Academia.edu no longer supports Internet Explorer.
To browse Academia.edu and the wider internet faster and more securely, please take a few seconds to upgrade your browser.
2003
https://doi.org/10.1109/FREQ.1999.840728…
7 pages
1 file
NET, in collaboration with the Jet Propulsion Laboratories (JPL), the University of Colorado, Politecnico di Torino and Harvard Smithsonian Center for Astrophysics (SAO) is building a laser-cooled cesium (Cs) atomic clock for flight on the Intemational Space Station (ISS). The clock, named PARCS (Primary Atomic Reference Clock in Space) takes advantage of the microgravity environment of the ISS to achieve a high stability of ,.(e) 5 x 10-'4*-"2 and an ultimate accuracy of 5 x 1 O-", more than an order of magnitude better than terrestrial Cs fountains. Additionally, this accurate clock on the ISS will be used to perform a variety of tests of fundamental physics, such as relativity theory. Since the ISS orbit will cover a large portion of the earth, PARCS will serve as an internationally accessible primary standard thus improving comparisons between intemational standards laboratories. Here we describe the scientific objectives of the PARCS mission, present our design considerations and laboratory studies of prototypes of clock components, and evaluate the anticipated performance of PARCS such as systematic shifts and the ultimate accuracy of the device. * Contribution of the US Government. Not subject to US copyright.
The PARCS (Primary Atomic Reference Clock in Space) experiment will use a laser-cooled Cesium atomic clock operating in the microgravity environment aboard the International Space Station (ISS) to provide both advanced tests of gravitational theory and to demonstrate a new cold-atom clock technology for space. PARCS is a joint project of the National Institute of Standards and Technology (NIST), NASA's Jet Propulsion Laboratory (JPL), and the University of Colorado (CU). This paper concentrates on the scientific goals of the PARCS mission. The microgravity space environment allows laser-cooled Cs atoms to have Ramsey times in excess of those feasible on Earth, resulting in improved clock performance. Clock stabilities of 5 × 10 −14 at one second, and accuracies better than 10 −16 are projected. The relativistic frequency shift should be measureable at least 35 times better than the previous best, Gravity Probe A.[1] PARCS is scheduled for launch in 2007 and will probably fly with the Stanford Superconducting Microwave Oscillator (SUMO), which will allow a Kennedy-Thorndike type experiment with an improvement of about three orders of magnitude compared to previous best results. PARCS will also provide a much-improved realization of the second, and a stable time reference in space. Significant improvements in testing fundamental assumptions of relativity theory, and in testing non-metric theories of gravity, are expected.
Advances in Space Research, 2005
The Primary Atomic Reference Clock in Space (PARCS) mission is designed to perform certain tests of relativity theory, to study the performance of individual GPS space-vehicle clocks, to study the dynamics of atom motion in microgravity, to advance the state-of-the art for space clocks, and to serve as a pathfinder for precision instruments based on laser cooling of atoms. After a brief overview of the project, this paper discusses the specific objectives of PARCS, describes the key subsystems, and discusses the systematic frequency shifts that limit the accuracy of the clock. Ó 2005 Published by Elsevier Ltd on behalf of COSPAR.
IEEE Transactions on Instrumentation and Measurement, 1999
We describe a space cold atom clock prototype and its operation on board an aircraft. We have recorded the atomic resonance in zero gravity during parabolic flights. This experiment must be considered as an essential step toward the construction of a space clock using cold atoms. In a microgravity environment, a cold atomic clock would outperform all groundbased clocks. By the year 2002, we plan to operate a cold atom clock on board the international space station. This mission is called Atomic Clock Ensemble in Space (ACES). We have also performed a preliminary accuracy evaluation of the prototype. The interrogation of the cold atoms is performed inside a TE 013 cavity. On earth, the phase variations of the field induce a relative frequency shift of about 1 2 10 013 . Although the frequency shift is expected to strongly decrease in microgravity, this cavity does not seem suitable for a 1 2 10 016 frequency uncertainty.
