The sunlight that we know, has its origins in the fusion process that takes place inside the Sun. The Sun is the process by “baking up” to an effective surface temperature of around 5500 ° C and sends a result of these temperature radiation, sunlight. If we sunlight with a prism to break up (think of a rainbow), we see that the sunlight from a large number of colors. Specifically, we see high energy (short wavelength) to violet and low energy (long wavelength) red. Read the rest of this entry »