Warning: main(../inc_frame_start.html) [function.main]: failed to open stream: No such file or directory in /home/sbtron.co.kr/public_html/gps_rubidium_time/applications_Scientifics_calibration.html on line 7

Warning: main(../inc_frame_start.html) [function.main]: failed to open stream: No such file or directory in /home/sbtron.co.kr/public_html/gps_rubidium_time/applications_Scientifics_calibration.html on line 7

Warning: main() [function.include]: Failed opening '../inc_frame_start.html' for inclusion (include_path='.:/usr/local/lib/php') in /home/sbtron.co.kr/public_html/gps_rubidium_time/applications_Scientifics_calibration.html on line 7

Scientifics & calibration


Scientifics & calibration

    Test Equipment, Calibration and Scientific Labs

    Introduction
  • Atomic frequency standards, kept in metrological laboratories, are being used as ¡°primary¡± frequency and time standards for the calibration of secondary time/frequency standards. Secondary time standards may be used for local calibration of laboratory instruments, seismic data collection, or as a basic ingredient of the calibration services. These users may be interested only in standard frequency dissemination, thus releasing stringent accuracy requirement on the primary source, but usually they ask for traceability to international standard. Such traceability should be recognized by international accreditation bodies. Under following heading you will find more information about the few of the test equipment, calibration and scientific labs' applications:
  • Calibration Laboratories
  • In the last decade most countries have established dedicated networks of calibration laboratories in order to transfer the traceability from national standards to instruments used at production level. The accredited calibration laboratories must ensure the traceability of their metrological standards to the national primary standards. In case of time and frequency quantities, the calibration laboratories have their own frequency standard – cesiums or disciplined rubidium, and the Traceability is ensured by means of different techniques that range from Radio coded signals, Telephone time codes, LF broadcasts, television broadcasts and navigation satellite broadcasts. Frequency sources used as reference in calibration laboratories usually are rubidium frequency standards, GPS disciplined.
  • Calibration labs need a frequency reference and not a ¡°time tagging reference¡±, i.e. they must calibrate frequency or time interval standard, not dating devices. The relative uncertainty on the knowledge of the frequency is at the level of 10-13 at best.
    Considering the transmission path and the uncertainty sources depicted in the Figure 8.2-1, some requests may relaxed. Indeed in frequency comparison systems all the ¡°fixed¡± or stable delays may disregarded.
  • Over the past years, most of the calibration laboratories bought their own frequency standards, usually an atomic one based on the rubidium or cesium atom. To ensure traceability, then they had to buy also a comparison system as well. Therefore the devices and the amount of money were twofold. Now, with the availability on the market of rubidium frequency standards disciplined to GPS, the market of stand alone frequency standards has dramatically decreased.
  • High Resolution Counter
  • A frequency counter is an electronic instrument, or component of one, that is used for measuring frequency. Since frequency is defined as the number of events of a particular sort occurring in a set period of time, it is generally a straightforward to measure it.
  • Most frequency counters work by using a counter which accumulates the number of events occurring within a specific period of time. After a preset period (1 second, for example), the value in the counter is transferred to a display and the counter is reset to zero. If the event being measured repeats itself with sufficient stability of frequency and this frequency is considerably lower than that of the clock oscillator being used, the resolution of the measurement can be greatly improved by measuring the time required for an entire number of cycles, rather than counting the number of entire cycles observed for a pre-set duration (often referred to as the reciprocal technique).
    The internal oscillator which enables the frequency counter to measure time is called the timebase, and must be calibrated very accurately. If what is to be counted is already in electronic form, simple interfacing to the instrument is all that is required.
  • More complex signals may need some conditioning to make them suitable for counting. Most general purpose frequency counters will include some form of amplifier, filtering and shaping circuitry at the input. Other types of periodic events that are not inherently electronic in nature will need to be converted using some form of transducer. For example, a mechanical event could be arranged to interrupt a light beam, and the counter made to count the resulting pulses.
    Frequency counters designed for radio frequencies (RF) are also common and operate on the same principles as lower frequency counters.
  • Often they have more range before they overflow. For very high frequencies, many designs use a high-speed prescaler to bring the signal frequency down to a point where normal digital circuitry can operate. The displays on such instruments take this into account so they still read true. If the measured frequency is too high for any prescaler, a mixer and a local oscillator can produce a suitable frequency to measure.
  • The accuracy of a frequency counter is greatly dependent on the stability of its timebase. Highly accurate circuits are used to generate this for instrumentation purposes, usually using a quartz crystal oscillator within a sealed temperature-controlled chamber known as a crystal oven or OCXO (oven controlled crystal oscillator). For higher accuracy measurements, an external frequency reference tied to a very high stability oscillator such as a GPS disciplined rubidium oscillator may be used. Where the frequency does not need to be known to such a high degree of accuracy, simpler oscillators can be used. It is also possible to measure frequency using the same techniques in software in an embedded system. A CPU for example, can be arranged to measure its own frequency of operation provided it has some reference timebase to compare with.
  • High Performance Synthesizers
  • A frequency synthesizer is an electronic system for generating any of a range of frequencies from a single fixed timebase or oscillator. They are found in many modern devices, including radio receivers, mobile telephones, radiotelephones, walkie-talkies, CB radios, satellite receivers, GPS systems, etc.
  • Coherent techniques generate frequencies derived from a single, stable master oscillator. In most applications, crystal oscillator are common, but Rubidium frequency sources can be used in high performance requirements.
  • Special Test Equipment
  • With greater expansion of wireless cells the need for rubidium standards for field service and calibration is growing. For example, new handset designs must meet the standards expected by the consumer and that means carrying out earlier and more comprehensive development, design verification and regression testing. In some of the solutions rubidium frequencies standards are required as frequency references.
  • Space Exploration
  • How does NASA know where a spacecraft is in deep space? The spacecraft's precise range, velocity and angular position are determined by the aid of highly stable frequency standards. The range is determined using information from the propagation time of microwave radiation between an antenna on Earth and the spacecraft. The velocity is determined from the "doppler," i.e., by comparing the phase of the incoming carrier signal with that of a reference signal generated from the ground station frequency standard. The angular position is determined by very long baseline interferometry (VLBI) in which widely separated stations (in California, Spain and Australia) simultaneously receive signals from the spacecraft. Differences between times of arrival coupled with knowledge of the baseline vectors joining the station antennas provide direct geometric determination of the angles between the baseline vectors and the direction to the spacecraft. Hydrogen masers (see chapter 6) provide the best stability (~10-15) for the propagation times of interest, which typically range from minutes to hours. VLBI is also used for high resolution angular measurements in radio astronomy.
  •  

 

 

 

 



Warning: main(../inc_frame_end.html) [function.main]: failed to open stream: No such file or directory in /home/sbtron.co.kr/public_html/gps_rubidium_time/applications_Scientifics_calibration.html on line 233

Warning: main(../inc_frame_end.html) [function.main]: failed to open stream: No such file or directory in /home/sbtron.co.kr/public_html/gps_rubidium_time/applications_Scientifics_calibration.html on line 233

Warning: main() [function.include]: Failed opening '../inc_frame_end.html' for inclusion (include_path='.:/usr/local/lib/php') in /home/sbtron.co.kr/public_html/gps_rubidium_time/applications_Scientifics_calibration.html on line 233