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Zonnestraling in Nederland - Knmi

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to various time scales. Successively the follow<strong>in</strong>g categories are presented:<br />

- the direct irradiance model for an hour or less;<br />

- direct irradiance models for a day or longer, accord<strong>in</strong>g to the algorithms developed by<br />

Revfeim and Page;<br />

- diffuse irradiance models for an hour or less, with the isotropic model and the algorithms<br />

accord<strong>in</strong>g to Hay, Gueymard and Perez as examples;<br />

- sky diffuse irradiance algorithms applicable to time <strong>in</strong>tegrals of a day or longer.<br />

Accord<strong>in</strong>g to the results of the IEA study and a separate test by Van den Br<strong>in</strong>k (1987), the<br />

algorithm accord<strong>in</strong>g to Perez is recommended to be used <strong>in</strong> the Netherlands to calculate<br />

diffuse radiation on <strong>in</strong>cl<strong>in</strong>ed surfaces.<br />

Section 5.3 gives the results of two years measurements of global radiation for 11 differently<br />

<strong>in</strong>cl<strong>in</strong>ed surfaces at Cabauw. The data are given <strong>in</strong> Table 5.2 for 24 days distributed<br />

across the year, and are displayed <strong>in</strong> Figure 5.5 for every month.<br />

S<strong>in</strong>ce no measurements of the spectral distribution of global radiation have been made <strong>in</strong><br />

the Netherlands, an algorithm developed by Slob (1985) has been used to adapt spectral data<br />

collected <strong>in</strong> Ukkel (Belgium) to Netherlands' circumstances. The results are given <strong>in</strong> Table<br />

5.5 for eight spectral bands bet ween 300 and 1000 nm.<br />

Chapter 5 concludes with section 5.5 on photometry, the lum<strong>in</strong>ous efficiency of the human<br />

eye and the conversion of radiation quantities <strong>in</strong> photometric quantities.<br />

Various appendices have been comb<strong>in</strong>ed <strong>in</strong> chapter 6. The first appendix, section 6.1, treats<br />

the different coord<strong>in</strong>ate systems for the position of the Sun <strong>in</strong> the sky, and gives conversion<br />

formulas as well as equations for the calculation of the Sun's decl<strong>in</strong>ation, elevation and<br />

azimuth.<br />

Local mean, national and Standard times are <strong>in</strong>troduced <strong>in</strong> appendix 6.2, with an emphasis<br />

on the history <strong>in</strong> the Netherlands. Also expressions for the equation of time and the length of<br />

the day are given.<br />

The third appendix, section 6.3, is devoted to radiometric and photometric units and their<br />

def<strong>in</strong>itions, and to the various radiometric scales that are or have been <strong>in</strong> use.<br />

With a list of symbols as the fourth appendix (section 6.4) chapter 6 is completed.<br />

153

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