Sentence examples for a function of the baffle temperature from inspiring English sources

Fig. 6 Temperature distributions of deep space as a function of the baffle temperature.

Fig. 3 Distribution of the brightness temperature retrieved from the deep-space area in LIR images with m = 32 and n = 32 as a function of the baffle temperature.

The brightness temperature distribution of deep space as a function of the baffle temperature is shown in Fig. 3a, where images were obtained from March to September 2016 with m = 32 and n = 32.

The result is independent of the baffle temperature and consistent with the results of previous studies.

The temperature distribution after the correction converges to 181 K, which is independent of the baffle temperature.

Since infrared radiation from the baffle does not directly enter the UMBA, we assumed at the time of the design process that the image brightness was completely independent of the baffle temperature.

When more Venus images are acquired near periapsis, fluctuation of the baffle temperature will be systematically revealed enough to eliminate the residual background bias.

We must note that the behavior of the baffle temperature during periapsis passage is not completely understood because the solar incident angle varies rapidly there.

However, we were not aware of the background bias in 2010; the baffle temperature ranged up to 327.4 K at the time of observation.

The residual component was simply correlated with the baffle temperature and was successfully corrected by using a reference table based on the deep-space images acquired at different baffle temperatures on orbit.

Although temperatures of the baffle and the UMBA are not directly linked, the deep-space temperature in the images was correlated with the baffle temperature.