Published March 27, 2024
| Version 1.0.0
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Spherical harmonic models of the gravity field of Jupiter
Description
This archive contains published spherical harmonic models of the gravity field of Jupiter. The coefficients are to be used with unnormalized spherical harmonic functions that exclude the Condon-Shortely phase factor of (-1)^m, and the file is formatted in a manner to be read by the pyshtools software (using format='shtools'). The header of the file contains the reference radius, GM, GM uncertainty, and maximum degree of the spherical harmonic expansion (all in SI units).
* Kaspi2023.sh (value of GM provided by Y. Kaspi, personal communication)
Files
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(88.4 kB)
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Additional details
Related works
- Is described by
- Publication: 10.1038/s41550-023-02077-8 (DOI)
References
- Kaspi, Y., Galanti, E., Park, R. S., Duer, K., Gavriel, N., Durante, D., Iess, L., Parisi, M., Buccino, D. R., Guillot, T., Stevenson, D. J., & Bolton, S. J. (2023). Observational evidence for cylindrically oriented zonal flows on Jupiter. Nature Astronomy, 7(12), 1463–1472. https://doi.org/10.1038/s41550-023-02077-8