| Proposal ID | 080376 |
| Title | In-situ measurements of the heavy ion content of the elusive polar solar wind |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803760301 |
| DOI | https://doi.org/10.5270/esa-duan0hw |
| Principal Investigator, PI | Dr Konrad Dennerl |
| Abstract | We propose to investigate the heavy ion content of the elusive polar solar windby observing the cometary X-ray emission which results from charge exchangebetween solar wind heavy ions and cometary neutrals, thus providing in-situinformation. We will utilize the favorable opportunity that during AO-16 we willapproach solar minimum, where the polar wind will have expanded to lowerlatitudes, and that a bright comet, C/2015 V2, will be continuously observablefor XMM from -2 deg to -32 deg ecliptic latitude. This observation is perfectlytailored to XMM, as it makes full use of its high soft X-ray sensitivity, itsspectral, temporal, and spatial resolution, its full field of view, and of allsix (PN, MOS1, MOS2, RGS1, RGS2, OM) of its scientific instruments. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2017-07-13T07:24:09Z/2017-09-18T03:43:32Z |
| Version | 20.10_20230417_1156 |
| 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 | 2018-10-13T22:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "situ measurements", "polar wind", "bright comet", "cometary xray emission", "deg ecliptic latitude", "soft xray sensitivity", "continuously observable", "approach solar minimum", "2015 v2", "cometary neutrals", "situ information", "charge exchange", "XMM", "heavy ion content", "lower latitudes", "scientific instruments", "perfectly tailored", "spatial resolution" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Konrad Dennerl, 2018, 'In-situ measurements of the heavy ion content of the elusive polar solar wind', 20.10_20230417_1156, European Space Agency, https://doi.org/10.5270/esa-duan0hw |