Sentence examples for dust size from inspiring English sources

We found that the single-sized and power-law dust size distributions yield a very similar detectability of LBGs at submillimeter wavelengths.

The lower limit of dust size cannot be detected directly and the dust size may not even follow a simple power-law distribution.

For example, the dust size distribution may be variable and is difficult to constrain.

Fig. 4. Variations of AV/Δτ3.4 μm and AV/Δτ9.7 μm with dust size.

In this paper, a concept for the improvement of SRM dust size modelling is discussed.

v rel is the relative speed between dust and the spacecraft and varies with the dust size (see Subsubsection 3.2.2).

We calculate AV/Δτ3.4 μm and AV/Δτ9.7 μm for various dust models with a range of porosities and dust sizes.

This sizedependence comes from the fact that smaller dust particles have higher temperatures in the dust sizes (≳1μm) we concern, owing to their lower emissivity.

While active sublimation at 100 110K is independent of dust sizes, small dust sublimes prior to large dust because the temperature of small dust is higher (Kobayashi et al., 2008).

The quantitative relation between dust flux and reflectance change is uncertain since the flux of the inflow dust colliding with the lunar surface has not yet been quantitatively estimated for different dust sizes.

In the future we will consider more realistic models in which more dust species (e.g. hydrogenated amorphous carbon with a range of C/H ratios), the distribution of dust along the line of sight toward the GC (e.g. see Sandford et al., 1995), a distribution of dust sizes, and the possible porous nature of the diffuse ISM dust (e.g. see Mathis and Whiffen, 1989) will be considered.