ArticlePDF Available
Vision of a Clock-Based Network for Absolute
Sea Level Monitoring
Asha Vincent and Jürgen Müller
Abstract
Global sea level shows an increasing trend for several decades driven mainly by climate
change. Absolute Sea Level (ASL) changes can only be extracted from Relative Sea Level
(RSL) measurements with proper reduction of vertical land movements of the bench marks.
Atomic clocks at those tide gauges can potentially provide the absolute, near real-time
physical height change. High-performance clocks with an uncertainty of 1018 enable a
height measurement with 1 cm accuracy. As RSL is related to regional tidal datums, one
has to account for the local variations to obtain a globally consistent measurement of
ASL. Hence, by incorporating land motion from clock observations, one can establish
a consistent and uniform reference datum for assessing geoid-based absolute sea level
changes worldwide.
Keywords
Absolute sea level Atomic clocks Physical height Relative sea level Relativistic
geodesy
1Introduction
The geoid, which represents the global mean sea level in rest,
serves as a reference surface in geodesy. Precise measure-
ments of the local relative sea level are typically carried out
by comparing the level of the sea surface at a specific location
to a fixed reference point on land (Wöppelmann and Marcos
2016). This reference point, often referred to as a benchmark
or tidal datum, serves as a baseline for determining how
the sea level at that location changes over time. At present
GNSS (Global Navigation Satellite System) stations nearby
tide gauge locations serve as benchmarks for estimating the
relative land movements (Larson et al. 2013) in order to
determine the Absolute Sea Level (ASL) (Peng et al. 2021).
A. Vincent () · J. Müller
Institute for Geodesy, Leibniz University Hannover, Hannover, Lower
Saxony, Germany
e-mail: vincent@ife.uni-hannover.de;mueller@ife.uni-hannover.de
The physical height at a point on the Earth surface
depends upon the geoid at the time of the measurement (Ihde
et al. 2017). As detailed in Dietrich (2014) ASL refers to
the height of the sea surface above a fixed global reference
without the effect of land motion. Unlike Relative Sea Level
(RSL), which is determined by tide gauges with respect to a
local or regional reference (tide gauge zero or a tidal datum),
absolute sea level is referenced to a mean ellipsoid when
using GNSS benchmarks as reference. Installation of high-
performance atomic clocks at the tide gauge locations can
provide the absolute physical height change which enables
to directly obtain ASL changes with respect to the geoid.
Philipp et al. (2020) give details on the relativistic definition
of geoid and gravity potential.
2 Clocks to Replace GNSS Benchmarks
The physical height at a point on Earth’s surface is contin-
uously varying mainly due to external tidal effects and non-
tidal mass distributions in the Earth system as explained in
International Association of Geodesy Symposia,
https://doi.org/10.1007/1345_2024_265, © The Author(s) 2024
A. Vincent and J. Müller
Fig. 1 Absolute sea level change (ASL) and relative sea level (RSL)
with respect to a tidal datum (TD) in the case of land uplift H vand
sea level (SL) rise
Voigtetal.(2016). Tidal effects include solid-earth tides
and ocean-load tides due to external bodies such as the
Sun, Moon and other planets, centrifugal effects of polar
motion result in pole tides and LOD (Length Of Day) tides
arise from the variations in the Earth’s angular velocity,
atmospheric tides, etc. Non-tidal effects include mass re-
distributions in the geosphere, hydrosphere, atmosphere and
biosphere. All these effects affect the geopotential at the
point of interest as a result of mass change and the associated
vertical displacements (Schröder et al. 2021). From terres-
trial clock observations, the physical height changes can
be inferred where GNSS receivers provide only ellipsoidal
height changes. Thus, we can compute ASL changes with
respect to the geoid by adding relative sea level changes with
time-variable land motion (H v) from clock observations:
ASL DRSL CH v:(1)
As RSL measurements are referenced to GNSS benchmarks
near tide gauges, it doesn’t necessarily guarantee consistency
in the vertical datum across different locations. Vertical
datums can vary regionally due to factors such as local
geoid variations, tectonic movements, and other geophysical
processes. Here, clocks offer an alternative by providing a
direct reference to an equipotential surface such as the geoid.
