## Abstract In this paper a solution for the focalization of the new 40‐m radiotelescope at the observatory of the Centro Astronómico de Yebes (CAY) in Guadalajara, Spain, is presented. Quasi‐optics theory is used in this paper for the propagation analysis of the beams through the different optics
Error correction in the Gaussian beam telescope applicated to the new 40 m radiotelescope of Centro Astronómico de Yebes
✍ Scribed by E. García; C. O'Sullivan; E. Rajo; J. L. Vázquez
- Book ID
- 102519393
- Publisher
- John Wiley and Sons
- Year
- 2006
- Tongue
- English
- Weight
- 280 KB
- Volume
- 48
- Category
- Article
- ISSN
- 0895-2477
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✦ Synopsis
2 ) should be the same as that (a 2 A 2 A 3 ) of lower injected-generation term (2 1 Ϫ 2 ). The phases between lower IMD3 and lower injected-generation term need to be out-of-phase. The phase of harmonic signal was adjusted and optimized by using RF phase shifter. The same logic was applied to reduce upper IMD3 (2 2 -1 : 1.3 GHz) with the magnitude/phase control of harmonic (2.4 GHz) in the feedback loop.
As shown in Figure 3(b), intermodulation distortion products were significantly reduced in 1 GHz bands. The experimental result showed that the CNR enhancement of 12 dB when compared with free-running operation was achieved by optimization of RF magnitude and phase. Figure 4 shows the received RF power of the fundamental signal (1.2 GHz) and IMD3 (1.3 GHz) with variation of input RF power for both free-running and the proposed schemes. As expected, the SFDR was improved from 72 to 81 dB Hz 2/3 by 9 dB with the proposed scheme.
4. CONCLUSION
A novel technique of intermodulation products reduction using the feedback harmonic injection in DFB LD for RoF link was proposed. The proposed scheme is mainly composed of a photodiode, two BPF, and RF phase shifter/amplifier. This scheme is capable of suppressing IMD up to 12 dB when compared with that of free-running DFB LD for RoF transmission link.
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