The intensity of a line is proportional to the number of photons emitted or absorbed by the atoms. It depends on the number of atoms giving rise to the line.
A carbon arc emission spectrograph is a piece of scientific equipment. Emission spectography is used to measure radiation intensity, and provides information about atoms and molecules as well as chemical composition of objects.
Niels Bohr in 1913.
line emission
The emission of laser beam through the semitransparent end face actually consists of spikes of high intensity emissions. This phenomen is called spiking of the laser.
Low light intensity lowers the rate of photosynthesis, Normal sunlight is good for a normal rate of photosynthesis, Very high intensity bleaches (destruction) the chlorophyll
Intensity ∞ Amplitude2
Power broadening is an effect whereby the line-width of a laser is broadened by the laser intensity itself. Higher laser intensity leads to a larger line-width. This can be explained by considering the decay rate of atoms from the upper to lower laser level. As the laser intensity increases, this decay rate (which is linearly related to the line-width) increases due to stimulated emission.
A carbon arc emission spectrograph is a piece of scientific equipment. Emission spectography is used to measure radiation intensity, and provides information about atoms and molecules as well as chemical composition of objects.
Niels Bohr studied the emission lines of Hydrogen.
Sound Intensity = Power / Area. So the more power delivered to a smaller area the greater the intensity.
Mass of object and distance from it
No. Atomic emission spectrum is non-contiuous and it is named as line spectrum.
Intensity of spectral line show the abundance of different elements in the light source. Every element has its own "fingerprint" which can indicate its presence.
Its volume or how loud it is.
The answer will depend on the addiction - both the substance (or activity) and intensity.
A spiral galaxy with a small, compact, bright nucleus that exhibits variable light intensity and radio-wave emission.
Niels Bohr in 1913.