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AD7708 数据表(PDF) 17 Page - Analog Devices |
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AD7708 数据表(HTML) 17 Page - Analog Devices |
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17 / 44 page ![]() REV. 0 AD7708/AD7718 –17– FREQUENCY – Hz 0 –80 –160 0 100 10 20 30 40 50 60 70 80 90 –20 –40 –120 –140 –60 –100 SF = 255 OUTPUT DATA RATE = 5.35Hz INPUT BANDWIDTH = 1.28Hz 50Hz REJECTION = –93dB, 50Hz 1Hz REJECTION = –93dB 60Hz REJECTION = –74dB, 60Hz 1Hz REJECTION = –68dB Figure 7. Filter Profile with SF = 255 FREQUENCY – Hz 0 –80 –160 0 100 10 20 30 40 50 60 70 80 90 –20 –40 –120 –140 –60 –100 SF = 69 OUTPUT DATA RATE = 19.8Hz INPUT BANDWIDTH = 4.74Hz FIRST NOTCH = 9.9Hz 50Hz REJECTION = –66dB, 50Hz 1Hz REJECTION = –60dB 60Hz REJECTION = –117dB, 60Hz 1Hz REJECTION = –94dB Figure 8. Filter Profile with Default SF = 69 Giving Filter Notches at Both 50 Hz and 60 Hz FREQUENCY – Hz 0 –80 –160 0 100 10 20 30 40 50 60 70 80 90 –20 –40 –120 –140 –60 –100 SF = 68 OUTPUT DATA RATE = 20.07Hz INPUT BANDWIDTH = 4.82Hz 50Hz REJECTION = –74dB, 50Hz 1Hz REJECTION = –54.6dB 60Hz REJECTION = –147dB, 60Hz 1Hz REJECTION = –101dB Figure 9. Filter Profile with SF = 68 ADC NOISE PERFORMANCE CHOP ENABLED ( CHOP = 0) Tables II to V show the output rms noise and output peak-to- peak resolution in bits (rounded to the nearest 0.5 LSB) for a selection of output update rates. The numbers are typical and generated at a differential input voltage of 0 V with AVDD = DVDD = 5 V and using a 2.5 V reference. The output update rate is selected via the SF7–SF0 bits in the Filter Register. It is important to note that the peak-to-peak resolution figures repre- sent the resolution for which there will be no code flicker within a six-sigma limit. The output noise comes from two sources. The first is the electrical noise in the semiconductor devices (device noise) used in the implementation of the modulator. Secondly, when the analog input is converted into the digital domain, quantization noise is added. The device noise is at a low level and is independent of frequency. The quantization noise starts at an even lower level but rises rapidly with increasing frequency to become the dominant noise source. The numbers in the tables are given for the bipolar input ranges. For the unipolar ranges the rms noise numbers will be the same as the bipolar range, but the peak-to-peak resolution is now based on half the signal range which effectively means losing one bit of resolution. |
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