric Data. I. Single- and Multiple-variable Inversions of Thermodynamic Quantities
title_short An Iterative OLA Method for Inversion of Solar Spectropolarimetric Data. I. Single- and Multiple-variable Inversions of Thermodynamic Quantities
title_sort iterative ola method for inversion of solar spectropolarimetric data i single and multiple variable inversions of thermodynamic quantities
topic Radiative transfer
Spectropolarimetry
Helioseismology
Solar physics
url https://doi.org/10.3847/1538-4357/aca536
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