G6.1 | Open Session in Geodesy with a Focus on Satellite Altimetry
EDI
Open Session in Geodesy with a Focus on Satellite Altimetry
Convener: Annette Eicker | Co-conveners: Bernd UebbingECSECS, Louise Sandberg Sørensen, Karina Nielsen, Roelof Rietbroek, Rebekka Steffen, Andreas KvasECSECS
Orals
| Fri, 28 Apr, 14:00–15:40 (CEST)
 
Room 0.11/12
Posters on site
| Attendance Thu, 27 Apr, 16:15–18:00 (CEST)
 
Hall X2
Posters virtual
| Attendance Thu, 27 Apr, 16:15–18:00 (CEST)
 
vHall GMPV/G/GD/SM
Orals |
Fri, 14:00
Thu, 16:15
Thu, 16:15
In this session we welcome contributions of general interest within the geodesy community. The session is open to all branches of geodesy and related fields of research.

A specific part of the session will focus on the topic of satellite altimetry, which provides the possibility to observe key parts of the hydrosphere, namely the ocean, ice, and continental surface water from space. Since the launch of Topex/Poseidon in 1992, the applications of altimetry have expanded from the open oceans to coastal zones, inland water, land, and sea ice. Today, several missions are in orbit, providing dense and near-global observations of surface elevation and several other parameters. Satellite altimetry has become an integral part of the global observation of the Earth‘s system and changes therein.

In recent years, new satellite altimetry missions have been launched carrying new instruments; the CryoSat-2, Sentinel-3, and Sentinel-6 missions equipped with a Delay/Doppler altimeter, the Saral AltiKa mission carrying the first Ka-band altimeter, and the photon-counting laser altimeter onboard NASA's ICESat-2. Further, new orbits with high inclination and long-repeat time are used for CryoSat-2 and ICESat-2.

Fully exploiting this unprecedented availability of observables will enable new applications and results but also require novel and adapted data analysis methods.
Across the different applications for satellite altimetry, the data analysis and underlying methods are similar and knowledge exchange between the disciplines has been proven to be fruitful.
In this multidisciplinary altimetry session, we, therefore, invite contributions that discuss new methodologies and applications for satellite altimetry in the fields of geodesy, hydrology, cryosphere, oceanography, and climatology.
Topics of such studies could for example be (but are not limited to); the creation of robust and consistent time series across sensors, validation experiments, a combination of radar and laser altimetry for e.g. remote sensing of snow, classification of waveforms, application of data in a geodetic orbit, retracking, or a combination with other remote sensing data sets.

Orals: Fri, 28 Apr | Room 0.11/12

Chairpersons: Rebekka Steffen, Bernd Uebbing, Karina Nielsen
Accross Geodesy
14:00–14:10
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EGU23-8977
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ECS
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On-site presentation
Raphaël Mukandila Ngalula, Mustapha Meghraoui, Frédéric Masson, and François Tondozi Keto

The southern Africa block (SAB) is one of the 4 blocks of the Africa plate (Mukandila, 2020). Using the east African seismicity as defined by Bird (2002), the Zululand boundary between the Nubia and Somalia plates separates this block into eastern (SABE) and western (SABW) sub-blocks. In addition, the level of seismicity in this region is remarkable (e.g., the 2006 Mozamique Mw 7 and 2017 Botswana Mw 6.5 earthquakes). However, there is no dense geodetic studies that establish correlation between the seismic activity and active deformation in this intraplate tectonic domain. In this study, we use position timeseries (longer than 20 years) from about 65 GNSS stations in southern Africa. The rigorous inversion of the GNSS velocities using the least square method and Newton-Raphson methods. The combined two methods make it possible to minimize the uncertainties in the location coordinates and angular velocities of the Euler poles (0.5e**-5° and 0.5e**-5 °/Ma, respectively). This approach made it possible to determine three Euler poles with the aforementioned precision, namely the pole of the SAB and those of its respective sub-blocks. The relative velocities between the southern and northern sub-blocks of (~0.157) mm/yr. at south and (0.185) mm/yr., respectively, with respect to the Zululand bourdary line describe a predominantly extensional deformation regime that correlates with seismic activity in the region.

