Observation and origin of non-thermal hard X-rays from Jupiter
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| Autores principales: | , , , , , , , , , , , , |
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| Formato: | Preprint |
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2022
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| author | Mori, Kaya Hailey, Charles Bridges, Gabriel Mandel, Shifra Garvin, Amani Grefenstette, Brian Dunn, William Hord, Benjamin J. Branduardi-Raymont, Graziella Clarke, John Jackman, Caitriona Nynka, Melania Ray, Licia |
| author_facet | Mori, Kaya Hailey, Charles Bridges, Gabriel Mandel, Shifra Garvin, Amani Grefenstette, Brian Dunn, William Hord, Benjamin J. Branduardi-Raymont, Graziella Clarke, John Jackman, Caitriona Nynka, Melania Ray, Licia |
| contents | Electrons accelerated on Earth by a rich variety of wave scattering or stochastic processes generate hard non-thermal X-ray bremsstrahlung up to >~ 1 MeV and power Earth's various types of aurorae. Although Jupiter's magnetic field is an order of magnitude larger than Earth's, space-based telescopes have previously detected X-rays only up to ~7 keV. On the basis of theoretical models of the Jovian auroral X-ray production, X-ray emission in the ~2-7 keV band has been interpreted as thermal (arising from electrons characterized by a Maxwell-Boltzmann distribution) bremsstrahlung. Here we report the observation of hard X-rays in the 8-20 keV band from the Jovian aurorae, obtained with the NuSTAR X-ray observatory. The X-rays fit to a flat power-law model with slope 0.60+/-0.22 - a spectral signature of non-thermal, hard X-ray bremsstrahlung. We determine the electron flux and spectral shape in the keV to MeV energy range using coeval in situ measurements by the Juno spacecraft's JADE and JEDI instruments. Jovian electron spectra of the form we observe have previously been interpreted to arise in stochastic acceleration, rather than coherent acceleration by electric fields. We reproduce the X-ray spectral shape and approximate flux observed by NuSTAR, and explain the non-detection of hard X-rays by Ulysses, by simulating the non-thermal population of electrons undergoing precipitating electron energy loss, secondary electron generation and bremsstrahlung emission in a model Jovian atmosphere. The results highlight the similarities between the processes generating hard X-ray auroras on Earth and Jupiter, which may be occurring on Saturn, too. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2202_08347 |
| institution | arXiv |
| publishDate | 2022 |
| record_format | arxiv |
| spellingShingle | Observation and origin of non-thermal hard X-rays from Jupiter Mori, Kaya Hailey, Charles Bridges, Gabriel Mandel, Shifra Garvin, Amani Grefenstette, Brian Dunn, William Hord, Benjamin J. Branduardi-Raymont, Graziella Clarke, John Jackman, Caitriona Nynka, Melania Ray, Licia Earth and Planetary Astrophysics High Energy Astrophysical Phenomena Electrons accelerated on Earth by a rich variety of wave scattering or stochastic processes generate hard non-thermal X-ray bremsstrahlung up to >~ 1 MeV and power Earth's various types of aurorae. Although Jupiter's magnetic field is an order of magnitude larger than Earth's, space-based telescopes have previously detected X-rays only up to ~7 keV. On the basis of theoretical models of the Jovian auroral X-ray production, X-ray emission in the ~2-7 keV band has been interpreted as thermal (arising from electrons characterized by a Maxwell-Boltzmann distribution) bremsstrahlung. Here we report the observation of hard X-rays in the 8-20 keV band from the Jovian aurorae, obtained with the NuSTAR X-ray observatory. The X-rays fit to a flat power-law model with slope 0.60+/-0.22 - a spectral signature of non-thermal, hard X-ray bremsstrahlung. We determine the electron flux and spectral shape in the keV to MeV energy range using coeval in situ measurements by the Juno spacecraft's JADE and JEDI instruments. Jovian electron spectra of the form we observe have previously been interpreted to arise in stochastic acceleration, rather than coherent acceleration by electric fields. We reproduce the X-ray spectral shape and approximate flux observed by NuSTAR, and explain the non-detection of hard X-rays by Ulysses, by simulating the non-thermal population of electrons undergoing precipitating electron energy loss, secondary electron generation and bremsstrahlung emission in a model Jovian atmosphere. The results highlight the similarities between the processes generating hard X-ray auroras on Earth and Jupiter, which may be occurring on Saturn, too. |
| title | Observation and origin of non-thermal hard X-rays from Jupiter |
| topic | Earth and Planetary Astrophysics High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2202.08347 |