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intercept point
The implemented mixers have a few decibels of conversion loss, a third-order input intercept point of a few dBm and a single sideband noise figure of about 15 dB.
      
The measured third order intercept point is 23 dBm and the 1 dB compression point is 10 dBm, both referred to the output.
      
The amplifier has a 2.4 dB noise figure with a -13 dBm third-order input intercept point, while drawing 5 mW from a 1.8 V power supply.
      
The front-end features a noise figure of 3.5?dB and an input-referred third-order intercept point of 5?dBm.
      
A 3rd-order intercept point can be calculated from the 3rd-order products, for predicting the level of inter modulation distortion.
      
Each intercept point between airplane trajectory and cloud boundary is with respect to the ground.
      
For the transmitter unit, the third-order output intercept point was 32.5 dBm, and the input intercept point was 2.5 dBm.
      
From this measurement, an output intercept point of 0 dBm can be extrapolated, approximately 6 dB above the compression point.
      
Feed-forward amplifiers are used extensively to increase inter-modulation intercept point and thereby decrease the inter-modulation products.
      
If so it returns intercept point as the new hit point.
      
If so, it returns intercept point as the new hit point.
      
It is found that the mixer with its buffer limits the receiver's cascade third-order intercept point to 8.5 dBm.
      
If such arrangements are used input third order intercept point will be degraded.
      
Input 1-dB compression point and input third-order intercept point analyses results are shown in figures 6 and 7, respectively.
      
Likewise, the input intercept point is slightly lower than expected.
      
More subtle is the same problem when posed as a spinning radar whose expected intercept point is to be estimated.
      
Nonlinear effects are described by definition of the compression point and the intercept point.
      
Once the histogram is transformed into a regression line it can be visualized as a point in the slope-intercept point space or Theta-Rho Hough space.
      
Output third-order intercept point was measured using a two-tone test.
      
Roughly speaking, a higher intercept point in dBm calls for an almost proportionally larger bias Veff in volts.
      
 

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