Proposal ID | 080193 |
Title | Joining Juno in Exploring Jupiters Aurora |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0801930701 |
DOI | https://doi.org/10.5270/esa-9u5iens |
Principal Investigator, PI | Mr William Dunn |
Abstract | Over the next year, NASAs Juno spacecraft will fly through the magnetosphericregions that trigger Jupiters X-ray aurora. This provides aonce-in-a-generation opportunity to connect X-ray observations with simultaneousin-situ measurements of the magnetic and particle environment that produce thoseemissions. Given that Juno has no X-ray instrument, we propose to augment Junowith high spectral resolution XMM-Newton observations to answer 4 long-standingquestions: 1)What acceleration processes lead to Jupiters X-ray aurora? 2)Howdo in-situ conditions and particle fluxes relate to observed X-ray spectra? 3)IsJupiters X-ray aurora produced by solar wind or magnetosphere particles? 4)Howdo Jupiters X-rays relate to other wavebands? |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2017-06-18T19:45:25Z/2019-04-02T23:02:28Z |
Version | 17.56_20190403_1200 |
Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 | 2020-05-06T22:00:00Z |
Last Update | 2025-01-27 |
Keywords | "situ measurements", "juno spacecraft", "joining juno", "xray aurora", "trigger jupiter", "magnetospheric region", "solar wind", "situ conditions", "xray spectra", "particle fluxes relate", "xray instrument", "connect xray", "XMM-Newton", "exploring jupiter", "3is jupiter", "XMM", "magnetosphere particles", "augment juno" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Mr William Dunn, 2020, 'Joining Juno in Exploring Jupiter's Aurora', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-9u5iens |