Repository navigation
ALE 2.0.0 Release Prep - #760
Merged
Merged
Conversation
Kelvinrr
approved these changes
Nov 6, 2026
This file contains hidden or bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Sign up for free
to join this conversation on GitHub.
Already have an account?
Sign in to comment
Add this suggestion to a batch that can be applied as a single commit.This suggestion is invalid because no changes were made to the code.Suggestions cannot be applied while the pull request is closed.Suggestions cannot be applied while viewing a subset of changes.Only one suggestion per line can be applied in a batch.Add this suggestion to a batch that can be applied as a single commit.Applying suggestions on deleted lines is not supported.You must change the existing code in this line in order to create a valid suggestion.Outdated suggestions cannot be applied.This suggestion has been applied or marked resolved.Suggestions cannot be applied from pending reviews.Suggestions cannot be applied on multi-line comments.Suggestions cannot be applied while the pull request is queued to merge.Suggestion cannot be applied right now. Please check back later.
Changes for 2.0.0:
Added
INS<ikid>_K1coefficient) that ISIS models, and subtracts 0.5 from the detector center to match the ISIS 0.5-based detector-coordinate convention. The resulting CSM camera agrees with the ISIS camera to sub-pixel (cam_test pixel difference drops from ~0.7 px to ~1e-8 px on a real NEAR MSI image). #740NirCamera+RadialDistortionMap) that ISIS models, and subtracts 0.5 from its detector center to match the ISIS 0.5-based detector-coordinate convention. The resulting CSM camera agrees with the ISIS camera to sub-pixel (cam_test pixel difference drops from ~1.2 px median, ~6 px max to ~1e-7 px on a real Clementine NIR image). The UVVIS, HiRes and LWIR Clementine cameras are unchanged; only NIR is modeled here. #740ck3sdn. This uses a tolerance to reduce the number of quaternions for ISDs that don't extract the exact CK times from the kernels. #747Fixed
find_package(ale)works without a priorfind_package(nlohmann_json). #748evaluateCubicHermiteFirstDerivnow checks thatyhas as many points as the derivatives and times, instead of reading past the end ofy. #749focal_lengthno longer raisesAttributeErrorwhenINS_FOCAL_LENGTHis defined.ephemeris_start_timeuses the scalar fromutcToEt(was a tuple). #739isd_generatenow fails with an error instead of writing an ISD with null required fields. #754Changed
isd_generate: default--reductiontolinear(sampling every 10th line for line-scan images with >= 1000 lines). This avoids creating oversized ISDs (tens of thousands of pose samples) for long line-scan sensors such as LRO NAC, MRO CTX, and HRSC. Pass--reduction noneto disable reduction and restore per-line sampling. #744Removed
Licensing
This project is mostly composed of free and unencumbered software released into the public domain, and we are unlikely to accept contributions that are not also released into the public domain. Somewhere near the top of each file should have these words: