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dc.contributor.authorSmith, Randall
dc.contributor.authorHahn, Michael
dc.contributor.authorRaymond, John
dc.contributor.authorKallman, T
dc.contributor.authorBallance, C P
dc.contributor.authorPolito, Vanessa
dc.contributor.authorDel Zanna, Giulio
dc.contributor.authorGu, Liyi
dc.contributor.authorHell, Natalie
dc.contributor.authorCumbee, Renata
dc.contributor.authorBetancourt-Martinez, Gabriele
dc.contributor.authorCostantini, Elisa
dc.contributor.authorCorrales, Lia
dc.date.accessioned2020-04-09T16:02:19Z
dc.date.available2020-04-09T16:02:19Z
dc.date.issued2020-04-06
dc.date.submitted2019-10-23
dc.identifier.citationJournal of Physics B: Atomic, Molecular and Optical Physics, volume 53, issue 9, page 092001
dc.identifier.issn0953-4075
dc.identifier.otherjpbab69aa
dc.identifier.otherab69aa
dc.identifier.otherjphysb-105714.r1
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/304231
dc.description.abstractAbstract: Cosmic EUV/x-ray spectroscopists, including both solar and astrophysical analysts, have a wide range of high-resolution and high-sensitivity tools in use and a number of new facilities in development for launch. As this bandpass requires placing the spectrometer beyond the Earth’s atmosphere, each mission represents a major investment by a national space agency such as NASA, ESA, or JAXA, and more typically a collaboration between two or three. In general justifying new mission requires an improvement in capabilities of at least an order of magnitude, but the sensitivity of these existing missions are already taxing existing atomic data quantity and accuracy. This roadmap reviews the existing missions, showing how in a number of areas atomic data limits the science that can be performed. The missions that will be launched in the coming Decade will without doubt require both more and improved measurements of wavelengths and rates, along with theoretical calculations of collisional and radiative cross sections for a wide range of processes.
dc.languageen
dc.publisherIOP Publishing
dc.rightsAttribution 3.0 Unported (CC BY 3.0)en
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/en
dc.subjectRoadmap
dc.subjectcosmic EUV
dc.subjectx-ray spectroscopy
dc.subjectastrophysics
dc.subjectatomic data
dc.titleRoadmap on cosmic EUV and x-ray spectroscopy
dc.typeArticle
dc.date.updated2020-04-09T16:02:19Z
dc.identifier.doi10.17863/CAM.51311
dcterms.dateAccepted2020-01-09
rioxxterms.versionofrecord10.1088/1361-6455/ab69aa
rioxxterms.versionVoR
rioxxterms.licenseref.urihttp://creativecommons.org/licenses/by/3.0/
dc.contributor.orcidSmith, Randall [0000-0003-4284-4167]
dc.contributor.orcidHell, Natalie [0000-0003-3057-1536]
dc.identifier.eissn1361-6455
pubs.funder-project-idNational Aeronautics and Space Administration (#80NSSC18K0409)


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Attribution 3.0 Unported (CC BY 3.0)
Except where otherwise noted, this item's licence is described as Attribution 3.0 Unported (CC BY 3.0)