Published October 21, 2022 | Version V1.1
Software Open

LESIA-Mag_IDL: LESIA Planetary Magnetic Field IDL computing scripts

Creators

  • 1. LESIA, Observatoire de Paris, CNRS, Meudon, France
  • 2. Dublin Institute for Advanced Studies, Dublin, Ireland
  • 3. ONERA, Toulouse, France

Description

The LESIA Planetary Magnetic Field IDL computing scripts (LESIA-Mag_IDL) repository contains IDL routines to compute planetary magnetic field lines for various planets and models. 

Files

Files (41.4 kB)

Name Size Download all
md5:8f935925f31b465e36f25241167868f2
41.4 kB Download

Additional details

Related works

Is supplement to
Software: https://gitlab.obspm.fr/maser/lesia-mag/lesia-mag_idl/-/tree/V1.1 (URL)

Funding

EPN-2024-RI – Europlanet 2024 Research Infrastructure 871149
European Commission

References

  • Anderson, B. J., C. L. Johnson, H. Korth, R. M. Winslow, J. E. Borovsky, M. E. Purucker, J. A. Slavin, S. C. Solomon, M. T. Zuber, and R. L. McNutt (2012). Low‐degree structure in Mercury's planetary magnetic field. J. Geophys. Res., 117, E00L12, doi:10.1029/2012JE004159.
  • Connerney, J E P. (2007). Planetary Magnetism. In Treatise on Geophysics: Planets and Moons, edited by Tilman Spohn, 10, 243–80. Elsevier.
  • Connerney, J. E. P. (1992). Doing more with Jupiter's magnetic field, in Planetary Radio Emissions III, edited by S. J. Bauer and H. O. Rucker, pp. 13-33, Austria Acad. of Sci. Press, Vienna. https://austriaca.at/?arp=0x0015cd0e
  • Connerney, J. E. P., M. H. Acuna, and N. F. Ness (1981). Modeling the Jovian current sheet and inner magnetosphere. J. Geophys. Res., 86(A10), 8370-8384. doi:10.1029/JA086iA10p08370.
  • Connerney, J. E. P., M. H. Acuna, and N. F. Ness (1984). The Z3 Model of Saturn's Magnetic Field and the Pioneer 11 Vector Helium Magnetometer Observations. J. Geophys. Res., 89(A9), 7541–7544. doi:10.1029/JA089iA09p07541.
  • Connerney, J. E. P., M. H. Acuna, and N. F. Ness (1987). The magnetic field of Uranus. J. Geophys. Res., 92(A13), 15329-15336. doi:10.1029/JA092iA13p15329.
  • Connerney, J. E. P., M. H. Acuna, N. F. Ness, and T. Satoh (1998). New Models of Jupiter's Magnetic Field Constrained by the Io Flux Tube Footprint. J. Geophys. Res., 103(A6), 11929–11939. doi:10.1029/97JA03726.
  • Connerney, J. E. P., S. Kotsiaros, R. J. Oliversen, J. R. Espley, J. L. Joergensen, P. S. Joergensen, J. M. G. Merayo, et al. (2018). A New Model of Jupiter's Magnetic Field From Juno's First Nine Orbits. Geophys. Res. Lett., 45(6), 2590–2596. doi:10.1007/s11214-009-9621-7.
  • Connerney, J. E. P., Timmins, S., Oliversen, R. J., Espley, J. R., Joergensen, J. L., Kotsiaros, S., et al. (2021). A New Model of Jupiter's Magnetic Field at the Completion of Juno's Prime Mission. Journal of Geophysical Research: Planets, 126, e2021JE007055. doi:10.1029/2021JE007055.
  • Connerney, J. E. P., S. Timmins, M. Herceg and J. L. Joergensen (2020). A Jovian magnetodisc model for the Juno era. J. of Geophys. Res., 125, doi:10.1029/2020JA028138.
  • Davis, L. Jr, and E. Smith (1990). A Model of Saturn's Magnetic Field Based on All Available Data. J. Geophys. Res., 95, 15257–15261. doi:10.1029/JA095iA09p15257.
  • Herbert, F. (2009). Aurora and magnetic field of Uranus. J. Geophys. Res., 114, A11206, doi:10.1029/2009JA014394.
  • Hess, S. L. G. and P. Zarka (2011). Modeling the radio signature of the orbital parameters, rotation, and magnetic field of exoplanets, A&A. doi:10.1051/0004-6361/201116510.
  • Hess, S. L. G., B. Bonfond, F. Bagenal, and L. Lamy (2017). A Model of the Jovian Internal Field Derived from in-situ and Auroral Constraints, PRE8 Proceedings, Austrian Academy of Science. doi:10.1553/PRE8s157.
  • Hess, S. L. G., B. Bonfond, P. Zarka, and D. Grodent (2011). Model of the Jovian Magnetic Field Topology Constrained by the Io Auroral Emissions. J. Geophys. Res., 116(A5), 177. doi:10.1029/2010JA016262.
  • Reiners, A and G. Basri (2008). The moderate magnetic field of the flare star Proxima Centauri. A&A 489, L45–L48. doi:10.1051/0004-6361:200810491.