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ExPRES Jovian Radio Emission Simulations Data Collection v11

Tuesday 19 December 2023, by Corentin Louis

This collection is composed of pre-computed simulation runs of the ExPRES code, with a fixed set of parameters, and for various observers, as described in Louis et al. (2019).

  • DOI: 10.25935/y0f3-9n63
  • Publisher: PADC
  • License: CC-BY 4.0
  • Citation: Louis, C., B. Cecconi & A. Loh (2023). ExPRES Jovian Radio Emission Simulations Data Collection (Version 11) [Data set]. PADC. https://doi.org/10.25935/y0f3-9n63

This collection is a new version of:


Link to data repository

Description

This data collection contains pre-computed ExPRES simulation runs, with the following input parameters:

  • Magnetic Field Model: JRM33 (Connerney et al, 2021)
  • Current Sheet Model: Connerney et al (2020)
  • CMI Mechanism: Loss Cone, with a 1° sheet thickness
  • Electron energy: 3 keV

The altitude of the Jovian aurora is set to 650 km (this constrains the maximum value of fc). There is no refraction.

The precomputed observers and associated time ranges are:

  • Earth (1990-01-01 to 2024-12-31)
  • Juno (2016-01-01 to 2023-12-31)

The data files contain the modelled following parameters: polarization, theta, CML (obs longitude), obs latitude, obs distance, srcfreqmax, srcfreqmaxCMI, srcLongitude,fp and fc (detailed informations are available in Louis et al (2019)).

The data files are provided in CDF format, and the ExPRES input files are JSON files.

References

  • Connerney, J. E. P., Timmins, S., Oliversen, R. J., Espley, J. R., Joergensen, J. L., Kotsiaros, S., et al. (2022). A new model of Jupiter’s magnetic field at the completion of Juno’s Prime Mission. Journal of Geophysical Research: Planets, 127, e2021JE007055. https://doi. org/10.1029/2021JE007055
  • Connerney, J. E. P., Timmins, S., Herceg, M., & Joergensen, J. L. (2020). A Jovian magnetodisc model for the Juno era. Journal of Geophysical Research: Space Physics, 125, e2020JA028138. https://doi.org/ 10.1029/2020JA028138
  • Hess, S L G, B Bonfond, F Bagenal, and L Lamy. 2018. “A Model of the Jovian Internal Field Derived From in-Situ and Auroral Constraints.” Planetary, Solar and Heliospheric Radio Emissions (PRE VIII), August, 157–68. doi:10.1553/PRE8s157.
  • Louis, C K, S L G Hess, B Cecconi, P Zarka, L Lamy, S Aicardi, and A Loh. 2019. “ExPRES: an Exoplanetary and Planetary Radio Emissions Simulator.” Astronomy and Astrophysics 627 (May): A30. doi:10.1051/0004-6361/201935161.

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