magnitudspektrum
Magnitudspektrum refers to the range of magnitudes observed for a particular phenomenon. In astronomy, it commonly relates to the brightness of celestial objects, where magnitude is a logarithmic scale of brightness. Brighter objects have lower or more negative magnitudes, while fainter objects have higher or more positive magnitudes. The magnitudspektrum can describe the distribution of stars in a galaxy by their apparent brightness or the range of luminosities of quasars.
Beyond astronomy, the concept of magnitudspektrum can be applied to other fields. For instance, in seismology,