How to cite: Mukandila Ngalula, R., Meghraoui, M., Masson, F., and Tondozi Keto, F.: The controversial rigidity of southern Africa block: Insights from geodetic results and seismicity, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-8977, https://doi.org/10.5194/egusphere-egu23-8977, 2023.

14:10–14:20
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EGU23-6419
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ECS
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On-site presentation
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Matthias Schartner and Benedikt Soja

The proliferation of spaceborne radio frequency interference (SRFI) is threatening the operation of Very Long Baseline Interferometry (VLBI). Most SRFI is caused by the excessive number of newly launched satellites, in particular from mega-constellations such as Starlink, OneWeb, or Amazon Kuiper. Some of these satellites will emit signals in the upper-frequency range that is currently observed by the next-generation VLBI system, the VLBI Global Observing System (VGOS). The power of these signals may saturate the amplifiers of VLBI antennas causing nonlinearities within the observations. Besides, some planned InSAR satellites might emit signals strong enough to permanently damage the highly sensitive VLBI hardware.

Within this work, we will investigate an active mitigation approach that modifies the current VLBI observing strategy to avoid observations in the direction of SRFI. However, active avoidance means additional constraints during the observation planning. We will investigate the impact of these constraints w.r.t. the precision of the geodetic parameters using simulations and compare it to a situation without active avoidance, where affected observations are simply removed from the simulations, and to a situation without any SRFI being present. The simulations will be conducted based on current and future VGOS networks and current and future satellite constellation expansion stages. We will demonstrate that active avoidance has the potential to pose a solution to avoid SRFI but also highlight its limitations.

 

How to cite: Schartner, M. and Soja, B.: Active mitigation of spaceborne radio frequency interference for VLBI, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-6419, https://doi.org/10.5194/egusphere-egu23-6419, 2023.

14:20–14:30
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EGU23-7746
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On-site presentation
Julia Pfeffer, Anny Cazenave, Séverine Rosat, Mioara Mandea, Véronique Dehant, Lorena Moreira, and Anne Barnoud

A cycle of about 6 years has long been observed in the Earth’s magnetic field, length of day, dynamic oblateness, polar motions and surface displacements and attributed to dynamical processes occurring in the core and at the core mantle boundary. Recently, a 6-year cycle has also been detected in the rate of change of the global mean sea level and the ice-mass contributions from Greenland and continental glaciers. In this study, we report new observations of a 6-year cycle in the terrestrial water storage estimates based on the satellite gravity missions GRACE and GRACE-FO, consistent with precipitation and global hydrological models. The causes for such oscillations in the climate system are still unexplained, but raise the question of the respective contributions of the Earth’s deep interior and external surface fluid envelopes to the 6-year cycles reported in many geodetic variables. Indeed, while some of these 6-year fluctuations are convincingly attributed to Earth’s deep interior processes, for some other variables, climate-related processes occurring in the surface fluid envelopes or at the Earth’s surface may be more likely. This issue is exacerbated by an opposition of phase discovered between the angular momentum of the atmosphere and the length of day at around 6 years, suggesting that dynamical processes occurring in the Earth’s core induce a rotation of the solid Earth and the atmosphere as a single system. An overview of the 6-yr cycle observed in different variables of the Earth System may therefore help to better understand potential links between the solid Earth and climate.

How to cite: Pfeffer, J., Cazenave, A., Rosat, S., Mandea, M., Dehant, V., Moreira, L., and Barnoud, A.: Detections of a 6-year cycle in the Earth system, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-7746, https://doi.org/10.5194/egusphere-egu23-7746, 2023.

14:30–14:40
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EGU23-9321
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ECS
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On-site presentation
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Elmas Sinem Ince, Christoph Förste, Oleh Abrykosov, and Frank Flechtner

