http://arxiv.org/abs/1703.04828
The increased amount of high precision seismic data for solar-like stars calls for the existence of tools that can extract information from such data. In the case of the study of acoustic glitches there are no publicly available tools and most existing ones require a deep knowledge of their implementation. In this work a tool is presented that aims to both simplify the interaction with the user and also be capable of working automatically to determine properties of acoustic glitches from seismic data of solar-like stars. This tool is shown to work with both the Sun and other solar analogs but also shows that are still severe limitations to the methods used, when considering smaller datasets.
L. Pereira, J. Faria and M. Monteiro
Thu, 16 Mar 17
22/92
Comments: 4 pages; 5 figures; Submitted to the Proceedings of the joint TASC2/KASC9 workshop – SPACEINN & HELAS8 conference 2016
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