- [DAS-2216] The Swath Projector has been updated with quick fixes to add support for TEMPO level 2 data. These changes include optional transposing of arrays based on dimension sizes, addition of rows_per_scan parameter for ewa interpolation, and updates to the configuration file for TEMPO_O3TOT_L2 to correctly locate coordinate variables and exclude science variables with dimensions that do no match those of the coordinate variables.
- [TRT-558]
The Swath Projector has been updated to use
earthdata-varinfo
version 3.0.0. This update primarily involves the streamlining of the configuration file schema. Please see the earthdata-varinfo release notes for more information. The configuration file used by the Swath Projector has also been renamed toearthdata_varinfo_config.json
.
- [DAS-1934]
Input parameters that include both both resolutions (
xres
andyres
) and dimenions (height
andwidth
) no longer always raise an exception. An exception is raised only when the parameters describe a grid that is not internally consistent. #14
This version of the Swath Projector implements black code formatting across the entire repository. There should be no functional changes to the service.
This version of the Harmony Swath Projector contains all functionality
previously released internally to EOSDIS as sds/swot-reproject:0.0.4
.
Minor reformatting of the repository structure has occurred to comply with
recommended best practices for a Harmony backend service repository, but the
service itself is functionally unchanged. Additional contents to the repository
include updated documentation and files outlined by the
NASA open-source guidelines.
Repository structure changes include:
- Migrating
pymods
directory toswath_projector
. - Migrating
swotrepr.py
toswath_projector/adapter.py
. - Addition of
swath_projector/main.py
.
For more information on internal releases prior to NASA open-source approval, see legacy-CHANGELOG.md.