Microchip 5071A Datasheet

5071A
Primary Frequency Standard
Features
Easy to use with automatic startup and
intuitive menu structure
Fast warm up ±5.0 x 10
minutes or less for high-performance tube
Integrated clock and message displays
outputs with easy access at front and rear
Automatic synchronization of 1PPS signal
Remote interface and control including
alarm output
Meets requirements in the new ITU-T
G.811.1 ePRC standard
Benets
Maintains exceptional accuracy and
stability even in unstable environments—
unsurpassed stability in the lab or eld
Accuracy ±1.0 x 10
mance; ±5.0 x 10
Stability ≤1.2 x 10
mance; ≤5.0 x 10
(for 1 second averaging time)
Environmental stability ±1.0 x 10
standard performance; ±8.0 x 10 high performance (frequency change for any combination of environmental conditions)
Long-term stability ≤5.0 x 10
dard performance; ≤1.0 x 10
performance (for 5-day averaging time)
Proven reliability with an average mean
time between failures (MTBF) of greater than 160,000 hours
Full traceability to NIST
AC and DC input and internal battery
back-up
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accuracy in 30
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for standard perfor-
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for high performance
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for standard perfor-
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for high performance
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for
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for
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for stan-
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for high
The 5071A primary frequency standard has the accuracy and stability you need
for both laboratory and eld applications. A stability specication for 30-day aver-
aging time means the 5071A will keep extremely predictable time and phase for long periods. Further, the 5071A can be used for long-term averaging of noisy signals such as GPS.
The 5071A is easy to use. No more manual start-up steps or complicated adjustments—everything is automatic.
A logical menu structure simplies front
panel operations, selections, and status reporting. Remote control features tailor the 5071A for complete operation and manageability in virtually any location.
The instrument is a direct descendant of and replacement for the veteran 5060A, 5061A, and 5061B cesium standards. This innovative product is the result of more than 35 years of experience in the precision frequency standard business.
Frequency and Timing
Meeting the Needs of Leading­Edge Metrology and Calibration Labs
Timekeeping and National Standards Laboratories verify the stability and accu­racy of their in-house cesium standards to Coordinated Universal Time (UTC), provided by the Bureau International des Poids et Mesures (BIPM) in Paris. A standard’s accuracy and reliability determine the quality of service these timekeeping labs provide. Of even greater concern is the stability of a standard. Stability directly aects a laboratory’s abil­ity to deliver timekeeping and calibration services to its clients.
The 5071A oers exceptional stability and is the rst cesium standard to specify
its stability for averaging times longer than one day. The instrument takes into account environmental conditions that
can heavily inuence a cesium standard’s
long-term stability. Digital electronics continuously monitor and optimize the instrument’s operating parameters.
Thus, the 5071A’s response to environ­mental conditions such as temperature and humidity are virtually eliminated. The 5071A primary frequency standard maintains its accuracy and stability, even in unstable environments.
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Satellite Communications
Stable frequency generation is required to transmit and receive signals properly between ground terminals and
communication satellites. Frequency exibility is also needed to adjust for satellite-to-satellite carrier-frequency dierences. The 5071A’s state-of-the-art technology produces oset and
primary frequencies with the same guaranteed stability.
Exceptional Accuracy
The intrinsic accuracy of the improved cesium beam tube (CBT) assures that any high performance 5071A will power up to within ±5.0 x 10 This is achieved under full environmental conditions in 30 minutes or less, and without the need for any adjustments or alignments.
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of the accepted standard for frequency.
For secure communications, precise timing synchroniza­tion ensures that encrypted data can be recovered quickly. Frequency-agile signals also require exact synchronization between transmitter and receiver during channel hops.
The 5071A automates the synchronization to any external 1PPS signal, greatly simplifying this aspect of satellite communications.
The 5071A and GPS
The 5071A primary frequency standard can work very well with a GPS timing receiver to produce and maintain highly accurate time and frequency.
The GPS system provides accurate time, frequency, and location information worldwide by means of microwave radio broadcasts from a system of satellites. Timing accuracy for the GPS system is based, in large part, on the accuracy and stability of a number of 5071A primary frequency standards. These standards are maintained by the GPS system, the US Naval Observatory, and various timing laboratories around the world that contribute to UTC, the world time scale.
Because of their accurate time reference, GPS signals processed by a good GPS timing receiver can provide highly accurate time and frequency outputs. However, since GPS receivers rely on very low level microwave signals from the satellites, they sometimes lose accuracy because of interfering signals, local antenna problems, or bad satellite data.
In spite of these problems, a GPS timing receiver can be an excellent backup and reference to a local 5071A primary frequency standard. The GPS receiver provides an indepen­dent reference that can be used to verify the accuracy of a caesium standard, or it can be used as a temporary backup should the cesium standard need repair. The local 5071A standard has better stability, better output signal quality, and is not perturbed by interfering signals, intermittent signal loss, or bad satellite data.
With these characteristics, the synergy created by combin­ing a good quality GPS timing receiver and a 5071A primary frequency standard can produce a highly robust, inexpensive, and redundant frequency and time system.
Unsurpassed Stability
The 5071A high-performance cesium beam tube guarantees stability to be better than 1.0 x 10
ve days or greater. The 5071A is the rst cesium standard
to specify stability for averaging times longer than 1.0 x 105 seconds (approximately one day).
The 5071A is also the rst cesium standard to specify and guarantee a icker oor. Flicker oor is the point at which the standard’s stability (σy (2, τ)) does not change with longer averaging. The high performance 5071A icker oor is guar-
anteed to be 1.0 x 10
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or better. Long-term measurements
at the National Institute of Standards and Technology (NIST)
show that the icker oor is typically better than 5.0 x 10
Unstable environments are normal for many cesium standard applications. The 5071A features a number of microproces­sor controlled servo loops which allow it to virtually ignore
changes in temperature, humidity, and magnetic elds.
The 5071A delivers exceptional performance over very long periods of time, greatly increasing the availability of critical time and frequency services. Actual measurements made at NIST have demonstrated that a 5071A with the high­performance CBT will drift no more than 5.0 x 10 entire life of the CBT.
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for averaging times of
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over the
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.
Traditional Reliability
The 5071A has demonstrated an average mean time be­tween failures (MTBF) of greater than 160,000 hours since its
introduction in 1992. This data is based on actual eld repair
data. Backing up this reliability is a 10-year warranty on the standard long-life cesium beam tube and a 5-year warranty for the high performance tube.
Complete repair and maintenance services are available at our repair center in Beverly, Massachusetts.
Full Traceability to NIST
Microchip provides NIST traceability to the accuracy measure­ments made on every 5071A. Traceability to NIST is maintained through the NIST-supplied Time Measurement and Analysis System (TMAS). This service exceeds the requirements of
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