How to Correct for Spectral Errors of Popular Light Sources
可以使用波长相关的计算可以近似光谱误差,该计算考虑了量子传感器的光谱响应,校准光源的光谱输出和测量光源的光谱输出。下表显示了许多不同流行灯源的计算理论谱误差和相应的校正因子。频谱误差相对于每个传感器的校准源计算(SQ-110被校准为清晰的太阳光,SQ-120和SQ-500被校准为4100K冷却的白色荧光T5灯)。
To correct for spectral error multiply your measured value by the correction factor (CF) associated with your light source. For example, if you are using an SQ-120 under a Blue LED (448nm), which has a spectral error of -12.7 and a CF of 1.15, and you measured 115 µmol m-2s-1, you would multiply your measurement of 115 µmol m-2s-1by the CF 1.15 to get 132.3 µmol m-2s-1(115 x 1.15 = 132.3).
SQ-110 correction factors apply to sun calibrated models SQ-110, 212, 214, and 215, and models SQ-420, MQ-100, 200, and 210 when in SUN setting.
SQ-120 correction factors apply to electric calibrated models SQ-120, 222, 224, and 225, and models SQ-420, MQ-100, 200, and 210 when in ELEC setting.
SQ-500 correction factors apply to models SQ-500 and 520, and MQ-500, 501, and 510.
This information is also available as aninteractive tool, which allows users to upload their own lighting spectrum.