Temperature and composition disturbances in the southern auroral region of Jupiter revealed by JWST/MIRI
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2024
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| author | Rodríguez-Ovalle, Pablo Fouchet, Thierry Guerlet, Sandrine Cavalié, Thibault Hue, Vincent López-Puertas, Manuel Lellouch, Emmanuel Sinclair, James A. de Pater, Imke Fletcher, Leigh N. Wong, Michael H. Harkett, Jake Orton, Glenn S. Hueso, Ricardo Sánchez-Lavega, Agustín Stallard, Tom S. Bockelee-Morvan, Dominique King, Oliver Roman, Michael T. Melin, Henrik |
| author_facet | Rodríguez-Ovalle, Pablo Fouchet, Thierry Guerlet, Sandrine Cavalié, Thibault Hue, Vincent López-Puertas, Manuel Lellouch, Emmanuel Sinclair, James A. de Pater, Imke Fletcher, Leigh N. Wong, Michael H. Harkett, Jake Orton, Glenn S. Hueso, Ricardo Sánchez-Lavega, Agustín Stallard, Tom S. Bockelee-Morvan, Dominique King, Oliver Roman, Michael T. Melin, Henrik |
| contents | Jupiters south polar region was observed by JWST Mid Infrared Instrument in December 2022. We used the Medium Resolution Spectrometer mode to provide new information about Jupiters South Polar stratosphere. The southern auroral region was visible and influenced the atmosphere in several ways. 1: In the interior of the southern auroral oval, we retrieved peak temperatures at two distinct pressure levels near 0.01 and 1 mbar, with warmer temperatures with respect to non auroral regions of 12 pm 2 K and 37 pm 4 K respectively. A cold polar vortex is centered at 65S at 10 mbar. 2: We found that the homopause is elevated to 590+25-118 km above the 1-bar pressure level inside the auroral oval compared to 460+60-50 km at neighboring latitudes and with an upper altitude of 350 km in regions not affected by auroral precipitation. 3: The retrieved abundance of C2H2 shows an increase within the auroral oval, and it exhibits high abundances throughout the polar region. The retrieved abundance of C2H6 increases towards the pole, without being localized in the auroral oval, in contrast with previous analysis. We determined that the warming at 0.01 mbar and the elevated homopause might be caused by the flux of charged particles depositing their energy in the South Polar Region. The 1 mbar hotspot may arise from adiabatic heating resulting from auroral driven downwelling. The cold region at 10 mbar may be caused by radiative cooling by stratospheric aerosols. The differences in spatial distribution seem to indicate that the hydrocarbons analyzed are affected differently by auroral precipitation. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_08133 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Temperature and composition disturbances in the southern auroral region of Jupiter revealed by JWST/MIRI Rodríguez-Ovalle, Pablo Fouchet, Thierry Guerlet, Sandrine Cavalié, Thibault Hue, Vincent López-Puertas, Manuel Lellouch, Emmanuel Sinclair, James A. de Pater, Imke Fletcher, Leigh N. Wong, Michael H. Harkett, Jake Orton, Glenn S. Hueso, Ricardo Sánchez-Lavega, Agustín Stallard, Tom S. Bockelee-Morvan, Dominique King, Oliver Roman, Michael T. Melin, Henrik Earth and Planetary Astrophysics Jupiters south polar region was observed by JWST Mid Infrared Instrument in December 2022. We used the Medium Resolution Spectrometer mode to provide new information about Jupiters South Polar stratosphere. The southern auroral region was visible and influenced the atmosphere in several ways. 1: In the interior of the southern auroral oval, we retrieved peak temperatures at two distinct pressure levels near 0.01 and 1 mbar, with warmer temperatures with respect to non auroral regions of 12 pm 2 K and 37 pm 4 K respectively. A cold polar vortex is centered at 65S at 10 mbar. 2: We found that the homopause is elevated to 590+25-118 km above the 1-bar pressure level inside the auroral oval compared to 460+60-50 km at neighboring latitudes and with an upper altitude of 350 km in regions not affected by auroral precipitation. 3: The retrieved abundance of C2H2 shows an increase within the auroral oval, and it exhibits high abundances throughout the polar region. The retrieved abundance of C2H6 increases towards the pole, without being localized in the auroral oval, in contrast with previous analysis. We determined that the warming at 0.01 mbar and the elevated homopause might be caused by the flux of charged particles depositing their energy in the South Polar Region. The 1 mbar hotspot may arise from adiabatic heating resulting from auroral driven downwelling. The cold region at 10 mbar may be caused by radiative cooling by stratospheric aerosols. The differences in spatial distribution seem to indicate that the hydrocarbons analyzed are affected differently by auroral precipitation. |
| title | Temperature and composition disturbances in the southern auroral region of Jupiter revealed by JWST/MIRI |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2406.08133 |