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Which effective solar zenith angles to use for hourly irradiation measurements?

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HAL Id: hal-01197035

https://hal-mines-paristech.archives-ouvertes.fr/hal-01197035

Submitted on 21 Sep 2015

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Which effective solar zenith angles to use for hourly irradiation measurements?

Philippe Blanc, Lucien Wald

To cite this version:

Philippe Blanc, Lucien Wald. Which effective solar zenith angles to use for hourly irradiation measure- ments?. 15th EMS / 12th ECAM, EMS European Meteorological Society, Sep 2015, Sofia, Bulgaria.

pp.318. �hal-01197035�

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EMS Annual Meeting Abstracts Vol. 12, EMS2015-318, 2015 15th EMS / 12th ECAM

© Author(s) 2015. CC Attribution 3.0 License.

E M S

A n n ua l M ee ting on Applications of Meteorology

E CAM

y European Conference

Which effective solar zenith angles to use for hourly irradiation measurements?

Philippe Blanc and Lucien Wald

MINES ParisTech - PSL Research University, Sophia Antipolis cedex, France (lucien.wald@mines-paristech.fr)

Time-series of in situ or satellite-derived measurements of hourly irradiation on horizontal surface are increasingly

available. In many cases, such data are input to numerical procedures that can be performed only if a solar zenith

angle can be associated to each measurement. Currently, only time stamp is given for each measurement; no angle

is given. The solar zenith angle is greatly varying within 1 h and cannot be considered as constant. In this context,

there is a practical request from companies, academics, researchers...: what is the best practice for computing this

angle? The work presented here compares the performances of several existing practices and makes recommen-

dations keeping in mind the practical aspects faced by practitioners, companies, academics, researchers... High-

quality 1 min measurements of global, diffuse and direct collected by the BSRN station in Carpentras in France,

are aggregated to yield hourly irradiation, and used to assess the performances. It is found that several practices

may be used to compute in a satisfactory way the effective solar zenith angle. The most accurate results are ob-

tained if one may obtain corresponding irradiation values that should be observed under clear-sky conditions. The

McClear Service available at http://www.soda-pro.com is one Web service providing such estimates of cloud-free

irradiation for several summarizations, from 1 min to 1 month. If one may not obtain such cloud-free estimates,

then the most accurate results are obtained from using irradiation at the top of atmosphere. Performances show a

tendency to decrease during sunrise and sunset hours.

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