Dark lines of the absorption spectrum give the elemental composition of the chromosphere, information about the magnetic field and density of the surface. The peak of the continuous spectrum gives the surface temperature. The Doppler Effect shows the movement of the sun and the sun's surface. Splitting of spectral lines verifies the magnetism of sunspots.
Temperature, composition and speed relative to us.
binary star systems
The average reflectance is then determined by an averaging process, using a standard solar spectrum. This method is documented by ASTM (Amer. Soc. for ...
Marc S. Allen has written: 'High resolution atlas of the solar spectrum 2678-2831 A' -- subject- s -: Charts, diagrams, Solar Spectrum, Spectrum, Solar, Spectrum, Ultraviolet, Ultraviolet Spectrum
Charles Edward St. John has written: 'Revision of Rowland's Preliminary table of solar spectrum wave-lengths' -- subject(s): Solar Spectrum, Spectrum analysis, Spectrum, Solar
J. Houtgast has written: 'The variations in the profiles of strong Fraunhofer lines along a radius of the solar disc' -- subject(s): Solar Spectrum, Spectrum analysis, Spectrum, Solar
In the visible spectrum the color is determined by its' wavelength. The energy of the quantum package is determined by the wavelength. The shorter the wavelength the more power per package.
There is a few things that can be determined by studying the shape of classic grain. This is called the palynology study.
the answer to this question is when you use the power around you and it comes in as one so basically that is why it is called solar power
Genetic courses of behavior can be determined by studying genetic similarities between two species.
its violet
it is determined by studying the relative and absolute ages of rocks and fossils