The emission maximum wavelength and shoulder emission are located at 588 and 630 nm, respectively, revealing an orange-red light.
This suggests that the reconfiguration of the coronal magnetic fields and the subsequent energy release that gave rise to the impulsive burst emission did not significantly perturb that part of the corona where the noise storm emission was located.
Later on, a main source of emission was located in the core of the active region, which is an indirect signature of the magnetic reconnection occurring behind the erupting flux rope.
The assumed altitude of 105 km is reasonable, because we applied tomography analysis to the 428-nm images taken by the three EMCCD imagers and confirmed that the maximal peaks of the emission were located around 95- to 115-km altitude (not shown here).
The titration experiment showed that the probe gave colorimetric response towards sodium nitrite with the absorption maxima at 630 nm and 542 nm in pH = 5.0 disodium hydrogen phosphate-citric acid buffers containing 30% DMSO; its emission was located in 590 820 nm with the 9.1-fold fluorescent enhancement under excitation at 580 nm.
The galactic black hole, dubbed Sagittarius A*, and its surrounding emission are located in the brightest central region of the image.
For three volunteers with Caucasian skin, the same observation is made: clusters of cells exhibiting yellow or green emission are located around dermal papilla.
Because the FNDs are about 100 nm in diameter, the strong quenching effects suggest that the (N-V)- centers responsible for the FND fluorescence emission are located on or close to the surface of the FNDs.
The internal quantum efficiencies reached 3.4%, and the emissions were located at near-infrared and green (Fig. 11).
As indicated by a blue (green) dot, the CIE coordinates of pure p-6P (sub-ML 6T) emissions are located at (0.16, 0.07) and (0.42, 0.54), respectively.
