NIST statement on Daylight Saving Time (DST) problem
nist.gov
FOR IMMEDIATE RELEASE 9 March 2013 CONTACT: James Burrus, 303-497-4789 or 720-982-6222 Some older radio-controlled clocks may adjust for Daylight Saving Time early. Due to an unexpected technical issue, some older radio controlled clocks may have made the change to Daylight Saving Time (DST) up to a day earlier than intended. Daylight Saving Time begins on Sunday March 10, 2013, at 2:00 am local time. At that time, clocks should move ahead one hour (to 3:00 am local time) in areas observing DST. Radio-controlled clocks and watches (colloquially known as "atomic clocks") receiving time signals from the National Institute of Standards and Technology's radio station WWVB should make this time change automatically. However, this year some older versions of radio-controlled clocks may have made the change early. The WWVB time broadcast includes "warning" information that DST changes will be coming in the next day. Some older radio-controlled clocks may not have correctly interpreted this advance notice and instead made the switch to DST too early. All radio-controlled clocks, including those that may have made the DST switch early, should be working properly by the time DST officially begins on Sunday morning. NIST regrets any inconvenience caused by the error. Enhanced WWVB Broadcast Format Change Since October 29, 2012 at 1500 UTC (9:00 AM MDT), NIST Radio Station WWVB has been broadcasting a phase modulation (PM) time code protocol that has been added to the legacy AM/pulse-width-modulation signal. This enhancement to the broadcast, which has been tested throughout 2012, provides significantly improved performance in new products that are designed to receive it. Existing radio-controlled clocks and watches are not affected by this enhancement, and continue to work as before. A detailed technical description of the new format can be found here. Disciplined oscillator products that track and lock to the 60 kHz WWVB carrier and were designed to work as frequency standards, will not work with the PM signal and will now become obsolete. A few radio controlled clocks that used information from the carrier – specifically the Spectracom NetClock and receivers manufactured by True Time during the 1970s and 1980s – will no longer be able to read the time code and will also be obsolete. To allow users of these receivers to migrate to new products, the plan for implementing the new modulation protocol includes a transition period that will extend until at least March 21, 2013. During the transition period, the PM signal will be turned off for 30 minutes twice per day, at noon and midnight Mountain Standard Time (MST), allowing carrier tracking receivers to temporarily acquire the legacy signal. The new PM signal may also be turned off occasionally for further testing as needed. For more information, contact Broadcast Manager John Lowe at john.lowe@nist.gov or 303-497-5453. Station Information NIST radio station WWVB is located on the same site as WWV near Fort Collins, Colorado. The WWVB broadcasts are used by millions of people throughout North America to synchronize consumer electronic products like wall clocks, clock radios, and wristwatches. In addition, WWVB is used for high level applications such as network time synchronization and frequency calibrations. Signal Description WWVB continuously broadcasts digital time codes on a 60 kHz carrier that may serve as a stable frequency reference traceable to the national standard. The time codes are synchronized with the 60 kHz carrier and are broadcast continuously in two different formats at a rate of 1 bit per second using pulse width modulation (PWM) as well as phase modulation (PM). In the first of the two formats, based on PWM, which has been in use for several decades, the carrier power is reduced by 17 dB at the start of each second and restored to full power 0.2s later for a binary "0", 0.5s later for a binary "1", or 0.8s later to convey a position marker. The time code contains the year, day of year, hour, minute, UT1 time correction, and flags that indicate the status of Daylight Saving Time, leap years, and leap seconds, as listed here WWVB time code format, and detailed here: NIST Time and Frequency Services In the second of the two formats, based on PM, which has been in use since October 29, 2012, binary-phase-shift-keying (BPSK) modulation is used, wherein the carrier's phase is unaffected when conveying a "0", and is inverted (i.e. 180-degree shifted) when conveying "1". This time code, also operating at a rate of 1 bit/sec, is delayed by 0.1s with respect to the first time code described above, such that 180-degree transitions in the carrier phase can only occur 0.1s after the 17dB power reduction that is created by the pulse-width-modulation. The data content, physical properties and scheduling features of this BPSK time code may be found here: Enhanced WWVB Broadcast Format Antenna and Transmitters WWVB uses two identical antennas that were originally constructed in 1962, and refurbished in 1999. The north antenna was originally built for the WWVL 20 kHz broadcast (discontinued in 1972), and the south antenna was built for the WWVB 60 kHz broadcast. The antennas are spaced 857 m apart. Each antenna is a top loaded monopole consisting of four 122-m towers arranged in a diamond shape. A system of cables, often called a capacitance hat or top hat, is suspended between the four towers. This top hat is electrically isolated from the towers, and is electrically connected to a downlead suspended from the center of the top hat. The downlead serves as the radiating element. North antenna coordinates: 40° 40' 51.3" N, 105° 03' 00.0" W South antenna coordinates: 40° 40' 28.3" N, 105° 02' 39.5" W Ideally, an efficient antenna system requires a radiating element that is at least one-quarter wavelength long. At 60 kHz, this becomes difficult. The wavelength is 5000 m, so a one-quarter wavelength antenna would be 1250 m tall, or about 10 times the height of the WWVB antenna towers. As a compromise, some of the missing length was added horizontally to the top hats of this vertical dipole, and the downlead of each antenna is terminated at its own helix house under the top hats. Each helix house contains a large inductor to cancel the capacitance of the short antenna and a variometer (variable inductor) to tune the antenna system. Energy is fed from the transmitters to the helix houses using underground cables housed in two concrete trenches. Each trench is about 435 m long. A computer is used to automatically tune the antennas during icy and/or windy conditions. This automatic tuning provides a dynamic match between the transmitter and the antenna system. The computer looks for a phase difference between voltage and current at the transmitter. If one is detected, an error signal is sent to a 3-phase motor in the helix house that rotates the rotor inside the variometer. This retunes the antenna and restores the match between the antenna and transmitter. There are three transmitters at the WWVB site. Two are in constant operation and one serves as a standby transmitter that is activated if one of the primary transmitters fail. Each transmitter consists of two identical power amplifiers which are combined to produce the greatly amplified signal sent to the antenna. One transmitter delivering an amplified time code signal into the north antenna system, and one transmitter feeds the south antenna system. The time code is fed to a console where it passes through a control system and then is delivered to the transmitters. Using two transmitters and two antennas allows the station to be more efficient. As mentioned earlier, the WWVB antennas are physically much smaller than one quarter wavelength. As the length of a vertical radiator becomes shorter compared to wavelength, the efficiency of the antenna goes down. In other words, it requires more and more transmitter power to increase the effective radiated power. The north antenna system at WWVB has an efficiency of about 50.6%, and the south antenna has an efficiency of about 57.5%. However, the combined efficiency of the two antennas is about 65%. As a result, each transmitter only has to produce a forward power of about 54 kW for WWVB to produce its effective radiated power of 70 kW. Performance The frequency uncertainty of the WWVB signal as transmitted is less than 1 part in 1012. If the path delay is removed, WWVB can provide UTC with an uncertainty of about 100 microseconds. The variations in path delay are minor compared to those of WWV and WWVH. When proper receiving and averaging techniques are used, the uncertainty of the received signal should be nearly as small as the uncertainty of the transmitted signal. Other Information about WWVB ...
2013年3月11日 凌晨2点11分
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