A dataset provided by the European Space Agency

Name: How Does the Solar Wind Drive Jupiter.s X-ray AuroraquestionMark
Published: 2017-06-15T22:00:00Z

Proposal ID	078183
Title	How Does the Solar Wind Drive Jupiter.s X-ray Aurora?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0781830301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0781830601
DOI	https://doi.org/10.5270/esa-68ghekv
Principal Investigator, PI	Mr William Dunn
Abstract	The Juno spacecraft.s approach to Jupiter presents the opportunity to utilisesimultaneous remote X-ray and in situ observations to address three fundamentalopen questions in X-ray and magnetospheric physics: 1) What processes atJupiter.s magnetopause (the source for ions that generate Jupiter.s soft X-rayaurora) drive the X-ray emission? 2) What is the nature of the globalinteraction between Jupiter and the solar wind? 3) How does the X-ray emissionconnect with UV and Radio emissions? To address these long-standing questions,we propose XMM-Newton EPIC and RGS observations of Jupiter during May and June2016 when Juno is in the solar wind and crossing the magnetopause. The nextopportunity to conduct observations like these will not be until 2030.
Publications	The independent pulsations of Jupiter.s northern and southern X-ray auroras \|Dunn, W. R., Branduardi-Raymont, G., et al. \| NatAs \| 1-758 \| 2017 \| 2017NatAs...1..758D \| http://ui.adsabs.harvard.edu/#abs/2017NatAs...1..758D Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Jupiter.s equatorial X-ray emissions over two solar cycles \|Wibisono, A. D., Branduardi-Raymont, G., et al. \| MNRAS \| 521-5596 \| 2023 \| 2023MNRAS.521.5596W \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.521.5596W From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, RGS1, RGS2
Temporal Coverage	2016-05-18T12:45:00Z/2016-05-24T22:32:20Z
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	2017-06-15T22:00:00Z
Keywords	"xmm newton epic", "xray emission connect", "global interaction", "XMM", "juno spacecraft", "remote xray", "xray aurora ?.", "radio emissions", "XMM-Newton", "xray emission", "EPIC", "solar wind", "magnetospheric physics"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr William Dunn, 2017, 'How Does the Solar Wind Drive Jupiter.s X-ray AuroraquestionMark', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-68ghekv