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A new method for correcting the refraction angle of starlight under the conditions of 0–$$90^{\circ }$$ zenith distance and 0–200 km observation height

Crossref DOI link: https://doi.org/10.1038/s41598-025-20261-w

Published Online: 2025-10-16

Update policy: https://doi.org/10.1007/springer_crossmark_policy

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