Using atomic clocks as benchmarks will be a more consistent
way of deriving the ASL change globally by referencing both
land and sea level measurements to a known equipotential
surface, e.g., geoid. Then, we do not need to consider the
regional tidal datum variations, as measurements will be
taken with respect to the global geoid that preserves the
uniformity of a reference surface without any local variations
(Fig. 1).
If connected to a stable reference clock that is related to
the geoid (W0), terrestrial clocks provide physical heights H,
which can also be represented in terms of the geopotential
Fig. 2 Loading and unloading effects on physical height which
depends upon geoid (G) height and vertical displacement of Earth
surface (T)
number, CpDW0Wp, where W0represents the potential
on the geoid and Wpis the gravity potential at point p (Torge
et al. 2023). Here, gravity potential changes can directly only
be observed by clocks. And keep in mind, a potential change
is independent of whether the mass change occurs above or
below the Earth’s surface, i.e. above or below the clock loca-
tion. The gravitational potential change or the corresponding
physical height difference between two clocks can be derived
from the fractional frequency difference (Bjerhammar 1986;
Müller et al. 2018; Wu and Müller 2019; Denker et al. 2018),
f
fW
c2gH
c2(2)
when using the GCRS (Geocentric Celestial Reference Sys-
tem) metric up to the first Newtonian order (orders of c4
are omitted) where W is the gravity potential difference
between the two clock sites, c is the speed of light and, g is
the mean gravity value. As illustrated in Fig.2, tidal effects
and non-tidal loading/unloading effects affect the physical
heights represented as H v
tidal and H v
nontidal respec-
tively. According to Eq. (2), these time-variable changes are
obtained by clocks (the static part cancels out for clocks at a
fixed location),
H vDH v
tidal CH v
nontidal:(3)
In order to get the time-dependent variations in physical
heights, there should be a stable reference clock somewhere
on ground or space that is related to the geoid (Wu and Müller
2020; Philipp et al. 2023). As shown by Lisdat et al. (2016),
the systematic uncertainty of the optical fibre link is of 1019.
For our purpose, we propose only a single link for each tide
gauge clock to the reference clock which is assumed to be in
a geostationary satellite. We assume a space link accuracy
in the 1018 level. The major influence on the space link
uncertainty is the clock error and velocity error as given in
Shen et al. (2023). A link accuracy of 1018 is sufficient to
achieve a 1 cm accuracy in the ASL estimation.
Vision of a Clock-Based Network for Absolute Sea Level Monitoring
Fig. 3 Tide gauge locations considered in this study: NEWL (Newlyn),
AND1 (Andenes), REYK (Reykjavik), IBIZ (Ibiza), GENO (Genova),
and, 0NYB (Kalix)
3 Methodology
Tide gauge locations along the European coast are consid-
ered for this study (Fig. 3). A total of 6 sites Newlyn (UK),
Andenes (Norway), Reykjavik (Iceland), Ibiza (Spain), Gen-
ova (Italy), and Kalix (Sweden) are chosen based on the
availability of nearby GNSS stations with longer time-series.
The simulations are carried out for the time period 2006-
2016 based on the availability of the needed datasets. The
mean over the time period is reduced from monthly RSL
RLR (Revised Local Reference) data obtained from PSMSL
(Permanent Service for Mean Sea Level) (Holgate et al.
2013; Permanent service for mean sea level 2023) to derive
the RSL change. Clock observations are simulated by com-
bining the physical height change due to tidal and non-tidal
effects (Eq. 3). Addition of RSL changes with the simulated
effective vertical displacements or the clock observations
generate the corresponding ASL changes at the selected tide
gauge locations (Eq. 1).
4 Results and Discussion
4.1 Simulation of Tidal Signals as Clock
Observations
Potential variations due to solid-earth tides, pole tides and
LOD tides are computed on the deformable Earth surface
using modified ETERNA34 (PREDICT program) Earth tide
data processing package (Wenzel 2022) for the chosen time
period. The HW95 (Hartmann and Wenzel 1995) tidal poten-
tial catalogue is used for deriving the hourly tidal poten-
tial values which are subsequently averaged to produce
monthly values. Similarly, monthly averages of potential
variations due to ocean tidal loading are determined with the
SPOTL3.3.0.2 package (Agnew 2012) using the Empirical
Ocean Tidal model (EOT11a) (Savcenko and Bosch 2012).
