During decoding and cleaning, it was assumed that the time slope of the files would be roughly guided by the Pulse Repetition Interval (PRI) of the satellite, i.e. a Pulse Repetition Frequency (PRF) of 1647 Hz means that 1,647 lines are being transmitted and received per second. This means that the PRI is 0.00060716 msec. Based upon this, then, each 1,000 lines of Seasat data should be equivalent to .60716 seconds.
Alternately, in milliseconds, the time slope for these files should always be 0.60716. It was discovered that this is not the case with much of the actual data, as shown in the following table and graphs:
|Line||Time||Time Diff||Calculated Slope|
Seasat Times: PRF = 1647 Hz, so PRI is 0.0006071645 msec. In MSEC, the time slope should always be 0.6071645. Yet, for this datatake, the time slope is consistently only 0.486!
Comparison of Original with Filtered: Although the times look fine in the first (unfiltered) plot, they are wrong for this satellite based upon the known PRI. The ASF cleaning software tried to fix these wrong time values using a known slope of 0.607. This introduced a discontinuity into the data and resulted in incorrect times.
These results, wherein the time slope of the raw data does not match the known PRI of the satellite, were incredibly perplexing. At first, it was assumed that these data could not be processed reliably and were simply categorized into the large time-slope error and wrong-fix error categories.
Analysis of the time slopes in the original unfiltered data only pointed out how extreme the problem really was. Well over 100 files showed slopes that were either less than 0.606 or more than 0.608, with the lowest in the 0.48 range. The highest reliable estimate showed a slope of well over 0.62.
6.1 Slope Issues Explained
Eventually, through conversation with original Seasat engineers at the Jet Propulsion Lab (JPL), it was discovered that the Seasat metadata field MSEC of Day actually contains not only the time of imaging but also the time to transmit data from the spacecraft to the ground station. This adds a variable time offset to the metadata field. Once this was understood, it was readily obvious that using the known PRF as a guide for filtering was an incorrect solution.
Thus, the entire cleaning process was revisited, with all of the codes allowing more relaxed slope values during linear regression. This worked considerably better than the previous cleaning attempt. However, it did not solve the problems entirely.
6.2 Final Results of Data Cleaning
The final set of cleaned Seasat raw swaths was assembled using three main passes through the archives with different search parameters, along with a few files that were fixed on a case-by-case basis. Basically, the final version of the code was run and the results examined for remaining time gaps. Any files with large or many time gaps were reprocessed using different parameters. In the end, 1,346 swaths were cleaned, 2 by hand, 14 from the first pass, 25 from the second pass, and the remainder in the final cleaning pass. These then are the final cleaned Seasat archives for the initial release of ASF’s Seasat products.
|Date||Total Datasets||Dataset with Time Gaps||Largest Time Gap||Largest number of gaps in a file||Files with >10 msec gap|
Final Cleaned Seasat Swaths: Approximately one year after the project started, 1,346 raw Seasat swaths were cleaned and ready to be processed into SAR image products.
Written by Tom Logan, July 2013