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dc.contributor.authorPereira, N.
dc.contributor.authorBolsée, D.
dc.contributor.authorSperfeld, P.
dc.contributor.authorPape, S.
dc.contributor.authorSluse, D.
dc.contributor.authorCessateur, G.
dc.date2018
dc.date.accessioned2018-12-17T10:53:36Z
dc.date.available2018-12-17T10:53:36Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/7153
dc.descriptionThe near-infrared (NIR) part of the solar spectrum is of prime importance for solar physics and climatology, directly intervening in the Earth's radiation budget. Despite its major role, available solar spectral irradiance (SSI) NIR datasets, space-borne or ground-based, present discrepancies caused by instrumental or methodological reasons. We present new results obtained from the PYR-ILIOS SSI NIR ground-based campaign, which is a replication of the previous IRSPERAD campaign which took place in 2011 at the Izaña Atmospheric Observatory (IZO). We used the same instrument and primary calibration source of spectral irradiance. A new site was chosen for PYR-ILIOS: the Mauna Loa Observatory (MLO) in Hawaii (3397 m a.s.l.), approximately 1000 m higher than IZO. Relatively to IRSPERAD, the methodology of monitoring the traceability to the primary calibration source was improved. The results as well as a detailed error budget are presented. We demonstrate that the most recent results, from PYR-ILIOS and other space-borne and ground-based experiments, show an NIR SSI lower than the previous reference spectrum, ATLAS3, for wavelengths above 1.6 µm.
dc.languageeng
dc.titleMetrology of solar spectral irradiance at the top of the atmosphere in the near infrared measured at Mauna Loa Observatory: the PYR-ILIOS campaign
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.source.titleAtmospheric Measurement Techniques
dc.source.volume11
dc.source.issue12
dc.source.page6605-6615
Orfeo.peerreviewedYes
dc.identifier.doi10.5194/amt-11-6605-2018


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