Both ETERNA34 and SPOTL calculate the effective poten-
tial variations due to mass changes and land motion. Figure 4
shows the simulated major tidal values at a high-latitude
site and a low-latitude site. The LOD tidal values are of
the order of 0:001 m2/s2which can be neglected. Similarly,
atmospheric tidal values are also much less than the range
of 1018 (= 0.1 m2/s2) clock sensitivity which again can be
neglected (Voigt et al. 2016).
The monthly averages of solid-earth tides range from
approximately 10 cm at high-latitude sites, making it an
important factor in total land motion. All the three major tidal
contributions (Fig. 4) are combined to generate the total tidal
effects (second subplots of Fig. 5). The observed negative
long-term trend in the tidal values is caused by the 18.61 year
lunar nodal cycle. According to Rochlin and Morris (2017),
the declination of Moon’s orbit is smallest from 2005 to 2015
which results in increasing tidal amplitudes that correspond
to negative potential variations on the Earth surface.
4.2 Simulation of Non-Tidal Signals as
Clock Observations
Non-tidal mass distributions include loading and unloading
effects arising from various effects such as changes in Ter-
restrial Water Storage (TWS), atmospheric pressure, ocean
bottom pressure, solid earth processes like GIA (Glacial
Isostatic Adjustment), etc. (Schröder et al. 2021). The time
series of geoid height variation due to the variation in the
TWS can be determined from GRACE (Gravity Recovery
And Climate Experiment) fully normalised monthly spheri-
cal harmonic coefficients (Kvas et al. 2019). Similarly, using
the fully normalised monthly spherical harmonic coefficients
(GAC) from Atmosphere and Ocean De-aliasing product
(AOD1B RL06) (Dobslaw et al. 2017), the effect of atmo-
sphere and ocean mass variability can be well estimated.
The surface deformations associated with these non-tidal
mass distributions are given by NGL (Nevada Geodetic Lab-
oratory) GNSS time-series solutions (Blewitt et al. 2018). A
loading effect leads to a downward vertical displacement and
vice versa. The effective gravitational potential variations
can be computed by combining the potential variations due
to mass changes and surface displacements (Vincent and
Müller 2023). The separate effects of geoid height variations
(GRACE+AOD) and the corresponding vertical displace-
ments of the Earth surface (GNSS) are shown by the first
subplots of Fig. 5.
A. Vincent and J. Müller
Fig. 4 Monthly averages of solid-earth tides (SET), ocean-load tides (OTL) and pole tides (POL) with their linear trends at Andenes (a)and
Genova (b)
The simulated clock observations by combining the tidal
and non-tidal potential variations (Eq. 3) at the chosen tide
gauge locations are given by the third subplots of Fig.5.
1018 clocks can provide absolute land motion of 1 cm
(i.e. corresponding gravity potential variations of 0.1 m2/s2)
between the clock sites in near real-time. When one considers
monthly observations over several years as done in this
study the resulting trend accuracy is less than 1 mm/yr
(Fig. 5).
4.3 Estimation of ASL Changes
As mentioned in Sect. 2, geoid-based ASL changes can be
derived by combining clock observations with RSL data
from tide gauges (Eq. 1). Clock observations of height
variations provide a globally consistent and uniform refer-
ence for deriving ASL changes. High-performance clocks
with fractional frequency uncertainty of 1018 (McGrew
et al. 2018; Takamoto et al. 2022) with same level of link
accuracy can be utilised well in deriving ASL changes with
high accuracy of 1 cm. The monthly variations of RSL are
determined by reducing the mean over the chosen time-
span. The clock observations which are simulated in terms
of potential variations (m2/s2) are transferred into physical
height variations (cm) by multiplying with g to combine
with the RSL changes. Figure 6shows the graphs of the
estimated ASL changes with the long-term trend, clock
observations in terms of physical height, and RSL changes.
The measurement noise of RSL affects the estimation of
ASL.
Present-day land uplift, e.g., at Kalix (0NYB) can fake a
sea level fall. So, the land motion must be taken into account
when deriving actual sea level changes. As seen in Figs.5
and 6, the offsets from the monthly means of land motion
affect the monthly averages of ASL change at the clock sites.
On analyzing the linear trends at the tide gauge sites for the
estimated time period, there is an overall increase in ASL
with given accuracy.
