Solar Heat

SOLAR CONSTANT

    The energy density of solar radiation at Earth's distance from the Sun averages 1353 joules per second per square metre. Some of this energy is deflected and absorbed in Earths' atmosphere. On a sunny day at ground level we receive about 1000 joules of energy per second (1000 watts of power) per square metre perpendicular to the Sun. [This is equal to 833 watts per square yard. For interest, 746 watts = 1 horsepower.]

Principles of Solar Cooker Design
[This is the best I've found for explaining solar energy and heat principles simply and clearly. There is nothing like trying to build a solar cooker to get hands-on experience with solar energy, building techniques, and cooking.]

If you're a fan of Thermodynamics try here.
[Also from Solar Cookers International, but at an advanced level.]


HEAT ARRIVES

    Our planet is in a peculiar situation regarding heat. The interior of our planet is molten rock, kept heated by the slow energy-releasing break-down of large radioactive elements there. This heat slowly escapes through the Earth's crust. However, this by itself would not be enough to keep the surface of our planet warm. For warmth and light, and the active formation of life by plants, we require the energy received from the Sun.


HEAT CONDUCTION

    Although the colour and reflectivity of a material help us to determine the wavelengths and amount of solar energy an object will absorb (see Solar Optics), how well a material conducts heat determines whether the object will get hot all the way through (or how hot something behind it will get). Conduction is the way heat travels through an object.

    When an object is heated, it will share its heat energy with everything around it until everything is at the same temperature. This is entropy - a gradual dispersement of energy to equality everywhere. There are classically three ways that heat energy can be shared:  conduction, convection, and radiation. If something hot is touching something less hot, heat energy will be transferred by conduction.

    Different materials conduct heat at different rates. Metals conduct heat well. Materials that slow down heat flow are called insulators.

CONVECTION

    Different-temperatured masses of air or water can set up convection currents. The warmed gas or liquid is moved away from the Earth's surface. The force of gravity on cooler (and therfore more dense) gases or liquids displaces the warmed, less dense gases. We say "heat rises", and talk about "thermosiphoning". Actually, the less-dense hotter fluids and/or gases are displaced away from the Earth as cooler, denser liquids and gases are attracted more forcefully by gravity to the Earth.

    Convection works well for our planet, with water and wind currents spreading heat from the equatorial regions into the temperate and polar zones. On a smaller scale this principle can be used for the distribution of solar-heated water and air into buildings...though usually a fan or pump is employed for this purpose.

    Solar radiational energy, after being absorbed by a dark pot in a solar oven, is transmitted by conduction and convection to cook food.

INSULATION, and REFLECTIVE RADIATION BARRIERS

    Some materials do not conduct heat well, and are known as thermal insulators. For example, because of the trapped dead air spaces in it, wool does not conduct heat energy nearly as well as  a solid metal. So heat energy can be trapped behind wool, which is what is happening when we wear wool clothing. Eventually heat energy will pass through wool, but much more slowly than if the wool insulation wasn't in place. Insulation doesn't allow heat energy to travel through it easily; it slows heat transfer down.

    What  prevents easy heat conduction in wool is all the tiny air spaces. Air doesn't conduct heat well, and the smallness of the air spaces prevent convection currents from being set up. This same idea is used in fibreglass insulation, blown cellulose, and styrafoam.

    Want to keep heat in for a longer while? Use lots of insulation.

    It's not that the insulation is inherently warm, and shares its warmth with the interior object - the coat doesn't make you hot. It's that the insulation keeps the heat trapped longer - your own body heat can't escape quickly. Eventually, if no more energy is added (as heat energy is to your coat by your body metabolizing food), no matter how well one insulates, an object hotter than its surroundings will share its heat with its surroundings, and will eventually wind up at the same temperature. It's just that insulation slows that dispersion down...a lot.

    The same is true for keeping heat out...which is why containers for keeping food cool are insulated. One wonders why they aren't called out-sulated  (but perhaps that's reserved for the reflective outer coating on the better ones, which bounces heat radiation away). Warmer surroundings attempt to share their heat with the colder food. Got to keep that heat energy out if you want the food to stay cool. Insulation works as well here as it does at keeping heat in...it slows down the transfer of heat energy.

    Food coolers and thermoses will keep even more heat energy out (or in) if they are shiny outside. Why?

    If you're out camping, try wrapping the food cooler in a wool blanket, and see if the ice lasts longer. Then wrap the whole combination of food cooler and wool blanket in one of those shiny emergency "space blankets" ($2 at camping supply stores). See how much longer again the ice lasts.

    While using solar energy to create electricity is about 12 -15 % efficient, direct absorbtion of solar energy to heat water or air can be up to 75% efficient. Onward to Solar Energy Uses to see solar heat in action!


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Updated: February 2004