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VERSIONS.md

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Version History

Latest Release - 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. 2020. "Auroral Radio Source Occultation Modeling and Application to the JUICE Science Mission Planning." Astron. Astrophys., Submitted.

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