5 Conclusions
Till now, land-based absolute sea level measurements are
estimated with respect to GNSS benchmarks or local tidal
datums that give ASL changes with respect to the reference
ellipsoid. Further calculations are needed in order to derive
a globally consistent measure of ASL. High-performance
atomic clocks at tide gauge locations with better link uncer-
tainty can provide more accurate physical height changes
and thus, geoid-based ASL changes can be directly obtained.
Hence, clock networks can be used for monitoring vertical
land movements and providing uniform and consistent ASL
changes world-wide.
We have estimated the ASL changes at some tide gauge
locations along the European coast. The obtained long-
term trend values indicate the geoid-based ASL changes
per year for the given time-span. A maximum value of
0.71˙0.49 cm/year was observed at Andenes (AND1) for
the time period 2008–2016. All sites other than Ibiza (IBIZ)
and Newlyn (NEWL)show an increasing trend. Significant
land uplift at sites Kalix (0NYB), Andenes (AND1), and
Reykjavik (REYK) should be effectively reduced for the
accurate estimation of ASL changes. Also, for all the sites,
tidal effects play an important role as even the monthly-
averages can be as high as 10–20 cm. Thus, the accurate
Vision of a Clock-Based Network for Absolute Sea Level Monitoring
Fig. 5 Simulated clock observations (CLOCK) by combining the potential variations due to non-tidal effects (mass changes in TWS (GRACE),
atmosphere and ocean (AOD) and associated vertical deformations (GNSS)) and tidal effects (TIDAL=SET+OTL+POL) with their linear trends
(m2/s2yr) at the tide gauge sites
A. Vincent and J. Müller
Fig. 6 Estimated monthly ASL changes (ASL) by reducing the clock observations (CLOCK) from RSL changes (RSL) at the tide gauge sites.
The long-term trends of ASL changes (cm/yr) are also given
Vision of a Clock-Based Network for Absolute Sea Level Monitoring
estimation of globally consistent geoid-based ASL changes
favours the realization of clock-based networks in the near
future.
Acknowledgements This study has been funded by the Deutsche
Forschungsgemeinschaft (DFG, German Research Foundation) under
Germany’s Excellence Strategy EXC 2123 Quantum Frontiers
Project-ID 90837967 and the SFB 1464 TerraQ Project-ID 434617780
within project C02.
References
Agnew DC (2012) Spotl: Some programs for ocean-tide loading. https://
api.semanticscholar.org/CorpusID:127800542
Bjerhammar A (1986) Relativistic geodesy. U.S. Dept. of Commerce,
National Oceanic and Atmospheric Administration, National Ocean
Service, Charting and Geodetic Services, For sale by the National
Geodetic Information Center, NOAA, Rockville, MD
Blewitt G, Hammond WC, Kreemer C (2018) Harnessing the gps data
explosion for interdisciplinary science. Eos 99:485. https://doi.org/
10.1029/2018EO104623
Denker H, Timmen L, Voigt C, Weyers S, Peik E, Margolis HS,
Delva P, Wolf P, Petit G (2018). Geodetic methods to determine the
relativistic redshift at the level of 1018 in the context of international
timescales: a review and practical results. J Geodesy 92(5):487–516.
