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The SSI data exhibit similar characteristics as the AD data.
The SORCE TSI and SSI data describe solar variability without the proxy of the 10.7-cm radio flux.
The SSI data have a spectral resolution of 1 nm with a maximum uncertainty of approximately 0.15 % in the UV range.
Second, the inability to distinguish between organ space and deep space means that any aggregated SSI data reported by type of infection will likely be unreliable and incomparable.
The use of retrieved SSI data depends on the accuracy of the output results.
We present a brief synopsis of the nature of SSI data that was taken during the nominal Galileo mission.
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NOIS-SSI data were appended to NPR data for data analysis purposes.
In addition, NOIS-SSI data are manually checked by infection control practitioners who may manually correct the data.
In addition we evaluated the accuracy based on the type of ICM used for collecting NOIS-SSI data.
Type of ICM was manually coded into four categories according to whether the NOIS-SSI data for a specific year was generated from of one of the three ICM suppliers (anonymized as A, B or C to protect the identity of individual hospitals), or from a manual or in-house system (other).
The identified flutter derivatives of the thin plate model based on the SSI-DATA technique agree well with those obtained theoretically.
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