IPOPv2 online service for the generation of opacity tables
arXiv:1511.07260 · doi:10.1016/j.jqsrt.2015.11.010
Abstract
In the framework of the present phase -- IPOPv2 -- of the international Opacity Project (OP), a new web service has been implemented based on the latest release of the OP opacities. The user may construct online opacity tables to be conveniently included in stellar evolution codes in the format most commonly adopted by stellar physicists, namely the OPAL format. This facility encourages the use and comparison of both the OPAL and OP data sets in applications. The present service allows for the calculation of multi-element mixtures containing the 17 species (H, He, C, N, O, Ne, Na, Mg, Al, Si, S, Ar, Ca, Cr, Mn, Fe and Ni) considered by the OP, and underpins the latest release of OP opacities. This new service provides tables of Rosseland mean opacites using OP atomic data. We provide an alternative to the OPAL opacity services allowing direct comparison as well as study of the effect of uncertainties in stellar modeling due to mean opacities.
accepted in JQSRT
References in corpus (5)
- The chemical composition of the Sun from helioseismic and solar neutrino data
- OPserver: interactive online-computations of opacities and radiative accelerations
- Control and diagnosis of temperature, density, and uniformity in x-ray heated iron/magnesium samples for opacity measurements
- The Solar Heavy Element Abundances: II. Constraints from Stellar Atmospheres
- Helioseismic Constraints on the Solar Ne/O Ratio and Heavy Element Abundances
Cited by in corpus (6)
- Line broadening and the solar opacity problem
- Quantitative comparison of opacities calculated using the -matrix and Distorted-Wave methods: Fe XVII
- Rotating Solar Models in Agreement with Helioseismic Results and Updated Neutrino Fluxes
- Computation of atomic astrophysical opacities
- Solar Models and Astrophysical S-factors Constrained by Helioseismic Results and Updated Neutrino Fluxes
- Progress towards a 3D Monte Carlo radiative transfer code for outflow wind modelling