A dataset provided by the European Space Agency

Name: Plasma in the Jovian magnetosphere: X-ray+EUV study of aurora &amp; Io plasma torus
Published: 2015-05-07T22:00:00Z

Proposal ID	072896
Title	Plasma in the Jovian magnetosphere: X-ray+EUV study of aurora & Io plasma torus
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728960601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728960631 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728960632 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728960801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728960831 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728960832
DOI	https://doi.org/10.5270/esa-n0kwoxx
Principal Investigator, PI	Dr Ralph Kraft
Abstract	We propose 4x40 ks Chandra/HRC-I and 2x40 ks XMM-Newton observations of theJovian aurora and Io plasma torus in conjunction with the Japanese SPRINT-Asatellite. SPRINT-A will continuously observe Jupiter from Dec 2013 to Apr 2014,making sensitive EUV spectroscopic observations of the aurora and IPT. We willcorrelate variations in the X-ray flux from the aurora and IPT with changes inthe EUV flux observed by SPRINT-A and with the properties of the solar wind. Wewill conclusively resolve the puzzle of the origin of the Jovian X-ray emissionand determine if the precipitating particles originate from Io or from the solarwind.
Publications	The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F 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 Suzaku observations of Jovian diffuse hard X-ray emission \|Numazawa, Masaki, Ezoe, Yuichiro, et al. \| PASJ \| 73-894 \| 2021 \| 2021PASJ...73..894N \| http://ui.adsabs.harvard.edu/#abs/2021PASJ...73..894N 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 The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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, OM, RGS1, RGS2
Temporal Coverage	2014-04-15T20:55:00Z/2014-04-20T14:59:02Z
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	2015-05-07T22:00:00Z
Keywords	"precipitating particles", "correlate variations", "XMM", "apr 2014", "dec 2013", "conclusively resolve", "xray flux", "jovian aurora", "4x40 chandra", "sensitive euv spectroscopic", "euv flux", "io plasma torus", "XMM-Newton", "jovian magnetosphere", "japanese sprint", "solar wind", "jovian xray emission", "2x40 xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ralph Kraft, 2015, 'Plasma in the Jovian magnetosphere: X-ray+EUV study of aurora & Io plasma torus', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-n0kwoxx