The resulting spectral lines from the entire galaxy blend together to form a FAT line.
Not exact matches
An interesting
result from this data was that no emission was detected in the Stokes I
spectral line profiles during the flare, which is traditionally seen in such magnetic transient regions.
A
spectral line is a dark or bright
line in an otherwise uniform and continuous spectrum,
resulting from emission or absorption of light in a narrow frequency range, compared with the nearby frequencies.
The bold
line in the bottom graph shows the modeled
spectral results including the effects of the long - term changes in the trace gases CO2, O3, N2O, CH4, CFC11 and CFC12.
I understand (to some extent) how individual atoms can radiate specific frequency
spectral lines, as a
result of energy level transitions of an electron in that atom.