Photometric Parameters of the Canon EOS 6D Mark II Camera

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
V. O. Psaryov, Yu. I. Velikodsky, V. V. Konichek, I. E. Sinelnikov
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引用次数: 0

Abstract

The paper presents metrological parameters of the full-frame camera Canon EOS 6D Mark II’s photosensor. The working range of output signal levels is from 0.1 to 15 870 reference units DN. Depending on ISO parameter value, the sensor solarization takes place when the output signal reaches levels from 11 318 up to 15 870 DN. According to the data of laboratory experiments, it is shown that the range of the photosensor output signal in the area of its linear response to changes in the active light flux is 20.2–20.4 dB (ΔS is 107.3–11 595.6, 142.0–14 819.9, and 132.2–14 309.0 DN in R, G, and B channels of the sensor, respectively.) When using the logarithmic function of photosensor sensitivity, the range of its linear response increases to 38.2 dB (ΔS = 2.24–14 819.9 DN). The sensor’s local response in the R, G, and B channels to changes in active light flux is 558.63, 1164.0, and 691.37 DN/s at ISO 100; 1283.5, 955.29, and 206.9 DN/s at ISO 12 800; and 4263.6, 3119.2, 698.42 DN/s at ISO 40 000, respectively. The dependence of the sensor output signal level on the ISO value at an exposure time of Texp = 5.2 s remains linear within the entire range of ISO values from ISO 100 to ISO 102 400 in all spectral channels of the sensor when using a logarithmic dependence log Se(log ISO). In the case when the sensor transfer function is presented on natural numbers scale, the sensor linear response ranges in R, G, and B spectral channels differ and are ΔISOR,G,B = 1600–102 400, 2016–102 400, 3200–102 400 DN, respectively. In the highest informativeness areas of the linear sensor response ranges, the signal-to-noise ratio (SNR) of the output signal takes values from 5.0 dB to 34.5 dB (Rose’s criterion); accordingly, the signal increases from 4.5 to 12 560 DN and is controlled by the ISO level. Similarly, when the signal intensity depends on exposure duration, at ISO 100 within the sensor linear response ranges, the critical SNR values of output signals are 5.0 dB at Sav = 14.0 DN and 47.6 dB at Sav = 14 820 DN. At ISO 40 000, the SNR parameter takes values from 5.0 dB to 33.6 dB at signal levels of 160–230 and 13 522 DN, respectively. Taking into account the results of conducted analysis, the use of digital cameras with a CMOS sensor in photometric studies can be considered acceptable.

佳能EOS 6D Mark II相机的光度参数
介绍了佳能EOS 6D Mark II全画幅相机光敏元件的计量参数。输出信号电平的工作范围为0.1 ~ 15870参考单位DN。根据ISO参数值,当输出信号达到从11 318到15 870 DN的电平时,传感器太阳化发生。根据实验室实验数据,光敏传感器输出信号在其对有源光通量变化线性响应区域的范围为20.2 ~ 20.4 dB (ΔS在传感器的R、G、B通道分别为107.3 ~ 11 595.6、142.0 ~ 14 819.9、132.2 ~ 14 309.0 DN)。当使用光敏度的对数函数时,其线性响应范围增加到38.2 dB (ΔS = 2.24-14 819.9 DN)。在ISO 100下,传感器在R、G和B通道对主动光通量变化的局部响应分别为558.63、1164.0和691.37 DN/s;ISO 12800下的1283.5、955.29和206.9 DN/s;ISO 40000时分别为4263.6、3119.2、698.42 DN/s。当使用对数依赖对数Se(log ISO)时,传感器输出信号电平在曝光时间为Texp = 5.2 s时对ISO值的依赖关系在传感器所有光谱通道的ISO值从ISO 100到ISO 102 400的整个范围内保持线性关系。当传感器传递函数以自然数尺度表示时,传感器在R、G、B光谱通道的线性响应范围不同,分别为ΔISOR,G、B = 1600-102 400、2016-102 400、3200-102 400 DN。在线性传感器响应范围的最高信息量区域,输出信号的信噪比(SNR)的值为5.0 dB至34.5 dB (Rose准则);因此,信号从4.5增加到12560 DN,并由ISO电平控制。同样,当信号强度取决于曝光时间时,在传感器线性响应范围内的ISO 100下,Sav = 14.0 DN时输出信号的临界信噪比为5.0 dB, Sav = 14 820 DN时输出信号的临界信噪比为47.6 dB。在ISO 40000下,在160-230和13 522 DN的信号电平下,信噪比参数的值分别为5.0 dB到33.6 dB。考虑到所进行的分析结果,在光度研究中使用带有CMOS传感器的数码相机可以被认为是可以接受的。
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来源期刊
Kinematics and Physics of Celestial Bodies
Kinematics and Physics of Celestial Bodies ASTRONOMY & ASTROPHYSICS-
CiteScore
0.90
自引率
40.00%
发文量
24
审稿时长
>12 weeks
期刊介绍: Kinematics and Physics of Celestial Bodies is an international peer reviewed journal that publishes original regular and review papers on positional and theoretical astronomy, Earth’s rotation and geodynamics, dynamics and physics of bodies of the Solar System, solar physics, physics of stars and interstellar medium, structure and dynamics of the Galaxy, extragalactic astronomy, atmospheric optics and astronomical climate, instruments and devices, and mathematical processing of astronomical information. The journal welcomes manuscripts from all countries in the English or Russian language.
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