研究目的
Design and measurement of a low-phase-noise space quali?ed microwave source for the cold atom clock experiment in space CAC operating in the Tiangong-2 Chinese space laboratory.
研究成果
The design of the microwave source of the CACES cold atom clock is robust, compact, and of low phase noise. The flight model and engineering qualified model have successfully passed all the space qualification tests while their performance remained unchanged. The microwave source was also tested on a fountain clock and showed a very good frequency instability limitation.
研究不足
The microwave source must be able to withstand the shock and random vibration during the launching stage of the rocket and pass the mechanical, thermal, and electromagnetic compatibility tests specified for space missions.
1:Experimental Design and Method Selection:
The microwave source consists of two parts: the reference oscillator and the frequency synthesis chain. A 5 MHz BVA type quartz oscillator is selected for the reference oscillator. A two-step phase-lock-loop (PLL) architecture was used in the frequency synthesis chain.
2:Sample Selection and Data Sources:
The output microwave signal benefits from both the ultra-high close-in spectral purity of the reference oscillator and the low phase noise level of the PLL at frequencies far from the carrier.
3:List of Experimental Equipment and Materials:
Includes a 5 MHz BVA type quartz oscillator, a low noise reference oscillator (LNRO), a power combiner, a frequency multiplier, a power splitter, a phase lock loop, an oven-controlled quartz oscillator, an amplifier, a coupler, a step recovery diode, a band pass filter, a direct digital synthesizer, a dielectric resonator oscillator, a switch, and an attenuator.
4:Experimental Procedures and Operational Workflow:
The 5 MHz signal of the reference oscillator is multiplied to 100 MHz, which is used to phase-lock a 100 MHz oven-controlled quartz oscillator. The 100 MHz signal is multiplied to 200 MHz, which is amplified and then sent to a 10 dB directional coupler. The coupled output is split into three signals. One signal is used to drive a direct digital synthesizer and the other two signals are sent to two mixers for frequency downconversion.
5:Data Analysis Methods:
The phase noise of the microwave source was characterized by comparing two identical devices using a phase noise test system.
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Direct digital synthesizer
AD9852
Analog
Driven by the 200 MHz signal for frequency synthesis
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Phase noise test system
E5505A
Agilent
Characterizes the phase noise of the microwave source
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BVA oscillator
8607
Oscilloquartz S. A.
Reference oscillator for the microwave source
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Low noise reference oscillator
LNRO-5 MHz
Orolia, Switzerland SA
Redundant oscillator for the BVA oscillator
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Power combiner
HE021-2B
CETC-13
Combines the output of the LNRO with that of the BVA oscillator
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Frequency multiplier
FS100-5
SpectraDynamics
Multiplies the 5 MHz signal of the reference oscillator to 100 MHz
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Oven-controlled quartz oscillator
OXLN512D-100M
CETC-13
Phase-locked by the 100 MHz signal to improve the phase noise level at high Fourier frequencies
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Mixer
MDB-12
CETC-13
Used for frequency downconversion
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Step recovery diode
HE1034
CETC-13
Comb generator for frequency synthesis
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Band pass filter
5FS10-7000
CETC-13
Filters the comb signal to isolate the 7 GHz harmonic
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Dielectric resonator oscillator
DRO-7034
CETC-13
Produces a 7.034 GHz signal for frequency downconversion
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RF switch
HE017
CETC-13
Switches off the microwave signal to avoid significant microwave leakage
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Digital attenuator
HE751-14
CETC-13
Adjusts the power of the microwave signal with a resolution of 0.25 dB
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