https://doi.org/10.1007/s00190-017-1075-1
Dietrich R (2014) Sea Level, pp 1 ˝
U-9. Springer Netherlands, Dor-
drecht. ISBN 978-94-007-6644-0. https://doi.org/10.1007/978-94-
007-6644-0_173-1
Dobslaw H, Bergmann-Wolf I, Dill R, Poropat L, Thomas M, Dahle
C, Esselborn S, König R, Flechtner F (2017) A new high-resolution
model of non-tidal atmosphere and ocean mass variability for de-
aliasing of satellite gravity observations: AOD1B RL06. Geophys
J Int 211(1):263–269. ISSN 0956-540X. https://doi.org/10.1093/gji/
ggx302
Holgate SJ, Matthews A, Woodworth PL, Rickards L, Tamisiea ME,
Bradshaw E, Foden PR, Gordon K, Jevrejeva S, Pugh J (2013). New
data systems and products at the permanent service for mean sea
level. https://api.semanticscholar.org/CorpusID:129718672
Ihde J, Sánchez L, Barzaghi R, Drewes H, Foerste C, Gruber T, Liebsch
G, Marti U, Pail R, Sideris MG (2017) Definition and proposed
realization of the international height reference system (ihrs). Surv
Geophys 38:549–570. https://doi.org/10.1007/s10712-017-9409-3
Kvas A, Behzadpour S, Ellmer M, Klinger B, Strasser S, Zehentner N,
Mayer-Gürr T (2019) Itsg-grace2018: Overview and evaluation of a
new grace-only gravity field time series. J Geophys Res Solid Earth
124(8):9332–9344. https://doi.org/10.1029/2019JB017415
Larson KM, Ray RD, Nievinski FG, Freymueller JT (2013) The
accidental tide gauge: A gps reflection case study from kachemak
bay, alaska. IEEE Geosci Remote Sens Lett 10:1200–1204. https://
api.semanticscholar.org/CorpusID:11995621
Lisdat C, Grosche G, Quintin N, Shi C, Raupach S, Grebing C, Nicolodi
D, Stefani F, Al-Masoudi A, Dörscher S, et al. (2016) A clock
network for geodesy and fundamental science. Nature Commun
7(1):1–7. https://doi.org/10.1038/ncomms12443
McGrew W, Zhang X, Fasano R, Schäffer S, Beloy K, Nicolodi
D, Brown R, Hinkley N, Milani G, Schioppo M, et al. (2018)
Atomic clock performance enabling geodesy below the centimetre
level. Nature 564(7734):87–90. https://doi.org/10.1038/s41586-018-
0738-2
Müller J, Dirkx D, Kopeikin SM, Lion G, Panet I, Petit G, Visser P
(2018) High performance clocks and gravity field determination.
Space Sci Rev 214(1):1–31. https://doi.org/10.1007/s11214-017-
0431-z
Peng D, Feng L, Larson KM, Hill EM (2021) Measuring coastal
absolute sea-level changes using gnss interferometric reflectome-
try. Remote Sens 13(21). ISSN 2072–4292. https://doi.org/10.3390/
rs13214319
Permanent service for mean sea level (psmsl) (2023). tide gauge data,
May 2023. http://www.psmsl.org/data/obtaining/
Philipp D, Hackmann E, Lämmerzahl C, Müller J (2020) Relativis-
tic geoid: Gravity potential and relativistic effects. Phys Rev D
101:064032. https://doi.org/10.1103/PhysRevD.101.064032
Philipp D, Hackmann E, Hackstein JP, Lämmerzahl C (2023) General
relativistic chronometry with clocks on ground and in space. https://
doi.org/10.48550/arXiv.2310.11576
Rochlin I, Morris JT (2017) Regulation of salt marsh mosquito popu-
lations by the 18.6-yr lunar-nodal cycle. Ecology 98(8):2059–2068.
https://doi.org/10.1002/ecy.1861
Savcenko R, Bosch W (2012) DGFI-Report No.89: Eot11a empirical
ocean tide model from multi-mission satellite altimetry. Technical
report, DGFI-TUM
Schröder S, Stellmer S, Kusche J (2021) Potential and scientific require-
ments of optical clock networks for validating satellite-derived time-
variable gravity data. Geophys J Int 226(2):764–779. https://doi.org/
10.1093/gji/ggab132
Shen Z, Shen W, Xu X, Zhang S, Zhang T, He L, Cai Z, Xiong S,
Wang L (2023) A method for measuring gravitational potential of
satellite’s orbit using frequency signal transfer technique between
satellites. Remote Sens 15(14).. ISSN 2072-4292. https://doi.org/10.
3390/rs15143514.https://www.mdpi.com/2072-4292/15/14/3514
Takamoto M, Tanaka Y, Katori H (2022) A perspective on the future of
transportable optical lattice clocks. Appl Phys Lett 120(14):140502.
https://doi.org/10.1063/5.0087894
Torge W, Müller J, Pail R (2023) Geodesy. De Gruyter Olden-
bourg, Berlin, Boston. ISBN 9783110723304. https://doi.org/10.
