Mapping Nighttime and All-Day Radiative Cooling Potential in Europe and the Influence of Solar Reflectivity

Radiative cooling is a natural process to cool down surfaces through the rejection of thermal radiation using the outer space as a cold sink, taking advantage of the transparency of the atmospheric windows (8–14 μm), which partially matches the infrared radiation band. With the development of new ma...

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Main Authors: Roger Vilà, Marc Medrano, Albert Castell
Format: Article
Language:English
Published: MDPI AG 2021-08-01
Series:Atmosphere
Subjects:
Online Access:https://www.mdpi.com/2073-4433/12/9/1119
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author Roger Vilà
Marc Medrano
Albert Castell
author_facet Roger Vilà
Marc Medrano
Albert Castell
author_sort Roger Vilà
collection DOAJ
description Radiative cooling is a natural process to cool down surfaces through the rejection of thermal radiation using the outer space as a cold sink, taking advantage of the transparency of the atmospheric windows (8–14 μm), which partially matches the infrared radiation band. With the development of new materials that have a high reflectivity of solar radiation, daytime radiative cooling can be achieved. This phenomenon depends on the optical properties of the surface and the local weather conditions. In this research, climatological data from 1791 weather stations were used to present detailed nighttime and all-day radiative cooling maps for the potential implementation of radiative cooling-based technologies. The paper offers a parametric study of the variation of the potential as a result of decreasing the solar reflectivity. The results show that southern Europe is the region with the highest potential while northern Europe holds more hours of available radiative cooling. After varying the solar reflectivity from 1 to 0.5 the average power reduces from 60.18 to 45.32 W/m<sup>2</sup>, and energy from 527.10 to 264.87 kWh/m<sup>2</sup>·year. For solar reflectivity lower than 0.5, all-day radiative coolers behave as nighttime radiative coolers, but power and energy values improve significantly for high values of solar reflectivity. Small variations of solar reflectivity have greater impacts on the potential at higher reflectivity values than at lower ones.
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spelling doaj.art-96c121fc94ad41248e9146470f3cb6462023-11-22T11:59:31ZengMDPI AGAtmosphere2073-44332021-08-01129111910.3390/atmos12091119Mapping Nighttime and All-Day Radiative Cooling Potential in Europe and the Influence of Solar ReflectivityRoger Vilà0Marc Medrano1Albert Castell2Sustainable Energy, Machinery and Buildings (SEMB) Research Group, INSPIRES Research Centre, Universitat de Lleida, Pere de Cabrera s/n, 25001 Lleida, SpainSustainable Energy, Machinery and Buildings (SEMB) Research Group, INSPIRES Research Centre, Universitat de Lleida, Pere de Cabrera s/n, 25001 Lleida, SpainSustainable Energy, Machinery and Buildings (SEMB) Research Group, INSPIRES Research Centre, Universitat de Lleida, Pere de Cabrera s/n, 25001 Lleida, SpainRadiative cooling is a natural process to cool down surfaces through the rejection of thermal radiation using the outer space as a cold sink, taking advantage of the transparency of the atmospheric windows (8–14 μm), which partially matches the infrared radiation band. With the development of new materials that have a high reflectivity of solar radiation, daytime radiative cooling can be achieved. This phenomenon depends on the optical properties of the surface and the local weather conditions. In this research, climatological data from 1791 weather stations were used to present detailed nighttime and all-day radiative cooling maps for the potential implementation of radiative cooling-based technologies. The paper offers a parametric study of the variation of the potential as a result of decreasing the solar reflectivity. The results show that southern Europe is the region with the highest potential while northern Europe holds more hours of available radiative cooling. After varying the solar reflectivity from 1 to 0.5 the average power reduces from 60.18 to 45.32 W/m<sup>2</sup>, and energy from 527.10 to 264.87 kWh/m<sup>2</sup>·year. For solar reflectivity lower than 0.5, all-day radiative coolers behave as nighttime radiative coolers, but power and energy values improve significantly for high values of solar reflectivity. Small variations of solar reflectivity have greater impacts on the potential at higher reflectivity values than at lower ones.https://www.mdpi.com/2073-4433/12/9/1119radiative coolingnighttime radiative coolingdaytime radiative coolingall-day radiative coolingcooling potentialpotential maps
spellingShingle Roger Vilà
Marc Medrano
Albert Castell
Mapping Nighttime and All-Day Radiative Cooling Potential in Europe and the Influence of Solar Reflectivity
Atmosphere
radiative cooling
nighttime radiative cooling
daytime radiative cooling
all-day radiative cooling
cooling potential
potential maps
title Mapping Nighttime and All-Day Radiative Cooling Potential in Europe and the Influence of Solar Reflectivity
title_full Mapping Nighttime and All-Day Radiative Cooling Potential in Europe and the Influence of Solar Reflectivity
title_fullStr Mapping Nighttime and All-Day Radiative Cooling Potential in Europe and the Influence of Solar Reflectivity
title_full_unstemmed Mapping Nighttime and All-Day Radiative Cooling Potential in Europe and the Influence of Solar Reflectivity
title_short Mapping Nighttime and All-Day Radiative Cooling Potential in Europe and the Influence of Solar Reflectivity
title_sort mapping nighttime and all day radiative cooling potential in europe and the influence of solar reflectivity
topic radiative cooling
nighttime radiative cooling
daytime radiative cooling
all-day radiative cooling
cooling potential
potential maps
url https://www.mdpi.com/2073-4433/12/9/1119
work_keys_str_mv AT rogervila mappingnighttimeandalldayradiativecoolingpotentialineuropeandtheinfluenceofsolarreflectivity
AT marcmedrano mappingnighttimeandalldayradiativecoolingpotentialineuropeandtheinfluenceofsolarreflectivity
AT albertcastell mappingnighttimeandalldayradiativecoolingpotentialineuropeandtheinfluenceofsolarreflectivity