Mirror image synthetic aperture radiometer correction method based on external source with known orientation
A comprehensive aperture and correction method technology, applied in radio wave measurement systems, instruments, etc., can solve the problems of microwave radiation imaging quality degradation, complex correction operation, and reduced imaging quality, so as to avoid errors, simplify correction steps, and improve imaging accuracy Effect
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Embodiment 1
[0081] Example 1: Brightness temperature image of a point source scene
[0082] In this embodiment, the calibration method of the mirror synthetic aperture radiometer based on the external source with known orientation is simulated and verified, Figure 4 The array used in the simulation is a 24-element rectangular array.
[0083] Specific steps are as follows:
[0084] (1) For a 24-element rectangular array, the mirror synthetic aperture system collects the noise source scene radiation signal;
[0085] (2) Gather the correction data of the external source, and calculate the error of the relevant output of the collected external source;
[0086] (3) The brightness temperature image of the noise source without correction, such as Figure 5 ;
[0087] (4) Correct the noise source signal data with the calculated error of the correlation output of the external source to obtain the corrected noise source brightness temperature image, as shown in Image 6 .
[0088] From the s...
Embodiment 2
[0089] Example 2: The brightness temperature image of the source scene in a stepwise exhibition
[0090] In this embodiment, a simulation verification is carried out for the calibration method of the mirror synthetic aperture radiometer based on an external source with a known orientation.
[0091] Specific steps are as follows:
[0092] (1) For a 24-element rectangular array, the mirror synthetic aperture system collects the noise source scene radiation signal;
[0093] (2) collecting external source correction data, and finding the phase error of the relevant output of the collected external source;
[0094] (3) The brightness temperature image of the stepped source without correction, such as Figure 7 ;
[0095] (4) Use the calculated error of the correlation output of the external source to correct the step spread source signal data to obtain the corrected step spread source brightness temperature image, as shown in Figure 8 .
[0096] From the simulation results, ...
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