On the importance of Ca II photoionisation by the hydrogen Lyman transitions in solar flare models

Osborne, C.M.J., Heinzel, P., Kasparova, J. and Fletcher, L. (2021) On the importance of Ca II photoionisation by the hydrogen Lyman transitions in solar flare models. Monthly Notices of the Royal Astronomical Society, 507(2), pp. 1972-1978. (doi: 10.1093/mnras/stab2156)

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Abstract

The forward fitting of solar flare observations with radiation-hydrodynamic simulations is a common technique for learning about energy deposition and atmospheric evolution during these explosive events. A frequent spectral line choice for this process is Ca ii 854.2 nm due to its formation in the chromosphere and substantial variability. It is important to ensure that this line is accurately modeled to obtain the correct interpretation of observations. Here we investigate the importance of photoionisation of Ca ii to Ca iii by the hydrogen Lyman transitions; whilst the Lyman continuum is typically considered in this context in simulations, the associated bound-bound transitions are not. This investigation uses two RADYN flare simulations and reprocesses the radiative transfer using the Lightweaver framework which accounts for the overlapping of all active transitions. The Ca ii 854.2 nm line profiles are found to vary significantly due to photoionisation by the Lyman lines, showing notably different shapes and even reversed asymmetries. Finally, we investigate to what extent these effects modify the energy balance of the simulation and the implications on future radiation-hydrodynamic simulations. There is found to be a 10-15 per cent change in detailed optically thick radiative losses from considering these photoionisation effects on the calcium lines in the two simulations presented, demonstrating the importance of considering these effects in a self-consistent way.

Item Type:Articles
Additional Information:C.M.J.O. acknowledges support from the UK Research and Innovation’s Science and Technology Facilities Council (STFC) doctoral training grant ST/R504750/1. P.H. and J.K. were supported by grant 19-09489S (GACR) and project RVO:67985815. L.F. acknowledges support from UK Research and Innovation’s Science and Technology Facilities Council under grant award number ST/T000422/1.
Status:Published
Refereed:Yes
Glasgow Author(s) Enlighten ID:Fletcher, Professor Lyndsay and Osborne, Chris and Kasparova, Dr Jana
Authors: Osborne, C.M.J., Heinzel, P., Kasparova, J., and Fletcher, L.
College/School:College of Science and Engineering > School of Physics and Astronomy
Journal Name:Monthly Notices of the Royal Astronomical Society
Publisher:Oxford University Press
ISSN:0035-8711
ISSN (Online):1365-2966
Published Online:29 July 2021
Copyright Holders:Copyright © 2021 The Authors
First Published:First published in Monthly Notices of the Royal Astronomical Society 507(2): 1972-1978
Publisher Policy:Reproduced under a Creative Commons License
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Project CodeAward NoProject NamePrincipal InvestigatorFunder's NameFunder RefLead Dept
301388STFC Glasgow 2017 DTPMartin HendryScience and Technology Facilities Council (STFC)ST/R504750/1P&S - Physics & Astronomy
306515PHAS A&A Group STFC ConsolidatedLyndsay FletcherScience and Technology Facilities Council (STFC)ST/T000422/1P&S - Physics & Astronomy