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EPC635 データシート(PDF) 51 Page - Espros Photonics corp |
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EPC635 データシート(HTML) 51 Page - Espros Photonics corp |
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51 / 97 page ![]() The following terms are used for the formulas: DTOF sine Distance in meters [m] c Speed of light e.g. 300'000'000m/s fLED LED/LD modulation frequency e.g. 20MHz DCS0 - DCS3 Sampling amplitude [LSB] φ Phase shift caused by the time-of-flight [rad] DOFFSET Offset compensation [m] In the real case of 4x DCS samples used with π-delay matching algorithm, the time of flight calculation will be: [1] tTOF sine [sec ] = 1 2 π f LED ⋅ [π + atan2(DCS2−DCS0, DCS3−DCS1)] + t OFFSET then, the distance calculation will be (c is the speed of light): [2] DTOF sine [m] = c 2 ⋅ 1 2 π fLED ⋅ [π + atan2(DCS2−DCS0, DCS3−DCS1)] + D OFFSET 2π phase wrap-around If DTOF sine > DUnambiguity: DTOF = DTOF sine - DUnambiguity, if DTOF sine < DUnambiguity: DTOF = DTOF sine + DUnambiguity, else: DTOF = DTOF sine DUnambiguity [m] = c 2 ⋅ 1 f LED Based on the ideal case of 2x DCS samples (without any offsets), the time of flight may be computed as follows: [3] tTOF sine [sec] = 1 2 π f LED ⋅ [π + atan2(−DCS0, −DCS1)] then, the distance calculation is: [4] DTOF sine [m] = c 2 ⋅ 1 2 π fLED ⋅ [π + atan2(−DCS0, −DCS1)] Sine mode: Quality of the measurement result The epc635 provides information on the quality and the validity of the received optical signal. This reflects the confidence level of the mea - surement result. The better the received signal, the better and more precise the distance measurement will be. Each distance measurement of every pixel has its own validity and quality. The primary quality indicator for the measured distance data is the peak-to-peak amplitude value of the received modulated light ATOF sine PP. The amplitude is in direct relation ship to the distance noise: Refer to Figure 5. After each measurement, this needs to be calculated from the DCSx values delivered by the chip. This amplitude value is the feedback pa- rameter that is used to set the integration time for the next measurement. [5] ATOFsinePP = √(DCS2−DCS0)2 4 + (DCS3−DCS1) 2 4 Amplitude ATOF sine PP Classification Action < 25 LSB Weak illumination Too less signal for an accurate measurement: Increase integration time for the next measurement 25 … 100 LSB Enough signal for a useful measurement Distance noise approx. 4 times higher than the optimum: No action necessary. See note below 100 … 2'000 LSB Good signal strength No action necessary. See note below > 2'000 LSB Overexposed Decrease integration time for the next measurement. See note below Table 28: Signal amplitude versus classification Note: Generally, the higher the received signal, the better and more precise the distance measurement will be. However, it is good practice to control the integration time such that an amplitude value between 200 ... 1'000 LSB is achieved. Higher values will only slow down the ac- quisition rate due to longer integration times, but are not significantly improving signal to noise ratio. © 2017 ESPROS Photonics Corporation Characteristics subject to change without notice 51 / 97 Datasheet_epc635-V1.02 www.espros.com |
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