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Commit 6ce1622c authored by Trent Hare's avatar Trent Hare Committed by GitHub
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Update Readme to show updates for CSM vs ISIS3 testing

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...@@ -36,12 +36,13 @@ For full testing reports and example usage, please see the linked example Jupyte ...@@ -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) | | 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 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 | | 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) | No | sample mean=-80; line mean=-3 | sample mean=80; line mean=3 | | 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) | No (gross errors) | sample mean=-40; line mean=-5 | n/a | | 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) | No (gross errors) | sample mean=-5; line mean=-1516 | sample mean=5; line mean=1906 | | 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) | No | sample mean=-0.2; line mean=-5 | sample mean=0.3; line mean=5 | | 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 | [link](examples/cassini_isis_cmp.ipynb) | No | sample mean=-12.3; line mean=-0.1 | sample mean=-0.2; line mean=0.9 | | 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 |
| 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 | | 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*. 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*.
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