1515/9783110723304
Vincent A, Müller J (2023) Detection of time variable gravity signals
using terrestrial clock networks. Adv Space Res. ISSN 0273-1177.
https://doi.org/10.1016/j.asr.2023.07.058
Voigt C, Denker H, Timmen L (2016) Timevariable gravity potential
components for optical clock comparisons and the definition of
international time scales. Metrologia 53(6):1365. https://doi.org/10.
1088/0026-1394/53/6/1365
Wenzel H-G (2022) Eterna programs for tidal analysis and prediction.
Karlsruhe Institute of Technology. https://doi.org/10.35097/746
Wu H, Müller J (202) Towards an international height reference frame
using clock networks. In: Freymueller JT, Sánchez L (eds) Beyond
100: The Next Century in Geodesy, pp 3–10. Springer Interna-
tional Publishing, Cham. ISBN 978-3-031-09857-4. https://doi.org/
10.1007/1345_2020_97
Wu H, Müller J, Lämmerzahl C (2019) Clock networks for height
system unification: a simulation study. Geophys J Int 216(3):1594–
1607. https://doi.org/10.1093/gji/ggy508
Wöppelmann G, Marcos M (2016) Vertical land motion as a key
to understanding sea level change and variability. Rev Geophys
54(1):64–92. https://doi.org/10.1002/2015RG000502
A. Vincent and J. Müller
Open Access This chapter is licensed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.
org/licenses/by/4.0/), which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate
credit to the original author(s) and the source, provide a link to the Creative Commons license and indicate if changes were made.
The images or other third party material in this chapter are included in the chapter’s Creative Commons license, unless indicated otherwise in a
credit line to the material. If material is not included in the chapter’s Creative Commons license and your intended use is not permitted by statutory
regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder.
ResearchGate has not been able to resolve any citations for this publication.
Article
Full-text available
We introduce an approach for the direct measurement of the gravitational potential (GP) along the trajectory of a satellite, with a specific focus on Low-Earth Orbit (LEO) satellites. A LEO satellite communicates with several Geosynchronous Equatorial Orbit (GEO) satellites via frequency signal links. The GP difference can be measured in real-time using the gravitational frequency shift approach by equipping both LEO and GEO satellites with precise atomic clocks. Since the GP at the high orbits of the GEO satellites can be precisely determined by the present gravitational field model EGM2008, the GP along the LEO satellite’s trajectory can be determined. In this study, simulation experiments were conducted, featuring a GRACE-type satellite as the LEO satellite in communication with three equidistant GEO satellites. The results indicated that the accuracy of the GP measurements along the LEO satellite’s trajectory primarily depends on the precision of the onboard atomic clocks. Supposing optical atomic clocks attain an instability level of 1×10−17τ−1/2 (τ in seconds), we determined the GP distribution covered by the LEO satellite’s trajectories with 30-day observations. Then, we determined a gravitational field at the centimeter level based on the GP distribution. The GP data derived from the trajectory of a LEO satellite can be utilized to establish temporal gravitational fields, which have broad applications in different disciplines.
Article
Full-text available
Rising sea levels pose one of the greatest threats to coastal zones. However, sea-level changes near the coast, particularly absolute sea-level changes, have been less well monitored than those in the open ocean. In this study, we aim to investigate the potential of Global Navigation Satellite Systems Interferometric Reflectometry (GNSS-IR) to measure coastal absolute sea-level changes and tie on-land (coastal GNSS) and offshore (satellite altimetry) observations into the same framework. We choose three coastal GNSS stations, one each in regions of subsidence, uplift and stable vertical land motions, to derive both relative sea levels and sea surface heights (SSH) above the satellite altimetry reference ellipsoid from 2008 to 2020. Our results show that the accuracy of daily mean sea levels from GNSS-IR is <1.5 cm compared with co-located tide-gauge records, and amplitudes of annual cycle and linear trends estimated from GNSS-IR measurements and tide-gauge data agree within uncertainty. We also find that the de-seasoned and de-trended SSH time series from GNSS-IR and collocated satellite altimetry are highly correlated and the estimated annual amplitudes and linear trends statistically agree well, indicating that GNSS-IR has the potential to monitor coastal absolute sea-level changes and provide valuable information for coastal sea-level and climate studies.
