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Version History

Latest Release - 1.3.0 (2023)

Contributors: C. Louis, P. Zarka, B. Cecconi

Change Log for version 1.3.0:

  • Documentation:
  • Configuration:
    • Added the wave propagation mode (LO or RX) as an (optional) input. Default value is RX.

Version 1.2.0 (2023)

Contributors: C. Louis, B. Cecconi

Change Log for version 1.2.0:

Related Publication:

  • Louis, C. K, Lamy, L., Jackman, C. M., Cecconi, B., Hess, S. L. G. 2023. "Predictions for Unraus-moons radio emissions and comparison with Voyager 2/PRA observations." Planetary, Solar and Heliospheric Radio Emissions IX, edited by C. K. Louis, C. M. Jackman, G. Fischer, A. H. Sulaiman, P. Zucca, DIAS, TCD, Dublin, Ireland, doi: 10.25546/103106.
  • Hue, V., Gladstone, G. R., Louis, C. K., Greathouse, T. K., Bonfond, B., Szalay, J. R., Moirano, A., Giles, R. S., Kammer, J. A., Imai, M., Mura, A., Versteeg, M. H., Clark, G., Gérard, J. -C., Grodent, D. C., Rabia, J., Sulaiman, A. H., Bolton, S. J., Connerney, J. E. P. 2023. "The Io, Europa and Ganymede Auroral Footprints at Jupiter in the Ultraviolet: Positions and Equatorial Lead Angles." Journal of Geophysical Research: Space Physics, 128, 5, e2023JA031363, doi: 10.1029/2023JA031363.

Version 1.1.0 (2020)

Contributors: C. Louis, B. Cecconi

Change Log for version 1.1.0:

  • Documentation:
  • Configuration:
    • SIMU.NAME and SIMU.OUT are not required anymore. SIMU.NAME is curently not used. The SIMU.OUT entry is given by the user in the config.ini file.
    • Adding user-provided frequency list option
    • New configuration option for output CDF: SRCPOS (position of the sources, in cartesian)
    • New configuration option for output CDF: SRCVIS (for each hemisphere, sum of the visible sources)
  • Ephemeris:
    • Adding support for use-provided WebGeoCalc ephemeris files in csv format
    • Updated MIRIADE and WebGeoCalc ephemerides parsing methods (following undocumented webservice API changes)
    • Modification on the User-defined ephemeris: the ephemerides given by the user can be defined to an accuracy of one second
  • Output CDF:
    • Changing the polarization output in cdf file: Polarization variable indicates LH or RH polarization, VisibleSources provides the sum of visible sources for LH and RH polarization.
    • Added Hemisphere_ID_Label variable in output CDF
    • Modified the calculation of CDF output SrcFreqMaxCMI
    • Modification of the CDF outputs if multiple sources
    • Correction of an error on the CDF output time table
  • Other:
    • Modify CDF file output version to: ...._v11.cdf
    • All CDF global attributes are now with type CDF_CHAR
    • Modifying call to MFL (lsh vs. msh, depending on the planet)
    • Added support for M-shell with JRM09 magnetic field model

Related Publication:

  • Cecconi, B. C. K. Louis, C. Muñoz, C. Vallat. 2021. "Jovian auroral radio source occultation modelling and application to the JUICE science mission planning." Planetary and Space Science, 209, 105344, doi: 10.1016/j.pss.2021.105344.

Version 1.0.0 (2019)

In this version, the code is called ExPRES (Exoplanetary and Planetary Radio Emissions Simulator)

Contributors: C. Louis, S. L. G. Hess, P. Zarka, B. Cecconi, L. Lamy

Main additions in this version:

  • open source licence and distribution on github
  • better documentation

Related Publications:

  • Louis CK, SLG 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: A30. doi:10.1051/0004-6361/201935161.

Version 0.6.1 (2018)

In this version, the code is called SERPE (Simulation d'Emission Radio Planétaires et Exoplanétaires)

Contributors: C. Louis, S. L. G. Hess, P. Zarka, B. Cecconi, L. Lamy

Main additions in this version:

  • better validation of the simulation steps
  • access IMCCE/Miriade ephemeris webservice for observers and natural body locations
  • output in CDF
  • input in JSON or SRP (original input file format)

Related publications:

  • Louis, CK, L Lamy, P Zarka, B Cecconi, and SLG Hess. 2017. “Detection of Jupiter Decametric Emissions Controlled by Europa and Ganymede with Voyager/PRA and Cassini/RPWS.” J. Geophys. Res. Space Physics 122 (September): 1–20. doi:10.1002/2016JA023779.
  • Louis, CK, L Lamy, P Zarka, B Cecconi, SLG Hess, X Bonnin. 2018. Simulating Jupiter-satellite decametric emissions with ExPRES: a parametric study", PRE8 proceedings, arXiv:1804.10499 and Cassini/RPWS.” J. Geophys. Res. Space Physics 122 (September): 1–20. doi:10.1002/2016JA023779.
  • Louis, CK, L Lamy, P Zarka, B Cecconi, M Imai, WS Kurth, G Hospodarsky, et al. 2017. “Io-Jupiter Decametric Arcs Observed by Juno/Waves Compared to ExPRES Simulations.” Geophys. Res. Lett., 1–17. doi:10.1002/2017GL073036.

