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Corresponding Dataset for Gravity Field of Ganymede after the Juno Extended Mission

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https://zenodo.org/record/6949644
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Corresponding Dataset for Gravity Field of Ganymede after the Juno Extended Mission     Luis Gomez Casajus August 2, 2022 ============================================================================= Introduction =============================================================================     This dataset contains the estimated gravity field and its corresponding full covariance matrix. This dataset is provided in order to  supplement the submitted article to the "Geophysical Research Letters" journal:     Gravity Field of Ganymede after the Juno Extended Mission.         L. Gomez Casajus (*), A. I. Ermakov, M. Zannoni, J. T. Keane,          D. Stevenson, D. R.Buccino, D. Durante, M. Parisi, R. S. Park,          P. Tortora and S. J. Bolton                  - (*) luis.gomezcasajus@unibo.it ============================================================================= File description =============================================================================     This archive contains two files within the root directory.          ROOT         -SOI_gravity_field.txt             This file contains the estimated normalized spherical harmonics              coefficients of the Ganymede gravity field.             The file contains a header row which provides a description of              the file.         -SOI_cov_matrix.txt             This file contains the estimated full covariance matrix (32x32)              of the normalized spherical harmonics coefficients of the              Ganymede gravity field. The file contains a header row which              provides a description of the file. The matrix is represented as             a 2 dimensional array whose coefficients follow the following              order scheme: C20 C21 S21 C22 S22 C30 C31 ... ============================================================================= ACKNOWLEDGMENTS =============================================================================     The authors are grateful to William Folkner, to the entire Solar System  Dynamics Group and to Robert Haw, former Galileo navigator, for the useful  discussions and suggestions regarding the procedures for Galileo data  analysis. L.G.C., M.Z., and P.T. are grateful to the Italian Space Agency  (ASI) for financial support through Agreement No. 2017-40-H.1-2020, and its  extension2017-40-H.02020-13-HH.0, for ESA’s BepiColombo and NASA’s Juno radio science experiments. L.G.C., M.Z., and P.T. acknowledge Caltech and the Jet  Propulsion Laboratory for granting the University of Bologna a license to an  executable version of MONTE Project Edition S/W. JTK and AIE acknowledge  support from the Juno participating scientist program. The work of RP, DB,  JTK, and MP was carried out at the Jet Propulsion Lab, California Institute of Technology, under a contract with the National Aeronautics and Space  Administration (80NM0018D0004). Government sponsorship acknowledged.
创建时间:
2022-08-03
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