A dataset provided by the European Space Agency

Name 072896
Title Plasma in the Jovian magnetosphere: X-ray+EUV study of aurora & Io plasma torus
URL

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
Author Dr Ralph Kraft
Description We propose 4x40 ks Chandra-HRC-I and 2x40 ks XMM-Newton observations of the Jovian aurora and Io plasma torus in conjunction with the Japanese SPRINT-A satellite. SPRINT-A will continuously observe Jupiter from Dec 2013 to Apr 2014, making sensitive EUV spectroscopic observations of the aurora and IPT. We will correlate variations in the X-ray flux from the aurora and IPT with changes in the EUV flux observed by SPRINT-A and with the properties of the solar wind. We will conclusively resolve the puzzle of the origin of the Jovian X-ray emission and determine if the precipitating particles originate from Io or from the solar wind.
Publication No observations found associated with the current proposal
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 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 2015-05-07T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015-05-07T22:00:00Z, 072896, 17.56_20190403_1200. https://doi.org/10.5270/esa-n0kwoxx