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It was found that an x-ray pulse would be obtained with a critical photon energy of 0.69keV, a pulse width of 250fs and an average brightness of 3 × 106 photons/s/mm2/mrad2/0.1%BW.
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In DMF, molecules have an average brightness (Bav) of about 6.937, which after calibration corresponds to about 142 000 counts molecule 1 s 1.
Ste11 exhibited an average brightness close to that of dimeric cytosolic GFP, whereas Ste50 showed an average brightness in-between dimeric and trimeric cytosolic GFP.
The data reveal a dominant specie (N comprises approximately 65 to 75% of the total particles from the fit) with a mCherry average brightness (2400±150) consistent with that of a monomer (p = 0.12) and a GFP average brightness of 4980±230, which is indistinguishable from the 1dPCH GFP-GFP dimer brightness (p = 0.7).
The trend is consistent with a lower average brightness of the Ste11 component of this complex, and perhaps a distribution of interacting species that varies between 2∶1 and 1∶1 Ste1∶1Ste50.
Images were presented in gray scale and were adjusted to an average brightness level.
The amplitudes of flares in a unit of average brightness of the star range from 1.3×10−3 to 8.5×10−2, and the bolometric energies of flares range from 2×1032 to 8×1035 erg.
The problem of appearing dark against the sky was explored in the U.S. Navy's Yehudi lights project in 1943, using counter-illumination to raise the average brightness of a plane, when seen head-on, from a dark shape to the same as the sky.
Another form of animal camouflage uses bioluminescence to increase the average brightness of an animal to match the brightness of the background.
The average brightness of an empty portion of each picture was considered as the background for that picture (Bkg).
We observed a transient increase in the average brightness of the AFD neurons.
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