显像管亮均衡绿色调整 GDRV ; GD ; GREEN GAIN ; HI GREEN
显像管亮均衡蓝色调整 D-B ; HI BLUE ; B
显像管亮均衡调整 WHITE DRIVE
亮度均匀度 luminance uniformity ; uniformity of illuminance ; Brightness uniformity ; White Uniformity
平均亮度 nits ; mean brigtness ; mean intensity ; average luminance
显像管亮均衡蓝色调解 b ; d-b
显像管亮均衡赤色调整 D-R
亮度非均匀性 luminancenonuniformity
亮度均匀性 Luminance uniformity ; [电子] uniformity of luminance
均匀亮度技术 ULT
结果表明，只有基本暗孤子的频率抖动量（均方值）是亮孤子的一半，而其它小振幅暗孤子的频率抖动量大于亮孤子的频率抖动量。
The results show that only fundamental dark soliton has a frequency jitter half that of bright soliton, and small-amplitude dark soliton has a frequency jitter stronger than that of bright soliton.
亮的恒星通常有一个比较低的均方根，而暗的目标则具有较大的均方根。
Brighter stars will generally have a much lower RMS, but fainter objects will show larger values.
亮的恒星通常有一个比较低的均方根，而暗的目标则具有较大的均方根。
Brighter stars will generally have a much lower RMS but fainter objects will show larger values.
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