This dataset is a supplementary material to Rouillé et al. (2025), submitted to Radio Science. It contains a Jupyter notebook, which allows to reproduce the figures of the paper.
Link to data
Description
The provided Jupyter notebook can be used to reproduce the figures of Rouillé et al. (2025), submitted to Radio Science. It uses data from Zarka & Cecconi (2022) and Marc et al. (2024).
Scripts
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NOIRE_sensitivity_PKR.ipynb: Jupyter Notebook file.
Acknowledgement
ER was supported by CNES. BC was supported by PADC.
Contact
Any question or request should be addressed to contact.maser@obspm.fr
References
- Marc, G., Sicard, A, & Nénon, Q. (2024), Results of Cyclo-Synchrotron and Synchrotron Models with Python Visualization Program (V1) [Dataset], Recherche Data Gouv. doi:10.57745/WEAFZK
- Zarka, P., B. Cecconi. (2022), Solar System Low Frequency Radio Spectra (Version 1.0) [Dataset]. PADC/MASER. doi:10.25935/YAWF-AF18
- Zarka, P., J.-L. Bougeret, C. Briand, B. Cecconi, H. Falcke, J. Girard, J.-M. Grießmeier, S. Hess, M. Klein-Wolt, A. Konovalenko, L. Lamy, D. Mimoun, A. Aminaei. (2012), Planetary and exoplanetary low frequency radio observations from the Moon, Planetary and Space Science, 74(1), 156-166.
doi:10.1016/j.pss.2012.08.004.
