1986
DOI: 10.1016/0038-092x(86)90078-2
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An analytic function for the flux density due to sunlight reflected from a heliostat

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Cited by 96 publications
(39 citation statements)
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“…In a recent comparison [39] between the HFLCAL [19][20] and UNIZAR [40] models of the energy image sent by a single heliostat, which tests both models against actual spots measured for first generation heliostats, it is concluded that the HFLCAL model is much simpler and slightly more accurate than the UNIZAR model.…”
Section: Intercept Factormentioning
confidence: 98%
See 1 more Smart Citation
“…In a recent comparison [39] between the HFLCAL [19][20] and UNIZAR [40] models of the energy image sent by a single heliostat, which tests both models against actual spots measured for first generation heliostats, it is concluded that the HFLCAL model is much simpler and slightly more accurate than the UNIZAR model.…”
Section: Intercept Factormentioning
confidence: 98%
“…where s tot is the total standard deviation result measured on the image plane [40], i.e., a plane normal to the unit vector t, and with coordinates (x 0 , y 0 ).…”
Section: Intercept Factormentioning
confidence: 99%
“…where t denotes the time instant, Π t is the outlet thermal power collected at time t, calculated as in [5,12,16,17,18], and γ 1 is a constant that mesures the fixed energy losses related with the whole system.…”
Section: Functionsmentioning
confidence: 99%
“…For instance, if we consider 5, 9 or 13 different hours to compute the daily thermal energy, for different fixed days we obtain the results shown in The annual thermal energy collected is computed using an algorithm similar to NSPOC procedure, that is described in Crespo & Ramos (2009). We refer the reader to Biggs & Vittitoe (1976); Collado & Turégano (1986, 1989; Stine & Harrigan (2001), for further details.…”
Section: Functionsmentioning
confidence: 99%
“…In particular, f cos = f cos (t, x, y, Θ) is the cosine efficiency, see Collado & Turégano (1989); f sb = f sb (t, x, y, S, Θ) is the shading and blocking efficiency, see Sassi (1983); Collado & Guallar (2012); Stine & Harrigan (2001); f sp = f sp (t, x, y, Θ) is the interception efficiency or spillage factor, see Collado & Turégano (1986) and finally, f at = f at (x, y) is the atmospheric efficiency, which takes into account atmospheric losses between the heliostat and the receiver, see Biggs & Vittitoe (1976); Collado & Turégano (1989).…”
Section: Functionsmentioning
confidence: 99%