2020
Atomic clocks, which lock the frequency of an oscillator to the extremely stable quantized energy levels of atoms, are essential for navigation applications such as deep space exploration 1 and the Global Positioning System (GPS) 2 and as scientific tools for addressing questions in fundamental physics 3,4,5,6. Atomic clocks that can be launched into space are an enabling technology for GPS, but to date have not been applied to deep space navigation and have seen only limited application to scientific questions due to performance constraints imposed by the rigors of space launch and operation 7. The invention of methods to electromagnetically trap and cool ions has revolutionized atomic clock performance 8,9,10,11,12,13. Terrestrial trapped ion clocks have achieved orders of magnitude improvements in performance over their predecessors and have become a key component in national metrology laboratories 13. However, transporting this new technology into space has remained elusive. Here we show the results from the first-ever trapped ion atomic clock to operate in space. Launched in 2019, NASA's Deep Space Atomic Clock (DSAC) has operated for more than 12 months, demonstrating a short-term fractional frequency stability of between 1 and 2 x 10-13 at 1 second of averaging time (measured on the ground), a long-term stability of 3 x 10-15 at 23 days, and an estimated drift of 3.0(0.7) x 10-16 per day. Each of these exceeds current space clock performance by as much as an order of magnitude 14,15,16. We found the DSAC clock to be particularly amenable to the space environment, having low sensitivities to variations in radiation, temperature, and magnetic fields, and we were able to characterize these in detail. This level of space clock performance will enable new types of space navigation. In particular, the DSAC mission has demonstrated a process called one-way navigation whereby signal delay times are measured in-situ making near-real-time deep space probe navigation possible 17 .
Comptes Rendus Physique, 2015
The ESA mission "Space Optical Clock" project aims at operating an optical lattice clock on the ISS in approximately 2023. The scientific goals of the mission are to perform tests of fundamental physics, to enable space-assisted relativistic geodesy and to intercompare optical clocks on the ground using microwave and optical links. The performance goal of the space clock is less than 1 × 10-17 uncertainty and 1 × 10-15 τ-1/2 instability. Within an EU-FP7-funded project, a strontium optical lattice clock demonstrator has been developed. Goal performances are instability below 1 × 10-15 τ-1/2 and fractional inaccuracy 5 × 10-17. For the design of the clock, techniques and approaches suitable for later space application are used, such as modular design, diode lasers, low power consumption subunits, and compact dimensions. The Sr clock apparatus is fully operational, and the clock transition in 88 Sr was observed with linewidth as small as 9 Hz.
Journal of Physics B: Atomic, Molecular and Optical Physics, 2005
This paper describes advances in microwave frequency standards using laser-cooled atoms at BNM-SYRTE. First, recent improvements of the 133 Cs and 87 Rb atomic fountains are described. Thanks to the routine use of a cryogenic sapphire oscillator as an ultra-stable local frequency reference, a fountain frequency instability of 1.6 × 10 −14 τ −1/2 where τ is the measurement time in seconds is measured. The second advance is a powerful method to control the frequency shift due to cold collisions. These two advances lead to a frequency stability of 2 × 10 −16 at 50 000 s for the first time for primary standards. In addition, these clocks realize the SI second with an accuracy of 7 × 10 −16 , one order of magnitude below that of uncooled devices. In a second part, we describe tests of possible variations of fundamental constants using 87 Rb and 133 Cs fountains. Finally we give an update on the cold atom space clock PHARAO developed in collaboration with CNES. This clock is one of the main instruments of the ACES/ESA mission which is scheduled to fly on board the International Space Station in 2008, enabling a new generation of relativity tests.
Nature, 2021
Atomic clocks, which lock the frequency of an oscillator to the extremely stable quantized energy levels of atoms, are essential for navigation applications such as deep space exploration 1 and the Global Positioning System (GPS) 2 and as scientific tools for addressing questions in fundamental physics 3,4,5,6. Atomic clocks that can be launched into space are an enabling technology for GPS, but to date have not been applied to deep space navigation and have seen only limited application to scientific questions due to performance constraints imposed by the rigors of space launch and operation 7. The invention of methods to electromagnetically trap and cool ions has revolutionized atomic clock performance 8,9,10,11,12,13. Terrestrial trapped ion clocks have achieved orders of magnitude improvements in performance over their predecessors and have become a key component in national metrology laboratories 13. However, transporting this new technology into space has remained elusive. Here we show the results from the first-ever trapped ion atomic clock to operate in space. Launched in 2019, NASA's Deep Space Atomic Clock (DSAC) has operated for more than 12 months, demonstrating a short-term fractional frequency stability of between 1 and 2 x 10-13 at 1 second of averaging time (measured on the ground), a long-term stability of 3 x 10-15 at 23 days, and an estimated drift of 3.0(0.7) x 10-16 per day. Each of these exceeds current space clock performance by as much as an order of magnitude 14,15,16. We found the DSAC clock to be particularly amenable to the space environment, having low sensitivities to variations in radiation, temperature, and magnetic fields, and we were able to characterize these in detail. This level of space clock performance will enable new types of space navigation. In particular, the DSAC mission has demonstrated a process called one-way navigation whereby signal delay times are measured in-situ making near-real-time deep space probe navigation possible 17 .
