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These include the fact that this absorption band is weak compared to many other minerals, a number of other minerals also exhibit absorption bands in this wavelength region (leading to possible misidentifications), and that even small abundances of minerals that absorb strongly in this region will reduce the strength of the carbonate absorption band.
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More bluish and/or greenish portions indicate smaller abundances of absorbers, while reddish shades indicate a higher cloud-top level over other regions due to less CO2 absorption above the cloud top in the CO2 band (2.02 um). Figure 12 shows yellowish areas in the 10°S 10°N latitude, implying the area has less unknown absorber(s) and the cloud-top level is higher than the surrounding region.
Contrary to this observation, mammals and other vertebrates had a much smaller abundance of RP-sites within their large introns compared to their complementary strands (a ratio of 1.5 or less).
A smaller abundance of the LHCII trimers, fluorescence of LHCII antenna and smaller relative amounts of Lhcb1 to PsbA apoproteins in bean in comparison to pea thylakoids were found.
Mature forest monoculture also supports a low abundance of small mammals in Norway (Panzacchi et al. 2010).
Unfortunately, the small size and low abundance of Aβ oligomers, in combination with their considerable heterogeneity and high sensitivity to environmental changes, has rendered them challenging to characterise.
For transcript sequencing projects with extreme variation in read depth the latter is not possible because, while the probability of a single base substitution might be quite small, the abundance of the most abundant reads easily compensates for this.
Next, we compared the small RNA abundance of each individual cluster in wild-type and nrpe libraries and calculated the fold difference of HNA between them.
Other small neutral losses, although of considerably smaller abundance, correspond to Δ m values of 30.010, 56.070, and 72.023 Da and elemental compositions of C1H2O1, C4H8, and C3H4O2, respectively.
We observe that the difference is clear at small grain sizes: because small grains are also shattered efficiently for small ac, the abundance of smallest-sized grains is larger for smaller ac.
To assess the potential for differences in the relative abundances of small molecules in Calrose, Dixiebelle, and Neptune, we performed a principal component analysis (PCA).
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