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Add support for a third mode of nav.colocate that finds the planet's center based on cross-correlation between models and observations of planetary rings. This is useful because rings are often less time-variable than stormy planets, and they are also larger on the sky; together, this promises higher-accuracy centroiding.
The text was updated successfully, but these errors were encountered:
Add support for a third mode of nav.colocate that finds the planet's center based on cross-correlation between models and observations of planetary rings. This is useful because rings are often less time-variable than stormy planets, and they are also larger on the sky; together, this promises higher-accuracy centroiding.
The text was updated successfully, but these errors were encountered: