... density[*]
The HVC component was computed by integrating over the channels between -168.5 and -96.4 km s-1.
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... broadening[*]
Here we consider that the spectral response follows a Gaussian function.
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... constant[*]
Here we make the assumption that the depth of the cloud is small compared to the distance to the cloud, which allows us to do the integral in Cartesian coordinates and not take into account the fact that a beam sees structures of increasing physical size with distance.
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... maps[*]
The standard deviation of  $\sigma(x,y)$ is not given here and not used in this analysis as it is more affected by noise.
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... fields[*]
As shown by Brunt & Low (2004) and Esquivel & Lazarian (2005) this is only true for low contrast density fields ( $\sigma_n/\langle n\rangle \leq 1$).
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... them[*]
Miville-Deschênes et al. (2003b); Brunt & Low (2004) showed that the level of correlation between the density and velocity does not modify significantly the statistics of projected quantities.
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... spectrum[*]
From our tests on cubes with 0.1<H/L<10 and a spectral index $\gamma=-3.4$ we did not observe significant changes of the power spectrum after the modification of the fBm using Eq. (11).
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...$\sigma_n/\langle n\rangle $)[*]
Both the average density $\langle n\rangle $ and the standard deviation of thedensity $\sigma_n$ depend on D but not their ratio.
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... values[*]
These relatively low contrasts give an indication that the velocity power spectrum obtained from the centroid velocity is not affected significantly by density fluctuations.
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Copyright ESO 2007