Date: 2024/02/23
DOI: https://doi.org/10.5281/zenodo.10694319
Note: This is a processed and formatted version of the source dataset below. It's mean for use in documentation and tutorials of the Fatiando a Terra project. Please cite the original authors when using this dataset.
Data source: Goossens, S., Sabaka, T. J., Wieczorek, M. A., Neumann, G. A., Mazarico, E., Lemoine, F. G., et al. (2020). High‐Resolution Gravity Field Models from GRAIL Data and Implications for Models of the Density Structure of the Moon's Crust. Journal of Geophysical Research: Planets. doi:10.1029/2019je006086 ; NASA's Planetary Geology, Geophysics and Geochemistry Laboratory
Changes:
- Expanded the spherical harmonic model into a grid.
- Replaced the GM, radius, and angular velocity of the model the those from Wieczorek (2015).
- Generate the grid at a constant height of 11 km above the reference lunar sphere to guarantee the data are outside the topographic masses.
| Checksums | |
|---|---|
| MD5 | md5:d4b9c45f9cbfb0ff903816f89cd0edcf |
| SHA256 | sha256:2b38bdd8ef6ef3af301728387a5a1f27f0a028c0dfc867011125065a3d66acf9 |