Publications related to the GRACE Missions (no abstracts)

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MEMS accelerometer for satellite gravimetry

Zhang, Chaoyang, Encarnação, João, Dias, Rosana A., Hormigo, Tiago, Garcia, Ines S., Alves, Filipe S., and Tapley, Byron, 2025. MEMS accelerometer for satellite gravimetry. Advances in Space Research, 76(10):5797–5813, doi:10.1016/j.asr.2025.09.009.

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BibTeX

@ARTICLE{2025AdSpR..76.5797Z,
       author = {{Zhang}, Chaoyang and {Encarna{\c{c}}{\~a}o}, Jo{\~a}o and {Dias}, Rosana A. and {Hormigo}, Tiago and {Garcia}, Ines S. and {Alves}, Filipe S. and {Tapley}, Byron},
        title = "{MEMS accelerometer for satellite gravimetry}",
      journal = {Advances in Space Research},
     keywords = {MEMS accelerometer, Temporal gravity, Non-conservative force, Satellite gravimetry, CubeSat},
         year = 2025,
        month = nov,
       volume = {76},
       number = {10},
        pages = {5797-5813},
     abstract = "{Estimates of Earth's gravity temporal variations by
        GRACE({\ensuremath{-}}FO) have catalyzed a wide range of
        scientific studies and discoveries. Although an increase in the
        satellite pairs would reduce the error and increase the temporal
        and spatial resolution, mission costs limit populating
        additional GRACE-like pairs. One viable solution is to reduce
        costs by miniaturizing the satellite. As a first step in
        reaching this objective, the Miniaturized Prototype for GRavity
        field Assessment using Distributed Earth-orbiting assets
        (uPGRADE) project aims to produce a CHAMP-like prototype
        gravimetry satellite that includes star trackers, GNSS and
        accelerometers in CubeSat size. As one of the primary payloads,
        the utility of high-precision Micro-Electro-Mechanical Systems
        (MEMS) accelerometer for gravimetric mission has not been
        considered. Here, we evaluated three, six and nine MEMS
        arrangements. We found that the six MEMS parallel arrangement
        can observe both the desired non-gravitational accelerations and
        additional absolute value of the angular velocity. We developed
        a measurement error model, associated with MEMS position and
        orientation errors, to guide the MEMS optimal design and
        assembly. Finally, we conducted uPGRADE mission simulations
        using appropriate observations and model errors. The impact of a
        10 nm/s$^{2}$ MEMS accelerometer error on gravity recovery is
        very close to that of the 5 mm GNSS error. However, the
        accelerometer error degrades the low-degree coefficients more
        significantly, particularly <mml:math><mml:mrow><mml:msub><mml:m
        i>C</mml:mi><mml:mn>20</mml:mn></mml:msub></mml:mrow></mml:math>
        and <mml:math><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn>30</
        mml:mn></mml:msub></mml:mrow></mml:math>. The simulations
        indicate that the temporal gravity can be estimated up to degree
        15, albeit with some compromise in the low-degree coefficients.
        Recommendations are made to lower the projected noise floor of
        MEMS accelerometer to enhance the low-degree coefficients
        accuracy.}",
          doi = {10.1016/j.asr.2025.09.009},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2025AdSpR..76.5797Z},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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