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Exposure compensation step obtains the most blending exposures for each image by selecting the suitable brightness ratio of overlapping area between images.
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However, since no operational retrieval exists for MSG to compute the CWP during nighttime, suitable combinations of brightness temperature TIR10.8 and brightness temperature differences ΔTIR10.8 IR12.1, ΔTIR8.7 IR10.8, ΔTIR3.9 IR10.8 and ΔTIR3.9 WV7.3 are used to infer implicit information about microphysical and optical cloud properties.
To keep the brightness suitable, manual lighting control usually distracts the attendees' attentions in a meeting.
Therefore, we use suitable combinations of brightness temperature differences (∆T) between the thermal bands of MSG SEVIRI to infer qualitative information on CWP (ΔTIR3.9 WV7.3 and ΔTIR3.9 IR10.8) (Thies et al. 2008b; Feidas and Giannakos 2011).
We also notice that radiance (in units of W sr−1 m−2) is even more suitable than luminance (in units of cd m−2) to quantify the brightness of red to near-infrared persistent phosphors for the in vivo imaging application.
While it has been known for decades that other sunlike stars can harbor activity cycles reminiscent of the 11-yr solar cycle, it is only recently that precision photometry suitable for comparing solar brightness variability with its stellar analogs has become available.
Integrated phosphorescence intensity under 2P excitation plotted against excitation wavelength gave the 2P phosphorescence brightness spectra, directly suitable for comparison between different probes (see Experimental for details).
The probe is highly flexible, has a small diameter and produces a pattern of high brightness making it suitable for use with biological tissue and low light collection efficiency endoscope systems.
Then, according to this comparison, the DHRM adjusts the screen brightness to the most suitable level for the user.
MCNP simulations for protons or deuterons on a Beryllium target with a suitable target/moderator design yield a source brightness, from which we calculate the sample fluxes by phase space considerations for different types of spectrometers.
If a fluorescent phenotype is desired, the FP will have to fulfil several criteria including suitable excitation and emission wavelengths, photostability, brightness, and maturation speed.
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