2012 European Frequency and Time Forum, 2012
The use of ultra-precise optical clocks in space ("master clocks") will allow for a range of new applications in the fields of fundamental physics (tests of Einstein's theory of General Relativity, time and frequency metrology by means of the comparison of distant terrestrial clocks), geophysics (mapping of the gravitational potential of Earth), and astronomy (providing local oscillators for radio ranging and interferometry in space). Within the ELIPS-3 program of ESA, the "Space Optical Clocks" (SOC) project aims to install and to operate an optical lattice clock on the ISS towards the end of this decade, as a natural follow-on to the ACES mission, improving its performance by at least one order of magnitude. The payload is planned to include an optical lattice clock, as well as a frequency comb, a microwave link, and an optical link for comparisons of the ISS clock with ground clocks located in several countries and continents. Undertaking a necessary step towards optical clocks in space, the EU-FP7-SPACE-2010-1 project no. 263500 (SOC2) (2011-2015) aims at two "engineering confidence", accurate transportable lattice optical clock demonstrators having relative frequency instability below 1×10 -15 at 1 s integration time and relative inaccuracy below 5×10 -17 . This goal performance is about 2 and 1 orders better in instability and inaccuracy, respectively, than today's best transportable clocks. The devices will be based on trapped neutral ytterbium and strontium atoms. One device will be a breadboard. The two systems will be validated in laboratory environments and their performance will be established by comparison with laboratory optical clocks and primary frequency standards. In order to achieve the goals, SOC2 will develop the necessary laser systems -adapted in terms of power, linewidth, frequency stability, long-term reliability, and accuracy. Novel solutions with reduced space, power and mass requirements will be implemented. Some of the laser systems will be developed towards particularly high compactness and robustness levels. Also, the project will validate crucial laser components in relevant environments. In this paper we present the project and the results achieved during the first year.
Physical review letters, 2006
For the past 50 years, atomic standards based on the frequency of the cesium ground-state hyperfine transition have been the most accurate time pieces in the world. We now report a comparison between the cesium fountain standard NIST-F1, which has been evaluated with an ...
2007
Description/Abstract The authors have developed a chip-scale atomic clock (CSAC) for applications requiring atomic timing accuracy in portable battery-powered applications. At PTTI/FCS 2005, they reported on the demonstration of a prototype CSAC, with an overall ...
On-board atomic clocks represent the key technology for the success of any satellite navigation system mission, and their development has been continuously supported by European Space Agency (ESA). The Passive Hydrogen Maser (PHM) has been selected as master clock of the Galileo Navigation Payload and three years of continuous observation on board of GIOVE-B satellite has confirmed the outstanding performance in terms of frequency stability and negligible drift. Results coming from ground life testing have given important feedbacks on the PHM technology capability to comply with the required 12 years of lifetime . The above was the starting point for the development of other Atomic Clocks solutions like POP Rubidium clock and Mini PHM (mPHM). The main target is to preserve the excellent PHM frequency stability performance with a reduction of the overall mass, power consumption and more in general constraints for their usage on Navigation Payloads (i.e. environmental sensitivity, mai...
Pramana, 2014
Frequency corresponding to the energy difference between designated levels of an atom provides precise reference for making a universally accurate clock. Since the middle of the 20th century till now, there have been tremendous efforts in the field of atomic clocks making time the most accurately measured physical quantity. National Physical Laboratory India (NPLI) is the nation's timekeeper and is developing an atomic fountain clock which will be a primary frequency standard. The fountain is currently operational and is at the stage of complete frequency evaluation. In this paper, a brief review on atomic time along with some of the recent results from the fountain clock will be discussed.
Journal of Physics: Conference Series, 2011
Objectives ACES performances Scientific background and recent results Absolute measurement of the gravitational red-shift at an uncertainty level < 50 • 10 -6 after 300 s and < 2 • 10 -6 after 10 days of integration time.
