Want this question answered?
No. Atomic emission spectrum is non-contiuous and it is named as line spectrum.
Dark lines especially in solar spectrum have been named as Fraunhofer lines. These line are good examples for line absorption spectrum
They differ:* By their frequency * By their wavelength, which is inversely proportional to their frequency * By the energy per photon, which is proportional to the frequency
I have no clue Laugh out loud
Heat energy is measured by temperature and solar energy is the energy that comes from the sun in the form of heat or light. Isabel B.
No. Atomic emission spectrum is non-contiuous and it is named as line spectrum.
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
what r u on about
solar flares isfire
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
Seven
its violet
Because the band is broken by colorless gaps
The difference between continuous spectrum and the atomic emission espectrum of an element is that in emission spectrum, only certain specific frequencies of light are emitted while in a continuous spectrum, a continuous range of colors are seen in the visible light.
"atomic weight" is always on the x-axis of the mass spectrum graph.