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@vbrancat this looks good and seems to cover the basic configuration needed. Two extra design points that we discussed offline to some extent and could be documented here for more clarity are the following: 1- The geocoded bursts must be stackable
2- The geocoded bursts must be easy to mosaic without need for interpolation (resampling) Mosaicking the geocoded bursts should not require extra interpolation. The following plot shows the two geocoded grids and two different possible situations.
In summary I think by ensuring the top-left corners to be integer multiple of the spacing, 1-b and 2-b conditions above can be realized. The SAS design will anyways allow for 1-c by providing the configuration parameters of the geocoded grid. However, defining those parameters and populating them in the SAS run configuration by the data system needs to be further discussed. tagging @gshiroma @yunjunz @LiangJYu in case if they have more thoughts. |
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Some thoughts on the interface for geocoded S1-A/B CSLCs.
Problem we want to solve
Let' assume we have
N
frames (SAFE) for a static stack covering an Area of Interest (AoI). The SAS should geocode the burst with specifiedburst_id
. All the bursts with same burst_id belonging to different dates should be geocoded on the same geogrid.It is desirable that the SAS will handle invalid data in each burst (this will make stitching much easier). Therefore, the SAS should extract the valid data portion of each burst and geocode it on the assigned geogrid.
Interface with PCM/PGE
The SAS will accept as an input:
Functionalities we want to include in the processing section
A section
geocode
including all the parameters necessary to perform geocode.If the parameters necessary to create a geogrid are not assigned, as a deafult, we can use the burst polygon border to generate the geogrid with some default x and y spacings.
A section of split-spectrum. This functionality should be optional i.e., the user can decide to turn it on or off. If split-spectrum is activated, the SAS will extract the valid portion of each burst, split its spectrum, and generate a temporary output file containing 3 bands: the lower burst band, the main band, the high band. The SAS will then geocode all three bands.
This section will include:
Note that S1-A/B metadata have info on the window used during image formation. To taper the spectrum, we should use the same window as specified in the metadata. This will require to expose this functionality in the reader.
Anything else I am missing?
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