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For nearby objects, these two images will look just the same, since T will be very small due to the large speed of light.
The difference in Id2 values between durable vs. non-durable mudrocks can sometimes be very small, due to the fact that fragments of material retained in the test drum can be larger than 2 mm making the slake durability test inadequate to quantify durability of mudrocks.
This is not surprising since in some cases the coefficients of the linear combination may be very small (due to the random draw of these coefficients in these experiments) which makes the detection very challenging.
It should be noted that the estimation of transmitter and receiver IQ imbalance gain parameters involve the division operation per tone, since the frequency response of a certain tone can be very small due to deep channel fading, the estimated IQ imbalance gain parameters may then not be accurate if the quantization level is limited or for poor signal-to-noise conditions.
In particular, the magnetic anisotropy is likely dominated by shape anisotropy, and the contribution from magneto-crystalline anisotropy can be assumed to be very small due to the lack of texturing.
Also, measuring doubles for the Q3 mutants presents a technical challenge because the double event second peaks can be very small due to the lowered forces, and difficult to identify.
Similar(54)
Or, perhaps the amount of pollutants trapped by the star was very small due to its high ejection speed in the supernova.
Under same impact condition, the effective protection space of empty hemispherical shells is very small due to its larger vertex displacement.
After 20 h, further weight gains of all these specimens are very small, due to more stable α-Al2O3 growth and transformation from θ-Al2O3 to α-Al2O3.
Even though the change in the star's position is very small due to the tug of the planet, this tiny difference may be detectable through a close study of the star's position over time.
In particular, model uncertainties in the definition of two-neutron drip line at Z∼54, N= 126 and Z∼82, N= 184 are very small due to the impact of spherical shell closures at N= 126 and 184.
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Justyna Jupowicz-Kozak
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