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NOIRE Sensitivity plots for Planetary Kilometric Radiation

Wednesday 9 April 2025, by Baptiste Cecconi

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

  • 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.