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  2. Solar coverage rate - Wikipedia

    en.wikipedia.org/wiki/Solar_coverage_rate

    The solar coverage rate is the percentage of an amount of energy that is provided by the sun. This may be in reference to a solar thermal installation or a photovoltaic installation, i.e. a calculation of solar heat, electricity or total energy produced. The observation period is typically one year.

  3. List of solar cycles - Wikipedia

    en.wikipedia.org/wiki/List_of_solar_cycles

    Following is a comparison of the growth of cycle 25 versus cycle 24, using the 13-month sunspot averages, beginning with the months of the respective minimums. Numbers in brackets for cycle 25 indicate the minimum possible value for that month, assuming there are no more sunspots between now (Jan 3, 2024) and six months after the end of the ...

  4. Solar activity and climate - Wikipedia

    en.wikipedia.org/wiki/Solar_activity_and_climate

    One historical long-term correlation between solar activity and climate change is the 1645–1715 Maunder minimum, a period of little or no sunspot activity which partially overlapped the "Little Ice Age" during which cold weather prevailed in Europe. The Little Ice Age encompassed roughly the 16th to the 19th centuries.

  5. Small Differences Are Magnified in Solar

    www.aol.com/news/2012-03-08-small-differences...

    The solar industry can be measured by two main criteria: module efficiency and cost per watt. Without one, the other is useless, because they interact to define a company's competitive position.

  6. Solar access - Wikipedia

    en.wikipedia.org/wiki/Solar_Access

    The solar envelope is a space-time construct. In terms of space, a solar envelope assures solar access to the surrounding properties. Solar envelope defines shadow fences that avoid unacceptable shadow beyond the property lines by limiting the size the building on-site. [10] Solar envelope also offers the greatest potential volume within time ...

  7. Solar cycle - Wikipedia

    en.wikipedia.org/wiki/Solar_cycle

    The occurrence frequency of coronal mass ejections and flares is strongly modulated by the cycle. Flares of any given size are some 50 times more frequent at solar maximum than at minimum. Large coronal mass ejections occur on average a few times a day at solar maximum, down to one every few days at solar minimum.

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