Open Access
Table 7.
Description of the four published final versions of each EIT light curve.
| Version | Filename string | Description &suggested use cases |
|---|---|---|
| Version (1), viewing angle-corrected no viewing angle correction | Corrected_all_heliocentriccorr corrected_all | Uniformly corrected for instrumental systematics across whole mission lifetime; ∼homoscedastic uncertainties. |
| Suitable for e.g., testing pipelines that will be applied to long-baseline stellar light curve data with homoscedastic uncertainties. | ||
| Version without viewing angle correction could be used to study systematic trends in data from other SOHO instruments. | ||
| Version (2), viewing angle-corrected no viewing angle correction | Corrected_2008onwards_heliocentriccorr corrected_2008onwards | Corrected for bakeouts from 12 Nov. 2008 onward only; heteroscedastic uncertainties, where pre-12 Nov. 2008 uncertainties are much smaller. |
| Suitable for e.g., detailed analysis of how solar activity features appear in light curves, and for analysis of how light curve precision affects our ability to infer or reconstruct such features. | ||
| Version without viewing angle correction could be used for more detailed study of EUV flux incident on Earth. |
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