A dataset provided by the European Space Agency

Name 086195
Title Are Jupiter s Pulses Signatures of Global or Local Wave-Particle Interactions
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0861950201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0861950231
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0861950232
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0861950233
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0861950234
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0861950601

DOI https://doi.org/10.57780/esa-g5gt7tp
Author Dr William Dunn
Description Jupiter is the local-space archetype for many astrophysical bodies which cannot
be visited in-situ such as exoplanets, pulsars and brown dwarfs. Over the last 2
years, simultaneous Juno and XMM-Newton (XMM) Jupiter observations have provided
a paradigm-shift in our understanding of how planets produce X-rays. Since Juno
has no X-ray instrument, this rich array of discoveries would not have been
possible without XMM. Significantly, Juno and XMM have revealed that Jupiter s
X-ray aurora is produced when ion cyclotron waves in Jupiter.s magnetosphere
inject energetic ions into the pole. So far, Juno has only explored Jupiter.s
dawn-midnight sector, but for the remainder of its mission (end July 2021), it
will explore the midnight-dusk sector. [see pdf for complete abstract]
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, RGS1, RGS2
Temporal Coverage 2020-10-31T08:30:12Z/2020-11-01T23:15:15Z
Version 21.23_20231215_1101
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2021-12-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr William Dunn, 2021, 086195, 21.23_20231215_1101, European Space Agency, https://doi.org/10.57780/esa-g5gt7tp