Chapter
Full-text available
Establishing an International Height Reference Frame (IHRF) has been a major goal of the International Association of Geodesy (IAG) for a long time. One challenge is to obtain the vertical coordinates, i.e., geopotential numbers, of the reference stations with high precision and global consistency. A promising approach is using clock networks, which are powerful in precisely obtaining geopotential or height differences between distant sites through measuring the gravitational redshift effect by comparing clocks’ frequencies. We propose a hybrid clock network following a specific hierarchy. It includes stationary clocks as the backbone of the frame and transportable clocks for regional densifications. The vertical coordinates of the clock stations can be straightforwardly referenced to the unique benchmark by various long-distance frequency transfer techniques, like using optical fibers or free-space microwave and laser links via relay satellites. Another practical way towards an IHRF is to unify all local height systems around the world. Clock networks are considered as an alternative to classical geodetic methods. The idea was verified through closed-loop simulations. We found that the measurements acquired by a few 10⁻¹⁸ clocks, three or four in triangular or quadrangular distributions for each local system, are sufficient to adjust the discrepancies between local datums and the systematic slopes within local height networks.
Article
Full-text available
The Earth’s geoid is one of the most essential and fundamental concepts to provide a gravity field-related height reference in geodesy and associated sciences. To keep up with the ever-increasing experimental capabilities and to consistently interpret high-precision measurements without any doubt, a relativistic treatment of geodetic notions (including the geoid) within Einstein’s theory of general relativity is inevitable. Building on the theoretical construction of isochronometric surfaces and the so-called redshift potential for clock comparison, we define a relativistic gravity potential as a generalization of (post-)Newtonian notions. This potential exists in any stationary configuration with rigidly corotating observers, and it is the same as realized by local plumb lines. In a second step, we employ the gravity potential to define the relativistic geoid in direct analogy to the Newtonian understanding. In the respective limit, the framework allows to recover well-known (post-) Newtonian results. For a better illustration and proper interpretation of the general relativistic gravity potential and geoid, some particular examples are considered. Explicit results are derived for exact vacuum solutions to Einstein’s field equation as well as a parametrized post-Newtonian model. Comparing the Earth’s Newtonian geoid to its relativistic generalization is a very subtle problem, but of high interest. An isometric embedding into Euclidean three-dimensional space is an appropriate solution and allows a genuinely intrinsic comparison. With this method, the leading-order differences are determined, which are at the mm level.
Article
Full-text available
ITSG‐Grace2018 is a new series of GRACE‐only gravity field solutions based on reprocessed GRACE observation data (L1B RL03) and the latest atmosphere and ocean dealiasing product (AOD1B RL06). It includes unconstrained monthly and constrained daily solutions, as well as a high‐resolution static gravity field. Compared to the previous ITSG release, we implemented a number of improvements within the processing chain and use updated background models. In an effort to better model all known error sources, we propagate synthetic orientation uncertainties of the star camera assembly to the antenna offset correction for intersatellite ranging observations. This enables the disentanglement of the stationary noise of the K‐Band system and the nonstationary noise of the antenna offset correction. We further incorporated uncertainties of the atmosphere and ocean dealiasing product to reduce temporal aliasing effects. To mitigate errors in the applied ocean tide model, we used constrained GRACE estimates of selected tidal constituents as an additional background model. Variability over quiet ocean areas suggests a 27% to 46% lower noise level compared to the current spherical harmonic solutions of the official processing centers (300 km Gaussian filter applied). To ensure that the low noise floor is not accompanied by signal loss, we examined drainage basin averages, which showed consistent amplitudes with the official GRACE time series. These evaluations lead to the conclusion that ITSG‐Grace2018 is a state‐of‐the‐art GRACE time series which exhibits an excellent signal‐to‐noise ratio.
