diff --git a/README.md b/README.md index ec45c0a4fb0cfb78350e5d6c714e172e6de49510..b37e242c2c70114795949b713dcb10418a16ec28 100644 --- a/README.md +++ b/README.md @@ -36,12 +36,13 @@ For full testing reports and example usage, please see the linked example Jupyte | Instrument | Jupyter Notebooks | Production Ready | Difference CSM -> ISIS (in pixels) | Difference ISIS -> CSM (in pixels) | |:---------------------:|:-------------------------------------------------:|:-----------------:|:---------------------------------------:|:---------------------------------------:| | MRO HiRISE | [link](examples/mro_hirise_isis_cmp.ipynb) | sub-pixel; in testing for production | sample mean=-2.0e-05; line mean=2.5e-08 | sample mean=-3.0e-08; line mean=1.2e-04 | -| MRO CTX | [link](examples/mro_ctx_isis_cmp.ipynb) | No (gross errors) | sample mean=0.8; line mean=-896 | sample mean=0.8; line mean=-0.3 | -| MEX HRSC | [link](examples/mex_hrsc_isis_cmp.ipynb) | No | sample mean=-80; line mean=-3 | sample mean=80; line mean=3 | -| LROC NAC | [link](examples/lrocnac_isis_cmp.ipynb) | No (gross errors) | sample mean=-40; line mean=-5 | n/a | -| Kaguya Terrain Camera | [link](examples/kaguya_tc_isis_cmp.ipynb) | No (gross errors) | sample mean=-5; line mean=-1516 | sample mean=5; line mean=1906 | -| Messenger MDIS NAC | [link](examples/messenger_mdisnac_isis_cmp.ipynb) | No | sample mean=-0.2; line mean=-5 | sample mean=0.3; line mean=5 | -| Cassini ISS | [link](examples/cassini_isis_cmp.ipynb) | No | sample mean=-12.3; line mean=-0.1 | sample mean=-0.2; line mean=0.9 | -| Dawn Framing Camera | [link](examples/dawn_fc_isis_cmp.ipynb) | sub-pixel; in testing for production | sample mean=-1.9e-03; line mean=1.8e-03 | sample mean=1.9e-03; line mean=-1.8e-03 | - -The Difference column (CSM -> ISIS) represents the mean difference in pixels from running usgscsm's *image2ground* and then back to the camera using ISIS3's *campt* (ground2image). The Difference column (ISIS -> CSM) is simply the reverse starting with ISIS3 first with *campt* (image2ground) and then usgscsm's *ground2image*. \ No newline at end of file +| MRO CTX | [link](examples/mro_ctx_isis_cmp.ipynb) | nearly sub-pixel; in testing | | sample mean=1.4; line mean=0.01 | +| MEX HRSC | [link](examples/mex_hrsc_isis_cmp.ipynb) | sub-pixel; in testing for production | sample mean=-80; line mean=-3 | sample mean=0.0004 ; line mean=0.05 | +| LROC NAC | [link](examples/lrocnac_isis_cmp.ipynb) | sub-pixel; in testing for production | sample mean=-0.003; line mean=-0.0006 | sample mean=0.003 line mean=0.0005 | +| Kaguya Terrain Camera | [link](examples/kaguya_tc_isis_cmp.ipynb) | barely sub-pixel; in testing | sample mean=0.5; line mean=-0.9 | sample mean=-0.5; line mean=0.94 | +| Messenger MDIS NAC | [link](examples/messenger_mdisnac_isis_cmp.ipynb) | sub-pixel; in testing for production | sample mean=-0.01; line mean=-0.003 | sample mean=0.01; line mean=0.003 | +| Cassini ISS NAC | [link](examples/cassini_isis_nac_cmp.ipynb) | sub-pixel; in testing for production | sample mean=-0.001; line mean=0.01 | sample mean=0.001; line mean=-0.01 | +| Cassini ISS WAC | [link](examples/cassini_isis_wac_cmp.ipynb) | sub-pixel; in testing for production | sample mean=0.001; line mean=0.004 | sample mean=-0.001; line mean=-0.004 | +| Dawn Framing Camera | [link](examples/dawn_fc_isis_cmp.ipynb) | sub-pixel; in testing for production | sample mean=-0.02; line mean=0.003 | sample mean=0.02; line mean=-0.003 | + +The Difference column (CSM -> ISIS) represents the mean difference in pixels from running usgscsm's *image2ground* and then back to the camera using ISIS3's *campt* (ground2image). The Difference column (ISIS -> CSM) is simply the reverse starting with ISIS3 first with *campt* (image2ground) and then usgscsm's *ground2image*.