The combination of both methods provides decent performance in terms of high and steep OOB attenuation, thus confirming that such a combination of these methods possesses the potential for protecting both wideband and narrowband PU signals employing strict requirements with respect to the signal-to-interference-power ratio.
Protons with larger diffusion distances, e.g. in the intravascular space, show steep signal attenuation at low b values (b < 100 150 s mm−2).
The relationship between hypocentral distance and amplitude depends on the cutoff periods: the shorter the cutoff period, the steeper the attenuation.
The slope of this node is not so steep, multipath fading boosts the tail, and the higher attenuation at low distance cuts the head.
In the region, the effect of the attenuation is steeper than that of the amplification due to the conductivity enhancement toward the dip equator.
The large uncertainty in the determination of the parameters implies that only 20% of individual sources (40% of the sources detected in IR) exhibit a secure bump and and an attenuation curve steeper than the Calzetti et al. one.
Whereas the amplitude of the bump is well reproduced in the Inoue et al. model with LMC dust, the corresponding attenuation curve is steeper than the one derived from the data.
Conversely, the CC method alone results in a relatively steep OOB power reduction, but the resulting OOB attenuation is not very high.
When we apply this analysis to the QLV model, we obtain the same result, but there is overall less attenuation, so that the lines are less steep and the lowest ratio is 0.5 (not shown).
The slope of the average attenuation curve at UV wavelength is found steeper than that for local starburst galaxies.
