A dataset provided by the European Space Agency

Name 030548
Title A Coordinated XMM-Newton--Cassini Study of the Saturnian System
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305480101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305480201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305480301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305480401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305480501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305480601

DOI https://doi.org/10.5270/esa-w1louxa
Author Dr Graziella Branduardi-Raymont
Description We propose a coordinated observing campaign to study the X-ray emissions from
the Saturnian system with XMM-Newton (4 observations of 39 ks each), while
making in-situ particle and field measurements, and remote sensing observations
at UV, visible and IR wavelengths, with Cassini. Our aim is to investigate the
Chandra detection of strong variability in Saturn.s X-ray emission from both the
planetary disk and the auroral zones, and the faint X-ray emission from the
rings. Probable candidates for the variability are solar wind, solar
irradiation, and magnetospheric plasma. This unique coordinated campaign of
XMM-Newton and Cassini observations will provide crucial data for understanding
the physics of X-ray production at Saturn and its rings.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, RGS1, RGS2
Temporal Coverage 2005-04-21T22:01:32Z/2005-10-29T13:42:39Z
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 2008-06-27T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Graziella Branduardi-Raymont, 2008, 030548, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-w1louxa