After compensation for differences in grain size, the creep rate was also found to decrease significantly with increasing Y3+ concentration.
After compensation, the measurement error of geomagnetic field has decreased from more than ten thousands nT to tens of nT.
After compensation, RMS error is reduced from 10797.962 nT to 15.309 nT when the big magnet and steel tube are deployed.
After compensation for sample loss caused by expected acoustic interference between the transmitter tags, the resulting dataset revealed that the receiver units collected 90 95% of the signals in both cages.
After compensation, the broadened peaks become now much narrower.
After compensation, the power loss is only 0.14 dB, which is less than the uncompensated value.
After compensation, the locations of the three spheres are corrected very well, as shown in Figure 9b.
After compensation, the reduction of phase difference is not obvious because of the 0.1λ limitation, but this does not overthrow the effectiveness of the compensation.
After compensation, the maximum phase difference appears in the center and at the edge, and the minimum is a ring in the aperture.
After compensation, the time constant of the recording system was in the range of 35 70 µs.
a Before compensation, PV=8.27nm, RMS=0.80nm b After compensation, PV=6.30nm, RMS=0.70nm Fig. 3 Compensated errors of angular variation kNθ. a N=6, PV=8.22nm, RMS=1.07nm b N=12, PV=6.30nm, RMS=0.81nm.
