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The category of supergiants includes stars of all spectral types; these stars show a large spread in intrinsic brightness, and some even approach absolute magnitudes of −7 or −8.
The levels of Cu ions (0.023 0.63030.150150) are less with a large spread in concentration.
The cross-over between these two regimes is signified by a large spread in the multifractal spectrum.
From the figure, it is also evident that there is a large spread in the observed intensities for this region.
For each of the units there is a large spread in the measurement error (up to 65%).
On the other hand spectral results reveal a large spread in each one-third octave band (standard deviations of up to 5 dB).
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A larger spread in frequency shifts the phase of the response and appreciably decreases the amplitude.
In these figures, a larger spread in the distributions can be seen, as it was anticipated in the theoretical analysis.
A larger spread in the damage degrees for all the structures is observed by analyzing the results obtained using SPO2FRAG, as compared to the results from FRACAS.
This is probably more a reflection of the underlying data distributions than patterns in the relationship between estimation error and environmental variables (i.e., where there are more data you would expect a larger spread in the errors).
This might be because low sounds (below 400 Hz) travel a set distance in any environment, while higher (above 400 Hz) sounds have a larger spread in the distance travelled.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com