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dc.contributor.authorVon Savigny, C.
dc.contributor.authorEichmann, K.-U.
dc.contributor.authorRobert, C.E.
dc.contributor.authorBurrows, J.P.
dc.contributor.authorWeber, M.
dc.date2012
dc.date.accessioned2016-03-29T10:07:35Z
dc.date.available2016-03-29T10:07:35Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/2965
dc.descriptionNight-time observations of OH(3–1) rotational temperatures with SCIAMACHY (SCanning Imaging Absorption spectroMeter for Atmospheric CHartographY) on Envisat are used to study the sensitivity of equatorial mesopause temperatures to the 27-day solar forcing. Fourier and cross-correlation analysis are first used to demonstrate the presence of a solar-driven 27-day cycle in OH rotational temperatures. The temperature sensitivity to solar forcing is quantitatively evaluated based on a superposed epoch analysis that also demonstrates that the solar signal in the OH temperature time series is significant at the 99.9 % confidence level. The most remarkable result is that the temperature sensitivity to solar forcing in terms of the 27-day solar cycle (βF10.7= 2.46 (±0.93) K/(100 sfu)) agrees within uncertainties with the majority of published sensitivity values in terms of the 11-year solar cycle. This implies that the same underlying physical mechanism drives the mesopause temperature response to solar variability at both the 27-day and the 11-year time scale.
dc.languageeng
dc.titleSensitivity of equatorial mesopause temperatures to the 27-day solar cycle
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleGeophysical Research Letters
dc.source.volume39
dc.source.issue21
dc.source.pageL21804
Orfeo.peerreviewedYes
dc.identifier.doi10.1029/2012GL053563
dc.identifier.scopus2-s2.0-84868613787


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