Several hypotheses could explain these effects: atmospheric scattering, surface photometric effects, shift of the spatial registration or calibration.
It is difficult to recover the motion field from a real-world footage given a mixture of camera shake and other photometric effects.
For the first time, we performed an error evaluation on band depths and band centers introduced by the applied method, which is relevant for comparison of spectral parameters of Ceres regions and to better interpret mineralogy and photometric effects.
Thus, comets do not produce a photometric opposition effect, i.e., a non-linear decrease of apparent magnitude near backscattering.
We aim to utilize these results in multiple-scattering studies, such as the interpretation of polarimetric and photometric phase effects of asteroids and other atmosphereless solar-system objects.
For the examination of properties of objects on color-color planes, the effect of photometric errors is a matter of concern.
In Pollo et al. (2010a), we have examined the effect of photometric errors on the boundary of the star-galaxy classification, and found that this affects the position of the boundary on the color-color plane, but not so significantly that it would change quantitative conclusions.
The effect of the limited photometric sensitivity of the instrument and the limited information on the angular structure of the magnetic field tubes are considered.
Figure 1 Effect of pH on photometric absorbance and fluorometric quenching studies.
Thus it is necessary to subtract its effect from the observed images for both morphological and photometric purposes.
Here the authors show the operational environment of asteroid Bennu, validate its photometric phase function and demonstrate the accelerating rotational rate due to YORP effect using the data acquired during the approach phase of OSIRIS-REx mission.
