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Finally we calculate the energy shift due to the spacecraft motion for each individual looking direction of the instrument.
The orientation of an antenna array is represented by the normal looking direction of the array defined as follows.
We use γ q to represent the normal looking direction for the q-th BS, as a counterclockwise angle relative to the x-axis.
Define a normal looking direction of an antenna array as a main radiation direction when the phase shifts of all the antenna elements are zero.
The normal looking direction is determined by first setting the phase shifts of all the antenna elements to be zero and then determining the main radiation direction that is closest to the direction of arrival of the MD.
While the linear antenna array of an AP has two normal looking directions, we shall be interested in only the one that is closest to the direction of arrival of the MT. For the q-th AP, we denote the counter-clockwise angle of the normal looking direction relative to the x-axis as γ q.
Similar(51)
Gain margins for off-broadside looking directions are found to be even wider.
The 400- m2 region of interest for localization and the normal looking directions of the antenna arrays of four APs located at the corners.
The 400- m2 region of interest for localization and the normal looking directions of the antenna arrays of four BSs located at the corners.
This condition causes look direction error.
In the monopulse beamforming, the pattern look direction must be exactly known.
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