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Various illumination angle combinations among the three channels yield different displacement sensitivity matrices.
The mirrors also provide the fine adjustment of the illumination angle.
The illumination angle differences among the three channels result in different displacement sensitivity coefficients.
Furthermore, we demonstrate how illumination angle and hence seismic acquisition design is critical to avoid imaging artefacts.
Two mirrors projected the light over the sample and provided the fine adjustment of the illumination angle.
The illumination angle does have an effect on where the plasma blobs detach from Titan's ionosphere and their trajectories afterwards.
Similar(19)
Dual orbiter systems can provide multi-offset data that illuminate the target object from many different illumination angles.
The illumination angles will be discussed later.
In both types, the magnitudes of the illumination angles are equal, but the directions differ.
The kernel model may be a useful tool to quantify the LST uncertainties associated with viewing and illumination angles.
The other two channels follow the same principle, but have different illumination angles and reference beam incident angles.
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