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Dark-line spectrum is a "photo-negative" of emission spectrum. It is the gaps that appear in precisely the same location as corresponding bright lines. produced by a cool gas with a hot solid and you
No, its an absorption spectrum
They are like this due to the fact that most hydrogen atoms are ionized which makes a weaker balmer line. The strength of the Balmer line is sensitive to temperature so that's why it occurs more in the middle. The hot end of the hydrogen is low Balmer line due to them being in the ground state. Hope that's answers it =] -CRS
Away in a manger !!!!!!!!!!!!!!!!!!!!!!!!!LOL!!!!!!!!!!
The easiest way to identify Orion (the Hunter) is the 3 bright stars in line forming Orion's belt.
The bright line spectrum is useful because it shows us the different particles in the elements.
Line Spectra was created in 2006.
Gas comes out of peoples butts so when you look at its spectrum it has a green stinky color since gas or "farts" smeel and have a natural color of green.
The cavity radiation spectrum comes from surface temperature. Bright line (emission) spectra come from hot elements near the surface. Dark line (absorption) spectra come from cooler elements further out. Because they're at different temperatures and have slightly different elemental ratios, each star produces a unique "fingerprint".
There are several kinds of spectra. Bright line spectrum, or emission spectrum, is when light emitted by a gas has an electrical discharge going through it, and it produces a spectrum of just a few isolated parallel lines.
Emission spectra are bright-line spectra, absorption spectra are dark-line spectra. That is: an emission spectrum is a series of bright lines on a dark background. An absorption spectrum is a series of dark lines on a normal spectrum (rainbow) background.
It is called Visible light Spectrum.
Dark-line spectrum is a "photo-negative" of emission spectrum. It is the gaps that appear in precisely the same location as corresponding bright lines. produced by a cool gas with a hot solid and you
Each type of atom gives off a unique set of colors. The colored lines (or Spectral Lines ) are a kind of "signature" for the atoms
Each type of atom gives off a unique set of colors. The colored lines (or Spectral Lines ) are a kind of "signature" for the atoms
No, its an absorption spectrum
It depends on what you consider the Spectra meter. The original was called the Norwood Director and it came out in 1946 and was manufactured by a company called Photo Research (which did and does make the Spectra line of meters). In 1948, a redesigned Norwood Director was manufactured and sold through American Bolex. Photo Research continued to make the original Norwood as the "Spectra." So it's 1946 or 1948, depending on where you want to start counting.