ECLIPSE: Emission Calculation and Line Prediction for SOLAR-C EUVST
The ECLIPSE code (Emission Calculation and Line Prediction for SOLAR-C EUVST) is used to forward model the performance of the EUV spectrograph EUVST onboard the SOLAR-C spacecraft.
Contact: James McKevitt (jm2@mssl.ucl.ac.uk). See LICENSE for usage terms.
The instrument response generated by this code will be updated during instrument development, testing, and commissioning.
Full documentation - installation, quick start, the synthesis and instrument response guides, and the analysis tutorial - 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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