album Solar Spectrum - Solar Spectrum mp3 download

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Solar energy covers a spectrum from UV to infrared. For the purpose of solar power, intensity, energy yield and surface orientation are most important. The energy in solar irradiation comes in the form of electromagnetic waves of a wide spectrum. Longer wavelengths have less energy (for instance infrared) than shorter ones such as visible light or UV.

The second solar spectrum is an electromagnetic spectrum of the Sun that shows the degree of linear polarization. The term was coined by V. V. Ivanov in 1991. The polarization is at a maximum close to the limb (edge) of the Sun, thus the best place to observe such a spectrum is from just inside the limb

The solar spectrum changes throughout the day and with location. The previous solar spectrum, ASTMG159, was withdrawn from use in 2005. In most cases, the difference between the spectrum has little effect on device performance and the newer spectra are easier to use.

The debut album of SOLAR SPECTRUM was released 2009 on Free Freak Records as well with already two releases on Glowing Flame Records and Free Freak Records.