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Auroral processes at the giant planets: energy deposition, emission mechanisms, morphology and spectra

Research output: Contribution to Journal/Magazine › Literature review › peer-review

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Auroral processes at the giant planets: energy deposition, emission mechanisms, morphology and spectra. / Badman, Sarah V.; Branduardi-Raymont, Graziella; Galand, Marina et al.
In: Space Science Reviews, Vol. 187, No. 1-4, 04.2015, p. 99-179.

Research output: Contribution to Journal/Magazine › Literature review › peer-review

Harvard

Badman, SV, Branduardi-Raymont, G, Galand, M, Hess, SLG, Krupp, N, Lamy, L, Melin, H & Tao, C 2015, 'Auroral processes at the giant planets: energy deposition, emission mechanisms, morphology and spectra', Space Science Reviews, vol. 187, no. 1-4, pp. 99-179. https://doi.org/10.1007/s11214-014-0042-x

APA

Badman, S. V., Branduardi-Raymont, G., Galand, M., Hess, S. L. G., Krupp, N., Lamy, L., Melin, H., & Tao, C. (2015). Auroral processes at the giant planets: energy deposition, emission mechanisms, morphology and spectra. Space Science Reviews, 187(1-4), 99-179. https://doi.org/10.1007/s11214-014-0042-x

Vancouver

Badman SV, Branduardi-Raymont G, Galand M, Hess SLG, Krupp N, Lamy L et al. Auroral processes at the giant planets: energy deposition, emission mechanisms, morphology and spectra. Space Science Reviews. 2015 Apr;187(1-4):99-179. Epub 2015 Apr 2. doi: 10.1007/s11214-014-0042-x

Author

Badman, Sarah V. ; Branduardi-Raymont, Graziella ; Galand, Marina et al. / Auroral processes at the giant planets : energy deposition, emission mechanisms, morphology and spectra. In: Space Science Reviews. 2015 ; Vol. 187, No. 1-4. pp. 99-179.

Bibtex

@article{6cc4f1bc51864e95b61f67057d120365,
title = "Auroral processes at the giant planets: energy deposition, emission mechanisms, morphology and spectra",
abstract = "The ionospheric response to auroral precipitation at the giant planets is reviewed, using models and observations. The emission processes for aurorae at radio, infrared, visible, ultraviolet, and X-ray wavelengths are described, and exemplified using ground- and space-based observations. Comparisons between the emissions at different wavelengths are made, where possible, and interpreted in terms of precipitating particle characteristics or atmospheric conditions. Finally, the spatial distributions and dynamics of the various components of the aurorae (moon footprints, low-latitude, main oval, polar) are related to magnetospheric processes and boundaries, using theory, in situ, and remote observations, with the aim of distinguishing between those related to internally-driven dynamics, and those related to the solar wind interaction.",
keywords = "Giant planet, Aurora, Magnetodisk, HUBBLE-SPACE-TELESCOPE, X-RAY-EMISSION, SATURN KILOMETRIC RADIATION, DECAMETRIC RADIO-EMISSION, PLASMA-WAVE OBSERVATIONS, IONOSPHERIC PEDERSEN CONDUCTIVITY, JUPITERS MIDDLE MAGNETOSPHERE, COUPLED ROTATIONAL-DYNAMICS, CASSINI UVIS OBSERVATIONS, MAGNETIC-SECTOR STRUCTURE",
author = "Badman, {Sarah V.} and Graziella Branduardi-Raymont and Marina Galand and Hess, {Sebastien L. G.} and Norbert Krupp and Laurent Lamy and Henrik Melin and Chihiro Tao",
note = "Date of Acceptance: 17/03/2014",
year = "2015",
month = apr,
doi = "10.1007/s11214-014-0042-x",
language = "English",
volume = "187",
pages = "99--179",
journal = "Space Science Reviews",
issn = "0038-6308",
publisher = "Springer Netherlands",
number = "1-4",

}

RIS

TY - JOUR

T1 - Auroral processes at the giant planets

T2 - energy deposition, emission mechanisms, morphology and spectra

AU - Badman, Sarah V.

AU - Branduardi-Raymont, Graziella

AU - Galand, Marina

AU - Hess, Sebastien L. G.

AU - Krupp, Norbert

AU - Lamy, Laurent

AU - Melin, Henrik

AU - Tao, Chihiro

N1 - Date of Acceptance: 17/03/2014

PY - 2015/4

Y1 - 2015/4

N2 - The ionospheric response to auroral precipitation at the giant planets is reviewed, using models and observations. The emission processes for aurorae at radio, infrared, visible, ultraviolet, and X-ray wavelengths are described, and exemplified using ground- and space-based observations. Comparisons between the emissions at different wavelengths are made, where possible, and interpreted in terms of precipitating particle characteristics or atmospheric conditions. Finally, the spatial distributions and dynamics of the various components of the aurorae (moon footprints, low-latitude, main oval, polar) are related to magnetospheric processes and boundaries, using theory, in situ, and remote observations, with the aim of distinguishing between those related to internally-driven dynamics, and those related to the solar wind interaction.

AB - The ionospheric response to auroral precipitation at the giant planets is reviewed, using models and observations. The emission processes for aurorae at radio, infrared, visible, ultraviolet, and X-ray wavelengths are described, and exemplified using ground- and space-based observations. Comparisons between the emissions at different wavelengths are made, where possible, and interpreted in terms of precipitating particle characteristics or atmospheric conditions. Finally, the spatial distributions and dynamics of the various components of the aurorae (moon footprints, low-latitude, main oval, polar) are related to magnetospheric processes and boundaries, using theory, in situ, and remote observations, with the aim of distinguishing between those related to internally-driven dynamics, and those related to the solar wind interaction.

KW - Giant planet

KW - Aurora

KW - Magnetodisk

KW - HUBBLE-SPACE-TELESCOPE

KW - X-RAY-EMISSION

KW - SATURN KILOMETRIC RADIATION

KW - DECAMETRIC RADIO-EMISSION

KW - PLASMA-WAVE OBSERVATIONS

KW - IONOSPHERIC PEDERSEN CONDUCTIVITY

KW - JUPITERS MIDDLE MAGNETOSPHERE

KW - COUPLED ROTATIONAL-DYNAMICS

KW - CASSINI UVIS OBSERVATIONS

KW - MAGNETIC-SECTOR STRUCTURE

U2 - 10.1007/s11214-014-0042-x

DO - 10.1007/s11214-014-0042-x

M3 - Literature review

VL - 187

SP - 99

EP - 179

JO - Space Science Reviews

JF - Space Science Reviews

SN - 0038-6308

IS - 1-4

ER -