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Disc-averaged radial-velocity variations and unsigned magnetic flux of the Sun from SDO/HMI images

dc.contributor.authorHaywood, R
dc.contributor.authorMilbourne, TW
dc.contributor.authorSaar, SH
dc.contributor.authorMortier, A
dc.contributor.authorPhillips, D
dc.contributor.authorCharbonneau, D
dc.contributor.authorCollier Cameron, A
dc.contributor.authorCegla, HM
dc.contributor.authorMeunier, N
dc.contributor.authorPalumbo III, ML
dc.date.accessioned2022-07-21T07:58:40Z
dc.date.issued2022-07-21
dc.date.updated2022-07-20T12:57:23Z
dc.description.abstractThis is the dataset used for the Haywood et al. (2022) article "Unsigned magnetic flux as a proxy for radial-velocity variations in Sun-like stars" published in The Astrophysical Journal.en_GB
dc.description.sponsorshipScience and Technology Facilities Council (STFC)en_GB
dc.description.sponsorshipScience and Technology Facilities Council (STFC)en_GB
dc.description.sponsorshipNASAen_GB
dc.description.sponsorshipNASAen_GB
dc.description.sponsorshipNASAen_GB
dc.format.csv
dc.identifier.doi10.24378/exe.4086
dc.identifier.grantnumberST/V004735/1en_GB
dc.identifier.grantnumberST/R000824/1en_GB
dc.identifier.grantnumber1581003en_GB
dc.identifier.grantnumberNNX16AD42Gen_GB
dc.identifier.grantnumberNNX16AB79Gen_GB
dc.identifier.urihttp://hdl.handle.net/10871/130309
dc.identifierORCID: 0000-0001-9140-3574 (Haywood, Raphaelle)
dc.language.isoenen_GB
dc.publisherUniversity of Exeteren_GB
dc.relation.urlhttp://hdl.handle.net/10871/130655en_GB
dc.rightsCC BY 4.0en_GB
dc.subjectSolar cycleen_GB
dc.subjectActive sunen_GB
dc.subjectQuiet sunen_GB
dc.subjectSunspotsen_GB
dc.subjectSunspotsen_GB
dc.subjectExoplanet detection methodsen_GB
dc.subjectRadial velocityen_GB
dc.subjectAstronomy data analysisen_GB
dc.titleDisc-averaged radial-velocity variations and unsigned magnetic flux of the Sun from SDO/HMI imagesen_GB
dc.typeDataseten_GB
dc.date.available2022-07-21T07:58:40Z
dc.descriptionWe estimate disc-averaged radial-velocity variations, unsigned magnetic flux and active-region filling factors of the Sun using spatially resolved images from SDO/HMI between 2010 and 2018. We include overlapping S-index data and total solar irradiance data. Everything is described in detail in the associated paper: Unsigned magnetic flux as a proxy for radial-velocity variations in Sun-like stars, Haywood et al., 2022, in press at ApJ.en_GB
dc.descriptionThe article associated with this dataset is available in ORE at: http://hdl.handle.net/10871/130655en_GB
dc.rights.urihttps://creativecommons.org/licenses/by/4.0en_GB
pubs.funder-ackownledgementYes
pubs.date-of-acceptance2022-06-27
rioxxterms.versionNAen_GB
rioxxterms.licenseref.startdate2022-07-21
rioxxterms.typeOtheren_GB
refterms.dateFOA2022-07-21T07:59:37Z


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CC BY 4.0
Except where otherwise noted, this item's licence is described as CC BY 4.0