Article
Full-text available
The passage of time is tracked by counting oscillations of a frequency reference, such as Earth’s revolutions or swings of a pendulum. By referencing atomic transitions, frequency (and thus time) can be measured more precisely than any other physical quantity, with the current generation of optical atomic clocks reporting fractional performance below the 10⁻¹⁷ level1–5. However, the theory of relativity prescribes that the passage of time is not absolute, but is affected by an observer’s reference frame. Consequently, clock measurements exhibit sensitivity to relative velocity, acceleration and gravity potential. Here we demonstrate local optical clock measurements that surpass the current ability to account for the gravitational distortion of space-time across the surface of Earth. In two independent ytterbium optical lattice clocks, we demonstrate unprecedented values of three fundamental benchmarks of clock performance. In units of the clock frequency, we report systematic uncertainty of 1.4 × 10⁻¹⁸, measurement instability of 3.2 × 10⁻¹⁹ and reproducibility characterized by ten blinded frequency comparisons, yielding a frequency difference of [−7 ± (5)stat ± (8)sys] × 10⁻¹⁹, where ‘stat’ and ‘sys’ indicate statistical and systematic uncertainty, respectively. Although sensitivity to differences in gravity potential could degrade the performance of the clocks as terrestrial standards of time, this same sensitivity can be used as a very sensitive probe of geopotential5–9. Near the surface of Earth, clock comparisons at the 1 × 10⁻¹⁸ level provide a resolution of one centimetre along the direction of gravity, so the performance of these clocks should enable geodesy beyond the state-of-the-art level. These optical clocks could further be used to explore geophysical phenomena¹⁰, detect gravitational waves¹¹, test general relativity¹² and search for dark matter13–17.
Article
The unprecedented stability and accuracy of optical atomic clocks extend their role not only in frequency metrology but also in fundamental physics and geodesy. In particular, excellent stability of optical lattice clocks accessing a fractional uncertainty of [Formula: see text] in less than an hour opens a new avenue for chronometric leveling, which resolves a height difference of one cm in a short averaging time. However, for field use of such clocks, there remains a challenge in developing a transportable system that can operate outside the laboratory. In this Perspective, we describe transportable optical lattice clocks and discuss their future applications to chronometric leveling.
Article
The GRACE and GRACE-FO missions have provided an unprecedented quantification of large-scale changes in the water cycle. However, it is still an open problem of how these missions’ data can be referenced to a ground truth. Meanwhile, stationary optical clocks show fractional instabilities below 10−18 when averaged over an hour, and continue to be improved in terms of stability and accuracy, uptime, and transportability. The frequency of a clock is affected by the gravitational redshift, and thus depends on the local geopotential; a relative frequency change of 10−18 corresponds to a geoid height change of about 1 cm. Here we suggest that this effect could be exploited for sensing large-scale temporal geopotential changes via a network of clocks distributed at the Earth’s surface. In fact, several projects have already proposed to create an ensemble of optical clocks connected across Europe via optical fibre links. Our hypothesis is that a clock network with collocated GNSS receivers spread over Europe – for which the physical infrastructure is already partly in place – would enable us to determine temporal variations of the Earth’s gravity field at time scales of days and beyond, and thus provide a new means for validating satellite missions such as GRACE-FO or a future gravity mission. Here, we show through simulations how glacial, hydrological and atmospheric variations over Europe could be observed with clock comparisons in a future network that follows current design concepts in the metrology community. We assume different scenarios for clock and GNSS uncertainties and find that even under conservative assumptions – a clock error of 10−18 and vertical height control error of 1.4 mm for daily measurements – hydrological signals at the annual time scale and atmospheric signals down to the weekly time scale could be observed.
Article
The unification of local height systems has been a classical geodetic problem for a long time, the main challenges of which are the estimation of offsets between different height systems and the correction of tilts along the levelling lines. It has been proposed to address these challenges with clock networks. The latest generation of optical clocks as well as the dedicated frequency links, for example optical fibres, are now approaching to deliver the comparison of frequencies at the level of 1.0 × 10 -18. It corresponds to an accuracy of about 1.0 cm in height difference. Clock networks can thus serve as a powerful tool to connect local height systems. To verify the idea, we carried out simulations using the EUVN/2000 (European Unified Vertical Network) as apriori input. Four local height systems were simulated from the EUVN/2000 by introducing individual offsets and tilts, and were reunified by using measurements in clock networks. The results demonstrate the great potential of clock networks for height system unification. In case that the offsets between different height systems and tilts along national levelling lines in both longitudinal and latitudinal directions are considered, three or four clocks measurements for each local region are sufficient for the unification. These clocks are to be interconnected and should be properly arranged so that they can sense the levelling tilts where necessary. Our results also indicate that even clocks with one magnitude poorer accuracy than the desired ones can still unify the height systems to some extent, but it may cause a shift for the reunified system. © The Author(s) 2018. Published by Oxford University Press on behalf of The Royal Astronomical Society.