Sentence examples for spectra of around from inspiring English sources

As shown in Fig. 2b, test example of two fluorescent beads reveals a measured shift between the maxima of fluorescence emission spectra of around 9 nm, which agrees well with the shift of around 10 nm declared by the producer of the beads.

Regarding the ISM band, by removing the AGC noise from the spectrogram we have demonstrated a reduction in spectrum usage of around 40% as when compared with energy detection using the ITU recommended threshold.

Spending as a share of GDP ranges from 0.15% to 0.20% in the US and Japan, respectively on the one end of the spectrum, to around 1% in France, Germany and 1.5% or more in the Nordic countries.

Now, employing the DE-cad::mTomato allele it is possible to show the maximal projection without so much interference of the yolk as its auto-fluorescence is lower in the emission spectrum of mTomato (around 560-600 nm).

The corresponding Bi compositional profiles along the growth direction, determined by integrating the point EDX spectra of an area of around 130 nm, are shown in Fig. 2c as blue and black lines respectively.

Mobile operators in the Netherlands last week paid €3.8bn (£3.1 billion) for the country's 4G spectrum, easily surpassing expectations of around €450m.

It increases the utilization of the spectrum from around 44%% to around 48%% in the simulations and increases spectrum utilization from around 37 % to around 43 % in theory when SNR is −20dB.

All spectra for pre-sputtering and post-sputtering shows peaks positioned around 711 and 724 eV, which are typical core level spectra of Fe3O4 and around 710 and 723 eV, which are characteristic for Fe2+ ions in FeO [20].

We study the influence of these chemical treatments on the dynamic mechanical relaxation spectra of the composites around the main relaxation mode.

Characteristics peaks of Plasmon resonance spectra of Ag NPs around 400 nm are seen in these figures, and they are absent with dilute aqueous extract of neem and AgNO3 solutions.

The wavelengths and band strengths observed in the infrared spectra of circumstellar shells around evolved stars may be accounted for by the excitation of C60 in a cluster state (Zhang and Kwok, this issue).