M2 ocean tide parameters and the deceleration of the moon's mean longitude from satellite orbit data

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Lunar Tides, Moon-Earth Trajectories, Satellite Orbits, Data Acquisition, Deceleration, Longitude Measurement, Parameterization, Spherical Harmonics

Scientific paper

An estimation was made of the principal long period spherical harmonic parameters in the representation for the M2 ocean tide from the orbital histories of three satellites - 1967-92A (TRANSIT), Starlette, and GEOS-3. The data used were primarily the evolution of the orbital inclinations of the satellites, with the addition of the longitude of the ascending node from GEOS-3. The results are: (1) C22 superscript + = 3.42 plus or minus 0.24 cm; (2)42 superscript + = 0.97 plus or minus 0.12 cm; (3) epsilon subscript 22 superscript + = 325 D.5 plus or minus 3.D9; (4) epsilon subscript 42 superscript + = 42 = 124D.0 plus or minus 6 D.9. These values agree quite well with recent numerical models and another recent determination from satellite data. The M2 parameters obtained here infer an N of -25 plus or minus 3 arc seconds/century squared, in good agreement with other investigators. The range of current determinations of N is from -24.6 to 27.2 arc second/century squared.

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