Loading README.md +4 −7 Original line number Diff line number Diff line Loading @@ -35,13 +35,10 @@ Support Data (ISD)* file. Under the CSM standard, each plugin library can define its own ISD camera model format. This library uses an auxiliary JSON formatted file that must be next to the image file passed to the CSM::ISD class. We provide an OpenAPI server for generating these, [pfeffernusse](https://github.com/USGS-Astrogeology/pfeffernusse). The swagger specification is located on [swaggerhub](https://app.swaggerhub.com/apis/USGS-Astro/pfeffernusse2/0.1.4-oas3). You can also use [ALE](https://github.com/USGS-Astrogeology/ale) directly with metakernels to generate the auxiliary JSON file. be next to the image file passed to the CSM::ISD class. ISD files and strings can be generated by using [ALE](https://github.com/USGS-Astrogeology/ale) with metakernels and accompanying SPICE kernels, or from ISIS cubes that have attached SPICE data. The camera model read from an ISD file is converted at load time to an internal representation which makes camera operations more Loading Loading
README.md +4 −7 Original line number Diff line number Diff line Loading @@ -35,13 +35,10 @@ Support Data (ISD)* file. Under the CSM standard, each plugin library can define its own ISD camera model format. This library uses an auxiliary JSON formatted file that must be next to the image file passed to the CSM::ISD class. We provide an OpenAPI server for generating these, [pfeffernusse](https://github.com/USGS-Astrogeology/pfeffernusse). The swagger specification is located on [swaggerhub](https://app.swaggerhub.com/apis/USGS-Astro/pfeffernusse2/0.1.4-oas3). You can also use [ALE](https://github.com/USGS-Astrogeology/ale) directly with metakernels to generate the auxiliary JSON file. be next to the image file passed to the CSM::ISD class. ISD files and strings can be generated by using [ALE](https://github.com/USGS-Astrogeology/ale) with metakernels and accompanying SPICE kernels, or from ISIS cubes that have attached SPICE data. The camera model read from an ISD file is converted at load time to an internal representation which makes camera operations more Loading