Introduction to Solar Radiation and its Impact on Photovoltaic Production

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Solar radiation is the main source of energy used by photovoltaic systems. The solar constant at the top of the atmosphere is around 1361-1362 W/m², but this value varies according to the Earth's orbit. As it passes through the atmosphere, it undergoes absorption, scattering and attenuation, mainly due to clouds, aerosols, water vapor and atmospheric gases.

Types of Solar Radiation

The solar radiation reaching the Earth's surface, known as global radiation, consists of three main components:

  • 1 . Radiation directe – L'énergie solaire qui atteint la surface de la Terre sans dispersion.
  • 2 . Radiation diffuse – La lumière solaire qui est réfléchie ou dispersée par l'atmosphère.
  • 3 . Radiation réfléchie – L'énergie solaire réfléchie par le sol ou les obstacles environnants.

In clear sky conditions, solar radiation reaches its maximum level, which is crucial for modeling photovoltaic production in PVGIS.COM.

Estimating Solar Radiation: Ground Measurements vs. Satellite Data

Ground Measurements: High Accuracy but Limited Coverage

The most accurate way to measure solar radiation is through high-precision sensors , but this requires:

  • Regular sensor calibration and maintenance
  • Frequent measurements (at least once per hour)
  • Data collection over at least 20 years

However, ground measurement stations are limited and unevenly distributed, making satellite data a more reliable alternative.

Satellite Data: Global Coverage and Long-Term Analysis

Weather satellites like METEOSAT provide high-resolution images covering Europe, Africa, and Asia , with historical records spanning over 30 years.

Advantages of Satellite Data

  • Available even in areas without ground measurement stations
  • Data updates every 15-30 minutes
  • Reliable estimations based on cloud, aerosol, and water vapor analysis

Limitations of Satellite Data

Possible inaccuracies under certain conditions:

    • Snow may be misinterpreted as clouds
    • Dust storms can be difficult to detect
    • Geostationary satellites do not cover polar regions

To compensate for these limitations, PVGIS.COM also integrates climate reanalysis data for regions not covered by satellite observations.

Methods for Calculating Solar Radiation in PVGIS.COM

PVGIS.COM uses advanced algorithms to estimate solar radiation based on the following data sources:

  • PVGIS-CMSAF and PVGIS-SARAH – Data for Europe, Africa, and Asia
  • NSRDB – Solar radiation database for North and Central America
  • ECMWF ERA-5 – Climate model data from global reanalysis

Calculation Process

  • 1 . Analyzing satellite images to determine cloud cover
  • 2 . Modeling solar radiation under clear-sky conditions , considering the effects of aerosols, water vapor, and ozone
  • 3 . Computing total solar radiation using cloud reflectivity data and atmospheric models

Potential Sources of Error

Snow may be mistaken for clouds , leading to underestimated radiation values

Sudden changes in aerosol levels (e.g., dust storms, volcanic eruptions) may not be immediately detected

Data Sources and Availability in PVGIS.COM

METEOSAT Satellites – Provide hourly data for Europe, Africa, and Asia.

ECMWF ERA-5 – Global climate data reanalysis.

NSRDB – Solar radiation database for North and Central America.

These data sources allow PVGIS.COM to offer near-global coverage for solar radiation estimates and enhance photovoltaic simulations.

Conclusion

Advancements in satellite remote sensing and climate modeling enable PVGIS.COM to provide highly accurate solar radiation estimates, helping solar energy professionals optimize their PV installations.

Benefits of PVGIS.COM

Reliable data from satellite and climate models

Accurate simulations for each region to estimate solar energy production

Advanced tools for researchers and engineers in solar energy analysis