The noise spectrum is typically comprised of a wide-band section and some peaks that have been referred to as a periodic part plus its harmonics.
As summarized in "Satellite observation" section, peak-to-peak amplitude of (delta B_{y}) in Fig. 3b, which corresponds to zonal component of magnetic perturbations, is largest.
More specifically, VO2peak and GE were correlated to the last two uphill and two final flat section times, whereas Vpeak and peak cycle length were correlated to times in all uphill, flat, and curved sections except for the initial section (r = ~−0.80, P < 0.01).
Next, MALDI-IMS was performed on the successive tissue sections, and ion peaks corresponding to the pre-identified lipid molecular species by LC/ESI-MS/MS were selected.
Furthermore, one can alter the shape and size of the plasmonic nanoparticles to maximize their optical absorption and scattering cross section and tune the absorption peak position [ 16, 17], which is greatly beneficial for a variety of biomedical imaging applications.
Section 2.1 describes the OFDM signal model, Section 2.2 explores peak side lobe (PSL) and peak cross-correlation performance of wideband OFDM radar pulses with random subband composition, and Section 2.3 describes signal characteristics for the benchmark waveforms.
With a pump power of 5 W at 880 nm, when the heat sink temperature of Cr4+:YAG is fixed, the temperature of Nd YVO4 is changed to adjust its stimulated emission cross section; its peak power and single-pulse energy are improved from 700 W and 28 μJ to 1900 W and 65 μJ, respectively, as the temperature increases from 0 to 115 °C.
When the heat sink temperature of Nd YVO4 is fixed and the temperature of Cr4+:YAG is changed to adjust its ground state absorption cross section, the peak power and single-pulse energy are decreased by 50% and 30%, respectively, as the temperature increases from 0 to 170 °C.
Turbulent intensities in the streamwise (urms) and spanwise (vrms) directions peak at the sheath section and at the approximate top of the canopy (0.9 1.2Hv).
We converted the fitted M1 peak densities obtained in the section "M1 peak electron density and solar zenith angle" to subsolar values using N m =N 0 C h −0.5.
