GraceSstScaleModel
This programs estimate satellite-to-satellite-tracking (SST) deterministic signals due to eclipse transits and low-SNR values from post-fit residuals. The low-SNR effects are estimated by directly using the residual values. The ensemble averaging method is used to characterize the average properties of eclipse transit signal shapes across all transit events. Each shape is assigned to one arc of 3 hours (default). This can be modefied by enabling averagingInterval.
| Name | Type | Annotation |
|---|---|---|
inputfileGraceResiduals | filename | SST Residuals |
timeMargin | uint | epochs before instrumental events |
waveLength | uint | length of the sample wave |
estimateEclipseTransitScale | sequence | |
outputfileScaleModel | filename | |
inputfileGrace1EclipseFactor | filename | GRACE-A eclipse factors computed with integrated orbit |
inputfileGrace2EclipseFactor | filename | GRACE-B eclipse factors computed with integrated orbit |
averagingInterval | sequence | |
nearestNeighborNumber | uint | |
estimateLowSnrScale | sequence | |
outputfileScaleModel | filename | |
inputfileGraceSstSNR | filename | GRACE SNR values |