Version 0.6.0 (2011)

In this version, the code is called SERPE (Simulation d'Emission Radio Planétaires et Exoplanétaires)

Contributors: S. L. G. Hess, P. Zarka, B. Cecconi, L. Lamy

Main additions in this version:

  • major reorganization of the code
  • output of 3D movies added

Related publication:

  • Cecconi, B, SLG Hess, A Hérique, Maria Rosaria Santovito, Daniel Santos-Costa, Philippe Zarka, G Alberti, et al. 2012. “Natural Radio Emission of Jupiter as Interferences for Radar Investigations of the Icy Satellites of Jupiter.” Planet. Space Sci. 61: 32–45. doi:10.1016/j.pss.2011.06.012.

Version 0.5.0 (2010)

In this version, the code is called SERPE (Simulation d'Emission Radio Planétaires et Exoplanétaires)

Contributors: S. L. G. Hess, L. Lamy, P. Zarka, B. Cecconi

Main additions in this version:

  • possibility to run simulations for exoplanetary radio emissions

Related publication:

  • Hess, S L G, and P Zarka. 2011. “Modeling the Radio Signature of the Orbital Parameters, Rotation, and Magnetic Field of Exoplanets.” Astronomy and Astrophysics 531 (June): A29. doi:10.1051/0004-6361/201116510.

Version 0.4.2 (Feb 2008)

In this version, the code is called SERPE (Simulation d'Emission Radio Planétaires et Exoplanétaires)

Contributors: L. Lamy, S. L. G. Hess, P. Zarka, B. Cecconi

Main additions in this version:

  • added altitude of aurora (fmax_alt) parameter

Related Publication:

  • Lamy, L, Philippe Zarka, B Cecconi, SLG Hess, and Renée Prangé. 2008. “Modeling of Saturn Kilometric Radiation Arcs and Equatorial Shadow Zone.” J. Geophys. Res. 113 (A10213). doi:10.1029/2008JA013464.
  • Lamy, L, B Cecconi, P Zarka, P Canu, P Schippers, W S Kurth, R L Mutel, D A Gurnett, D Menietti, and P Louarn. 2011. “Emission and Propagation of Saturn Kilometric Radiation: Magnetoionic Modes, Beaming Pattern, and Polarization State.” J. Geophys. Res. 116 (A04212). doi:10.1029/2010JA016195
  • Lamy, L, R Prangé, W Pryor, J Gustin, S V Badman, H Melin, T Stallard, D G Mitchell, and P C Brandt. 2013. “Multispectral Simultaneous Diagnosis of Saturn's Aurorae Throughout a Planetary Rotation.” Journal of Geophysical Research (Space Physics) 118 (8): 4817–43. doi:10.1002/jgra.50404.

Version 0.4.1 (Oct 2007)

In this version, the code is called SERPE (Simulation d'Emission Radio Planétaires et Exoplanétaires)

Contributors: L. Lamy, S. L. G. Hess, P. Zarka, B. Cecconi

Main additions in this version:

  • New feature to use any trajectory provided by the user.
  • Plasma disc density contribution included.

More details in the version history part of the serpe.pro header.

Related publication:

  • Hess, SLG, A Pétin, Philippe Zarka, B Bonfond, and B Cecconi. 2010. “Lead Angles and Emitting Electron Energies of Io-Controlled Decameter Radio Arcs.” Planet. Space Sci. 58 (10): 1188–98. doi:10.1016/j.pss.2010.04.011.

Version 0.4.0 (Jun 2007)

In this version, the code is called JUNO.

Contributors: S. L. G. Hess, P. Zarka, B. Cecconi, L. Lamy

Main added features:

  • better portability (plotting option for Windows users)
  • added effect of plasma density

Version 0.3.7 (Mar 2007)

In this version, the code is called JUNO.

Contributors: L. Lamy, S. L. G. Hess, P. Zarka, B. Cecconi

Main added features:

  • latitude axis output

Version 0.3.6 (Feb 2007)

In this version, the code is called JUNO.

Contributors: S. L. G. Hess, P. Zarka, B. Cecconi, L. Lamy

Main added features:

  • ehanced planet description parameters
  • fixed spdyn output
  • local_time axis output

Version 0.3.5 (Jan 2007)

In this version, the code is called JUNO.

Contributors: S. L. G. Hess, P. Zarka, B. Cecconi

Main added features:

  • active_LT (local time) feature
  • set other planet than Jupiter
  • better portability for processing on different servers

Version 0.3.4 (Nov 2006)

In this version, the code is called JUNO.

Contributors: B. Cecconi, S. L. G. Hess, P. Zarka

Main added features:

  • speed up of computing

Version 0.3.3 (Nov 2006)

In this version, the code is called JUNO.

Contributors: B. Cecconi, S. L. G. Hess, P. Zarka

Main added features:

  • speed up of computing (vector computation instead of loop)
  • better spatial interpolation of magnetic field

Version 0.3.2 (Nov 2006)

In this version, the code is called JUNO.

Contributors: S. L. G. Hess, P. Zarka, B. Cecconi

Main added features:

  • two spectrogram per source for moon controlled source (Nother and Southern sources)

Version 0.3.1 (Nov 2006)

In this version, the code is called JUNO.

Contributors: B Cecconi, S. L. G. Hess, P. Zarka

Main added features:

  • spectral axis interpolation before computation (more accurate results)
  • one spectrogram per source for better analysis of the results

Version 0.3.0 (Oct 2006)

In this version, the code is called JUNO.

Contributors: B. Cecconi, S. L. G. Hess, P. Zarka

Main added features:

  • no more common blocks, using pointers instead

Version 0.2.0 (Sep 2006)

This is the first tracked version. In this version, the code is called JUNO.

Contributors: S. L. G. Hess, P. Zarka, B. Cecconi

Main features:

  • computation of the Jovian radio emission visibility from an observer
  • input of orbital parameters for observers in orbit around Jupiter