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Solar Energy Basics: Difference between revisions
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<b>Solar energy Basics:</b> {{tag|Solar energy|Solar energy}} is the {{tag|energy}}, heat, or electricity, that is produced directly by using the energy that is radiated from Earth's sun (Sol) onto Earth. | <b>Solar energy Basics:</b> {{tag|Solar energy|Solar energy}} is the {{tag|energy}}, heat, or electricity, that is produced directly by using the energy that is radiated from Earth's sun (Sol) onto Earth. | ||
When the sun shines onto land, it exerts 1367 watts per m². Taking into account the fact that Earth is a sphere (and therefore the rays often angled), and also rotates, the solar radiation upon Earth's surface on average 24 hours and four Seasons at European latitudes of about 200 watts per square meter. | |||
The amount of solar energy arriving | The amount of solar energy arriving upon Earth's surface is so huge, about a thousand times greater than all of the energy that is used by humans as a whole, but scattered, in the sense that it is necessary to collect energy from vast areas in order to have significant quantities. Also, it is rather difficult to convert that energy into an easily exploitable form (mainly electricity) with acceptable efficiencies. | ||
To exploit it are needed products generally high cost that make solar energy much expensive compared to other methods of generating energy. | To exploit it are needed products which are generally high in cost that make solar energy much expensive compared to other methods of generating energy. | ||
{{Size <!--see Template:Size for full detail--> | {{Size <!--see Template:Size for full detail--> | ||
|pages= 19 <!--type the plain number of pages - NO thousands separators--> | |pages= 19 <!--type the plain number of pages - NO thousands separators--> | ||