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- Latitude correction is calculated using the formula C = 0.5 * g * (sin^2 φ - sin^2 λ), where C is the latitude correction, g is the standard gravity value at sea level, φ is the latitude, and λ is the geodetic latitude1. This formula takes into account the change in gravitational acceleration due to the variation in latitude. There are other formulas available for calculating the latitude correction, such as the 1930 International Gravity Formula, the 1967 International Gravity Formula, the 1976 Telford formula, and the 1980 (Moritz) formula2.Learn more:✕This summary was generated using AI based on multiple online sources. To view the original source information, use the "Learn more" links.Latitude correction is calculated using the formula C = 0.5 * g * (sin^2 φ - sin^2 λ), where C is the latitude correction, g is the standard gravity value at sea level, φ is the latitude, and λ is the geodetic latitude. This formula takes into account the change in gravitational acceleration due to the variation in latitude.www.physicsforums.com/threads/gravity-correction…
There are five formulas provided for calculating the latitude correction:
- The 1930 International Gravity Formula [1] based on the International Ellipsoid used with the Potsdam Ellipsoid:
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