The solar radiation arriving at Earth (once known as the “solar constant”, now usually referred to as Total Solar Irradiance (TSI)), is the most fundamental of climate parameters as it indicates the totality of the energy driving the climate system. The solar irradiance is the output of light energy from the entire disk of the Sun, measured at the Earth. A project’s location determines the amount of sunlight, or irradiance, it will receive. Only half the Earth is ever lit by the Sun at one time, which halves the total solar irradiance. [1] The most accurate value of total solar irradiance during the 2008 solar minimum period is 1360.8 ± 0.5 W m−2 according to measurements from the Total Irradiance Monitor (TIM) on NASA’s Solar Radiation and Climate Experiment (SORCE) and a series of new radiometric laboratory tests. Last updated on April 17, 2017 Another way to calculate TSRF is to multiply the TOF by the Solar Access % (96% x 91.9% = 88.2%). The hours of insolation are equal to the average daily kilowatt hours received per square meter. The total solar irradiance is the maximum possible power that the Sun can deliver to a planet at Earth’s average distance from the Sun; basic geometry limits the actual solar energy intercepted by Earth. While typical values can range from 1,000 kWh/kWp to over 2,000 kWh/kWp, the actual value is driven by many factors, including: Location. It also varies throughout the day, depending on the position of the sun in the sky, and the weather. The Total Irradiance Monitor (TIM) measures the total solar irradiance (TSI), monitoring the incident radiant energy powering the Earth’s climate system. The current most accurate TSI values from the Total Irradiance Monitor (TIM) on NASA’s Solar Radiation and Climate Experiment ( SORCE ) is 1360.8 ± 0.5 W/m2 during the 2008 solar minimum as compared to previous estimates of 1365.4 ± 1.3 W/m2 established in the 1990s. What is Solar Insolation? METSTAT uses meteorological inputs such as cloud cover and precipitable water to produce a nominal value of solar irradiance and randomly varies this value via statistical tables derived from measured solar irradiance data. It is measured in watts per square metre (W/m2). To find Total Solar Resource Factor (TSRF) HelioScope compares Shaded Irradiance (1910.4 kWh/m2) to the Optimal POA Irradiance (2165.1 kWh/m2) which gives 88.2%. This irradiance varies throughout the year depending on the seasons. Both methods of calculating TSRF give the same value. ... We can easily see from the table that the Total Solar Irradiance (TSI) is the main contributor of energy to Earth. “”””…Total solar irradiance, also called “TSI”, is the total amount of energy coming from the sun at all frequencies. Solar Irradiance is a measure of how much solar power you are getting at your location. …””” See it says TSI is the “total” amount of energy coming from the sun at all frequencies. 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