A dataset provided by the European Space Agency

Name 084281
Title Is X-ray Aurora Produced by Magnetic Unloading?
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0842810501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0842810901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0842811001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0842811401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0842811501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0842811901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0842812001

DOI https://doi.org/10.5270/esa-[xxxxxxx]
Author Dr William Dunn
Description The combination of in-situ measurements from the Juno spacecraft and remote X-ray observations have provided tantalising clues towards the processes that permit rapidly-rotating magnetised bodies to produce X-ray aurora. Since Juno does not carry an X-ray instrument, AO 18 presents unique opportunities which may definitively identify the acceleration process-es that allow Jupiter to produce X-ray aurorae. We will:1. Identify whether magnetic unloading triggers the X-ray aurora by testing for correlations between X-ray auroral emissions and simultaneous Juno measurements of the plasma sheet. 2. Identify and quantify the auroral acceleration process-es at Jupiter by testing for correlations between X-ray spectral fluxes and in-situ electron and ion fluxes and multi-waveband observations.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, RGS1, RGS2
Temporal Coverage 2019-09-08T12:44:24Z/2020-04-10T13:18:27Z
Version 18.02_20200221_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 2021-04-22T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2021-04-22T00:00:00Z, 084281, 18.02_20200221_1200. https://doi.org/10.5270/esa-[xxxxxxx]