A dataset provided by the European Space Agency

Name: Probing Solar Wind Charge Exchange Emission From Earth's Magnetosheath
Published: 2007-06-16T00:00:00Z

Proposal ID	040253
Title	Probing Solar Wind Charge Exchange Emission From Earths Magnetosheath
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402530201
DOI	https://doi.org/10.5270/esa-yqs1tqo
Principal Investigator, PI	Dr Steve Snowden
Abstract	We propose to use the EPIC detectors to map out Solar Wind Charge Exchange(SWCX) emission from the upstream (relative to the solar wind) portion ofEarths magnetosheath. This is the region of maximum expected emission whichpeaks at the subsolar location. These observations will be used to investigateSWCX emission models which have never been tested for lack of appropriate data,study the interaction between the solar wind and the near-Earth environment in anew and novel manner, calibrate the contribution of this emission toobservations of more distant objects, and test the utility of using X-rayobservations to study global phenomena which currently can only be investigatedusing in situ measurements.
Publications	Observation of Solar Wind Charge Exchange Emission from Exospheric Material in and Outside Earths Magnetosheath 2008 September 25 \|Snowden S. L. Collier M. R. et al. \| ApJ \| 691-372 \| 2009 \| 2009ApJ...691..372S \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...691..372S The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens Nicola Romer A. Kathy et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies E. J. Romer A. Kathy et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley David B. Shelton Robin L. \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H X-rays from solar system objects \|Bhardwaj Anil Elsner Ronald F. et al. \| P&SS \| 55-1135 \| 2007 \| 2007P&SS...55.1135B \| http://ui.adsabs.harvard.edu/#abs/2007P&SS...55.1135B Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Sunyaev-Zeldovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao Weike Chen Chen et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X The Interaction of the Fermi Bubbles with the Milky Ways Hot Gas Halo \|Miller Matthew J. Bregman Joel N. \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M 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 The XMM Cluster Outskirts Project (X-COP): Physical conditions of Abell 2142 up to the virial radius \|Tchernin C. Eckert D. et al. \| A&A \| 595-42 \| 2016 \| 2016A&A...595A..42T \| http://ui.adsabs.harvard.edu/#abs/2016A&A...595A..42T Dark matter distribution in X-ray luminous galaxy clusters with Emergent Gravity \|Ettori S. Ghirardini V. et al. \| MNRAS \| 470-29 \| 2017 \| 2017MNRAS.470L..29E \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470L..29E Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas Konstantinos Reiprich Thomas H. \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M Reconstruction of the two-dimensional gravitational potential of galaxy clusters from X-ray and Sunyaev-Zeldovich measurements \|Tchernin C. Bartelmann M. et al. \| A&A \| 614-38 \| 2018 \| 2018A&A...614A..38T \| http://ui.adsabs.harvard.edu/#abs/2018A&A...614A..38T Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals \|Sibeck David G. Allen R. et al. \| SSRv \| 214-79 \| 2018 \| 2018SSRv..214...79S \| http://ui.adsabs.harvard.edu/#abs/2018SSRv..214...79S The XMM Cluster Survey: Present status and latest results \|Viana P. T. P. Mehrtens N. et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V The Physics of Galaxy Cluster Outskirts \|Walker Stephen Simionescu Aurora et al. \| SSRv \| 215-7 \| 2019 \| 2019SSRv..215....7W \| http://ui.adsabs.harvard.edu/#abs/2019SSRv..215....7W Testing emergent gravity on galaxy cluster scales \|Tamosiunas Andrius Bacon David et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood Devon L. Jeltema Tesla et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese A. Annis J. et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu Zhijie Huang Rui et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Yet another test of Radial Acceleration Relation for galaxy clusters \|Pradyumna S. Gupta Sajal et al. \| PDU \| 31-100765 \| 2021 \| 2021PDU....3100765P \| http://ui.adsabs.harvard.edu/#abs/2021PDU....3100765P The EXTraS project: Exploring the X-ray transient and variable sky \|De Luca A. Salvaterra R. et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D Graviton mass from X-COP galaxy clusters \|Piu00f3rkowska-Kurpas Aleksandra Cao Shuo \| JHEAp \| 33-37 \| 2022 \| 2022JHEAp..33...37P \| http://ui.adsabs.harvard.edu/#abs/2022JHEAp..33...37P Moffats modified gravity tested on X-COP galaxy clusters \|Harikumar Sreekanth Biesiada Marek \| EPJC \| 82-241 \| 2022 \| 2022EPJC...82..241H \| http://ui.adsabs.harvard.edu/#abs/2022EPJC...82..241H The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu Zhijie Koutroumpa Dimitra et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q The gravitational field of X-COP galaxy clusters \|Eckert D. Ettori S. et al. \| A&A \| 662-123 \| 2022 \| 2022A&A...662A.123E \| http://ui.adsabs.harvard.edu/#abs/2022A&A...662A.123E A test of galaxy cluster fundamental plane for the X-COP sample \|Pradyumna S. Desai Shantanu \| JCAP \| 1-58 \| 2022 \| 2022JCAP...01..058P \| http://ui.adsabs.harvard.edu/#abs/2022JCAP...01..058P A disturbing FABLE of mergers feedback turbulence and mass biases in simulated galaxy clusters \|Bennett Jake S. Sijacki Debora \| MNRAS \| 514-313 \| 2022 \| 2022MNRAS.514..313B \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.514..313B Constraints on dark matter self-interaction from the internal density profiles of X-COP galaxy clusters \|Eckert D. Ettori S. et al. \| A&A \| 666-41 \| 2022 \| 2022A&A...666A..41E \| http://ui.adsabs.harvard.edu/#abs/2022A&A...666A..41E Investigating the turbulent hot gas in X-COP galaxy clusters \|Dupourquu00e9 S. Clerc N. et al. \| A&A \| 673-91 \| 2023 \| 2023A&A...673A..91D \| http://ui.adsabs.harvard.edu/#abs/2023A&A...673A..91D Testing generalized scalar-tensor theories of gravity with clusters of galaxies \|Haridasu Balakrishna S. Karmakar Purnendu et al. \| PhRvD \| 107-124059 \| 2023 \| 2023PhRvD.107l4059H \| http://ui.adsabs.harvard.edu/#abs/2023PhRvD.107l4059H Three-dimensional Velocity Diagnostics to Constrain the Type Ia Origin of Tychos Supernova Remnant \|Uchida Hiroyuki Kasuga Tomoaki et al. \| ApJ \| 962-159 \| 2024 \| 2024ApJ...962..159U \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...962..159U 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	2006-06-04T13:31:53Z/2006-06-05T16:22:03Z
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	2007-06-16T00:00:00Z
Last Update	2025-01-27
Keywords	"situ measurements", "EPIC", "swcx emission models", "solar wind", "novel manner", "appropriate data", "epic detectors", "distant objects", "subsolar location", "global phenomena", "upstream relative"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Steve Snowden, 2007, 'Probing Solar Wind Charge Exchange Emission From Earth's Magnetosheath', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-yqs1tqo