13th International Conference on Space Operations 2014, 2014
NASA's Deep Space Atomic Clock mission is developing a small, highly stable mercury ion atomic clock with an Allan deviation of at most 1e-14 at one day, and with current estimates near 3e-15. This stability enables one-way radiometric tracking data with accuracy equivalent to and, in certain conditions, better than current two-way deep space tracking data; allowing a shift to a more efficient and flexible one-way deep space navigation architecture. DSAC-enabled one-way tracking will benefit navigation and radio science by increasing the quantity and quality of tracking data. Additionally, DSAC would be a key component to fully-autonomous onboard radio navigation useful for time-sensitive situations. Potential deep space applications of DSAC are presented, including orbit determination of a Mars orbiter and gravity science on a Europa flyby mission.
European Journal of Physics, 2008
The record of atomic clock frequency comparisons at NIST over the past half-decade provides one of the tightest constraints of any present-day temporal variations of the fundamental constants. Notably, the 6-year record of increasingly precise measurements of the absolute frequency of the Hg + single-ion optical clock (using the cesium primary frequency standard NIST-F1) constrains the temporal variation of the fine structure constant α to less than 2 • 10 -16 yr -1 and offers a Local Position Invariance test in the framework of General Relativity. The most recent measurement of the frequency ratio of the Al + and Hg + optical clocks is reported with a fractional frequency uncertainty of ±5.2 • 10 -17 . The record of such measurements over the last year sensitively tests for a temporal variation of α and constrains α/α = (-1.6 ± 2.3) • 10 -17 yr -1 , consistent with zero.
IEEE International Frequency Control Sympposium and PDA Exhibition Jointly with the 17th European Frequency and Time Forum, 2003. Proceedings of the 2003
We describe the development of a small Hg + ion clock suitable for space use. A small clock occupying 1-2 liters volume and producing stability of 10-12 /√τ would significantly advance the state of space-qualified atomic clocks. Based on recent measurements, this technology should produce long-term stability as good as 10-15 .
The European Physical Journal D, 1998
We describe the operation of a cold atom clock in reduced gravity. We have recorded the cesium hyperfine resonance signal at a frequency near 9.2 GHz in the ∼ 10 −2 g gravity environment produced by jet plane parabolic flights. With a resonance width of 7 Hz, the device operated in a regime which is not accessible on earth. In the much lower gravity level of a satellite, our cold cesium clock would outperform the fountains with a potential accuracy of 5 × 10 −17. This experiment paves the way to unprecedented performance in space applications such as tests of general relativity, global time dissemination, astronomy and geodesy.
IEEE Transactions on Instrumentation and Measurement, 1972
The European Physical Journal Special Topics, 2008
The record of atomic clock frequency comparisons at NIST over the past half-decade provides one of the tightest constraints of any present-day temporal variations of the fundamental constants. Notably, the 6-year record of increasingly precise measurements of the absolute frequency of the Hg + single-ion optical clock (using the cesium primary frequency standard NIST-F1) constrains the temporal variation of the fine structure constant α to less than 2 · 10 −16 yr −1 and offers a Local Position Invariance test in the framework of General Relativity. The most recent measurement of the frequency ratio of the Al + and Hg + optical clocks is reported with a fractional frequency uncertainty of ±5.2 · 10 −17 . The record of such measurements over the last year sensitively tests for a temporal variation of α and constrainsα/α = (−1.6 ± 2.3) · 10 −17 yr −1 , consistent with zero.
1981
NASA is planning a , Space Shuttle experiment to demonstrate high-accuracy global time and frequency transfer. A hydrogen maser clock on board the Space Shuttle will be compared with clocks on the ground using two-way microwave and short-pulse laser signals. The accuracy, goal for the experiment is 1 nsec or better for the time transfer and 10~1 4 for the frequency comparison. A direct frequency comparison of primary standards at the lO" 1^ accuracy level is a unique feature of the proposed system. Both time and frequency transfer will be accomplished by microwave transmission, while the laser signals provide calibration of the system as well as sub-nanosecond time transfer. Following the demonstration with the Space Shuttle, an operational system could be implemented in a free-flying satellite to provide permanent global time and frequency transfer.
Loading Preview
Sorry, preview is currently unavailable. You can download the paper by clicking the button above.