The present disclosure relates to a photonic generator; more particularly, relates to generating an ultra-broad band white noise for w-band (75˜110 GHz) noise source testing and microwave band testing.
As disclosed in U.S. Pat. No. 3,600,703 and U.S. Pat. No. 6,844,786, a noise diode with a broad-band low-noise amplifier is used to obtain noise. But, its output power is not enough and its change in amplitude is too big to be used as a white noise source for noise figure measurement of mixer, gain measurement of ultra-wide band instrument, digital concord of ultra-wide band analog-digital converter, ultra-wide band pseudo-random bit generation, and ultra-wide band analog.
Signals detected from outer space celestial body usually have small radio power range. Since stars may move, interference pattern happens. Thus, interference pattern signals have to be measured for a long time and stability of the measuring device becomes very important. As a result, structure of the device may become very complex, which may need thermostatic antenna, high-quality receiving amplifier and some complex components. Another choice is a middle-class receiver accompanied with a calibration device. Since band of the signal emitted from the celestial body would not be narrow and the signal should be an ultra-broad band white noise with interference pattern, a big and complex calibration device is required. Furthermore, phase of the ultra-wide band source is not under control and, thus, it is difficult to simulate optical signal source of the outer space celestial body received by antennas. Hence, the prior arts do not fulfill all users' requests on actual use.
The main purpose of the present disclosure is to provide a photonic generator to generate an ultra-broad band white noise for w-band noise source testing and microwave band testing.
The second purpose of the present disclosure is to provide a device for failure detection of instantaneous all-band device, noise detection of instantaneous all-band amplifier and mixer, wide-band cipher transmission, pseudo-random bit generation, ADC dithering of analog-digital converter, saturation power test of wide-band optical communicator, system noise detection of millimeter-wave (MMW) receiver, and gain and phase detection of millimeter-wave interferometer.
To achieve the above purposes, the present disclosure is a photonic generator of ultra-wide band MMW, comprising a wide-band optical source, a MMW band photodetector and an optical fiber device, where the wide-band optical source forms and outputs a wide-band optical signal; where a part of the MMW band photodetector is located in a waveguide; where the MMW band photodetector is combined with a horn antenna through the waveguide; where the MMW band photodetector comprises an electrical signal input; a radio frequency (RF) choke connected with the electrical signal input; an optical detection switch connected with the RF choke; a fan-shaped broadband transition device connected with the optical detection switch; and an emitter connected with the optical detection switch; where the MMW band photodetector obtains a MMW ultra-wide band signal of RF from the wide-band optical signal; where the MMW band photodetector transfers the MMW ultra-wide band signal to the waveguide to be outputted by the horn antenna; where the optical fiber device is located on an optical path between the wide-band optical source and the MMW band photodetector; where the optical fiber device comprises a single mode fiber (SMF); and a lensed fiber connected with a probe head of the SMF at a side of the SMF; where the SMF is optically coupled with a fiber amplifier and an attenuator at another side of the SMF; where the wide-band optical signal is amplified by the fiber amplifier and attenuated by the attenuator; where an optical beam is expanded by the SMF to output a collimated optical beam to the lensed fiber to focus the optical beam; and where the wide-band optical signal is transferred to the lensed fiber from the SMF to be filled into the MMW band photodetector. Accordingly, a novel photonic generator of ultra-wide band MMW is obtained.
The present disclosure will be better understood from the following detailed descriptions of the preferred embodiments according to the present disclosure, taken in conjunction with the accompanying drawings, in which
The following descriptions of the preferred embodiments are provided to understand the features and the structures of the present disclosure.
Please refer to
The wide-band optical source 1 is used to generate and output a wide-band optical signal.
The MMW band photodetector 2 is set on an optical path of the optical fiber device 3. In
The optical fiber device 3 is set on an optical path between the wide-band optical source 1 and the MMW band photodetector 2, where the optical fiber device 3 comprises a single mode fiber (SMF) 31 and a lensed fiber 32; where the lensed fiber 32 is set at a side of the SMF 31 and is connected with a probe head of the SMF 31; and where the SMF 31 is optically coupled with a fiber amplifier (erbium-doped fiber amplifier, EDFA) 33 and an attenuator 34 at another side of the SMF 31. Thus, a novel photonic generator of ultra-wide band MMW is obtained.
In
The MMW band photodetector 2 is used to transform the wide-band optical signal obtained from the wide-band optical source 1 into an electrical signal in the optical detection switch 23 for generating low RF impedance through the RF choke 22. Then, according to a wide-band signal generated by the fan-shaped broadband transition device 24, a MMW RF signal originated from the wide-band optical signal is outputted to be transferred from the emitter 25 to the waveguide 26 and emitted from the horn antenna 27.
Please refer to
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On an electrical path, an electrical spectrum analyzer is used to obtain electrical spectrum of an optical filter, i.e. a flat-top filter or a Gaussian filter. In
Thus, the present disclosure has a simple structure for obtaining an ultra-broad band white noise having a smooth spectrum. Although the present disclosure uses W-band (75˜110 GHz) noise source only, the basic principle for the present disclosure is suitable for all wave bands, from centimeter wave band to sub-MMW band.
Please refer to
The MMW band photodetector 2 is used to transform the wide-band optical signal obtained from the wide-band optical source 1 into an electrical signal in the optical detection switch 23 to generate low RF impedance through the RF choke 22. Then, according to a wide-band signal generated by the fan-shaped broadband transition device 24, a MMW RF signal originated from the wide-band optical signal is outputted to be transferred from the emitter 25 to the waveguide 26 and emitted from the horn antenna 27.
Please refer to
On using, the present disclosure is set before an object as a light generator for analyzing the object.
Hence, after the present disclosure generates a wide-band optical signal through a wide-band optical source, the wide-band optical signal is passed through an optical fiber device and a NBUTC photodetector to obtain a W-Band white noise with shining light. The present disclosure can be used for failure detection of instantaneous all-band device, noise detection of instantaneous all-band amplifier and mixer, wide-band cipher transmission, pseudo-random bit generation, ADC dithering of analog-digital converter, saturation power test of wide-band optical communicator, system noise detection of MMW receiver, and gain and phase detection of MMW interferometer.
To sum up, the present disclosure is a photonic generator of ultra-wide band MMW, where a ultra-broad band white noise is generated with a simple structure for w-band noise source testing and, furthermore, microwave band testing.
The preferred embodiments herein disclosed are not intended to unnecessarily limit the scope of the disclosure. Therefore, simple modifications or variations belonging to the equivalent of the scope of the claims and the instructions disclosed herein for a patent are all within the scope of the present disclosure.
Number | Date | Country | Kind |
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099119632 | Jun 2010 | TW | national |