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Statistical Properties of Clear and Dark Duration Lengths

Identifikátory výsledku

  • Kód výsledku v IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985807%3A_____%2F17%3A00475605" target="_blank" >RIV/67985807:_____/17:00475605 - isvavai.cz</a>

  • Nalezeny alternativní kódy

    RIV/68407700:21730/17:00320094

  • Výsledek na webu

    <a href="http://dx.doi.org/10.1016/j.solener.2017.06.003" target="_blank" >http://dx.doi.org/10.1016/j.solener.2017.06.003</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.solener.2017.06.003" target="_blank" >10.1016/j.solener.2017.06.003</a>

Alternativní jazyky

  • Jazyk výsledku

    angličtina

  • Název v původním jazyce

    Statistical Properties of Clear and Dark Duration Lengths

  • Popis výsledku v původním jazyce

    The focus of this study is on the properties of consecutive intervals consisting of pairs of clear periods (the Sun is shining) and dark periods (the Sun is obscured by clouds). Namely, the distribution of the duration length of clear and dark periods is studied and illustrated with results obtained for the climatic regime of Timisoara (Romania, Eastern Europe). Usual simple moment-based characteristics such as means and variances cannot be unambiguously estimated due to censoring. Seasonal changes in the length distributions have been studied through the (nonparametric) Kaplan-Meier estimates. Both dark and clear duration distributions are different among months. The correlation between clear and dark periods within one dark-clear pair is of substantial interest. Therefore, a rigorous approach based on Spearman’s rank correlation coefficient is used instead. The dependence of duration distribution upon covariates is studied using the Cox regression model, which fits the hazard ratio incurred by a unit change in the explanatory variables. It is shown that increasing the extraterrestrial irradiance on horizontal surface and the clearness index during dark/clear periods increases significantly the dark/clear period end risk. The Cox regression model enables more complicated analyses, such as the non-additive effects (i.e. interactions) of several covariates. The clearness index of a dark period (CID) has a much stronger effect than the extraterrestrial irradiance on horizontal surface of a dark period (EID) and the CID-EID interaction is still significant after the interactions when the months are included.

  • Název v anglickém jazyce

    Statistical Properties of Clear and Dark Duration Lengths

  • Popis výsledku anglicky

    The focus of this study is on the properties of consecutive intervals consisting of pairs of clear periods (the Sun is shining) and dark periods (the Sun is obscured by clouds). Namely, the distribution of the duration length of clear and dark periods is studied and illustrated with results obtained for the climatic regime of Timisoara (Romania, Eastern Europe). Usual simple moment-based characteristics such as means and variances cannot be unambiguously estimated due to censoring. Seasonal changes in the length distributions have been studied through the (nonparametric) Kaplan-Meier estimates. Both dark and clear duration distributions are different among months. The correlation between clear and dark periods within one dark-clear pair is of substantial interest. Therefore, a rigorous approach based on Spearman’s rank correlation coefficient is used instead. The dependence of duration distribution upon covariates is studied using the Cox regression model, which fits the hazard ratio incurred by a unit change in the explanatory variables. It is shown that increasing the extraterrestrial irradiance on horizontal surface and the clearness index during dark/clear periods increases significantly the dark/clear period end risk. The Cox regression model enables more complicated analyses, such as the non-additive effects (i.e. interactions) of several covariates. The clearness index of a dark period (CID) has a much stronger effect than the extraterrestrial irradiance on horizontal surface of a dark period (EID) and the CID-EID interaction is still significant after the interactions when the months are included.

Klasifikace

  • Druh

    J<sub>imp</sub> - Článek v periodiku v databázi Web of Science

  • CEP obor

  • OECD FORD obor

    10103 - Statistics and probability

Návaznosti výsledku

  • Projekt

  • Návaznosti

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Ostatní

  • Rok uplatnění

    2017

  • Kód důvěrnosti údajů

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Údaje specifické pro druh výsledku

  • Název periodika

    Solar Energy

  • ISSN

    0038-092X

  • e-ISSN

  • Svazek periodika

    153

  • Číslo periodika v rámci svazku

    1 September

  • Stát vydavatele periodika

    US - Spojené státy americké

  • Počet stran výsledku

    11

  • Strana od-do

    508-518

  • Kód UT WoS článku

    000411847200045

  • EID výsledku v databázi Scopus

    2-s2.0-85020642153