ECLIPSE: Emission Calculation and Line Prediction for SOLAR-C EUVST
ECLIPSE (Emission Calculation and Line Prediction for SOLAR-C EUVST) predicts what the EUV spectrograph EUVST on SOLAR-C will measure, and how precisely, starting from a model of the solar atmosphere. It also models Hinode/EIS.
Contact: James McKevitt (jm2@mssl.ucl.ac.uk). See LICENSE for usage terms.
The instrument model will be updated as EUVST is built, tested and commissioned.
ECLIPSE is installed with pip install eclipse. ECLIPSE 0.12 and earlier were on PyPI as solarc-eclipse.
The documentation, with installation and a first run, guides to synthesising spectra, simulating the instrument and analysing the results, and a worked example, is at solarc-eclipse.readthedocs.io.
Acknowledgements
The SOLAR-C/EUVST-SW instrument is an ESA-funded contribution to the JAXA-led SOLAR-C mission. The EUVST-LW (long wavelength) instrument is contributed by NASA. The ECLIPSE code is developed and maintained at Mullard Space Science Laboratory (UCL), and was made using Austrian Super Computing (ASC) infrastructure in collaboration with the University of Vienna.
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