The gravity field plays a crucial role in Earth System Sciences. Access to the entire field on global scale is only possible via mathematical modelling. The heterogeneous gravity field shapes the mean sea level surface and can be used e.g., to determine ocean surface currents, to unify height systems globally, and to map mass distributions that mirror the processes in Earth’s interior, such as plate tectonics, mantle convection, seafloor spreading and volcanic eruption. Currently available static global gravity field models are limited in resolution due to the band-limited spectral content of the input data from satellite observations and gravity measurements on the Earth’s surface. We can complement such models beyond their current limits using high-resolution digital elevation models (DEMs) and laterally varying density estimates. Here we present a study, where we aim to compute a new very high-resolution topographic gravity field model in terms of harmonic coefficients via direct numerical integration of Newton’s law of gravitation using state-of-the-art DEM and density models. This work is a continuation of our previous activities in this field (Ince et al. 2020) and first results of a DFG project GRAV4GEO (GRAVitational field modelling of Earth’s topography For GEOdetic and GEOphysical applications). The outcomes of this project will be reduction of the omission error and enhancement of the spectral and spatial resolution of global gravity field models and delivery of topography/density-based gravity information particularly in hard-to reach areas. A third result will be the improved reduction of the gravity measurements for the topographic effect to investigate the residual signal of deeper Earth layers. This should help in the 3D crustal and lithospheric modelling especially in geologically complex areas, Finally, improvement in the accuracy of gravity modelling is expected from using laterally varying density instead of the commonly used averaged density values. With the high-resolution topographic gravity field model delivered at the end of the project, the spatial resolution of recent global gravity field models shall be increased up to ~2 km Uncertainty estimates, which have not been presented in current topographic gravity field models, will be provided. Our project will lead to an improved global gravity field up to degree/order 10800 which will also deliver a more accurate reference surface for global vertical datum and basis for better geophysical modelling especially in the regions of density discontinuities. In this presentation, we will be conveying the first results of the project which uses a laterally varying density model in the development of topographic gravity field model and its contribution to the state-of-the-art model EIGEN-6C4.

 

Reference:

Ince ES, Abrykosov O, Förste C, and Flechtner F (2020) Forward Gravity Modelling to Augment High-Resolution Combined Gravity Field Models. Surv. Geop., 1-38. doi:10.1007/s10712-020-09590-9

How to cite: Ince, E. S., Förste, C., Abrykosov, O., and Flechtner, F.: Towards a very High-Resolution Global Gravity Field Model up to degree and order 10800 based on Forward Modelling of the Earth’s Topography, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-9321, https://doi.org/10.5194/egusphere-egu23-9321, 2023.

Satellite Altimetry
14:40–14:50
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EGU23-701
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ECS
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On-site presentation
Sergi Hernández, Ferran Gibert, Antoni Broquetas, Albert Garcia-Mondéjar, Marcel Kleinherenbrink, and Mònica Roca

The Copernicus Sentinel-6 mission was planned to keep studying the sea-surface height and ocean state measurements and since April 2022 its first satellite, the Sentinel-6 Michael Freilich (S6MF), has become the current reference altimetry mission.

One of the key design aspects of the S6MF altimeter is the “interleaved” chronogram pattern, which increases the number of received pulses, reducing the ambiguities in the along-track dimension, and increasing the energy obtained from the surface. Thanks to the continuous surface illumination, the echoes from the same target can be coherently integrated making a significant improvement in the along-track resolution leading to more detailed understanding of the ocean, the polar zones and inland and coastal waters dynamics. Measurement parameters such as swell state, lead and iceberg detection or inland water level changes can take advantage of these advances.

Nowadays, unfocused azimuth steering methods, such as Delay Doppler, provide along-track resolutions around 300 meters. However Fully-Focused SAR (FF-SAR) algorithms can improve it to the order of sub-meter.  In 2017, Alejandro Egido and Walter H.F. Smith published the FF-SAR method description, based on the backprojection approach. Compared to the unfocused steering, it requires more computational time, making it difficult to be implemented operationally, keeping the data generation rate in the same order of magnitude as the unfocused chain products. In 2018, Pietro Guccione et. al. published the FF-SAR 2D Frequency Domain algorithm, based on the Omega-K (WK) algorithm from SAR radar. In this paper, it is shown that the two dimensional frequency domain can be used to decrease the number of operations needed to focus the data, under some circumstances that depend on the type of orbit and the emitted signal. FF-SAR WK algorithm achieves similar results in terms of along-track resolution for the CryoSat-2 mission, but notably improving the computational efficiency. Although Omega-K algorithm intrinsic assumptions can impact negatively in the accuracy estimation of parameters such as the sea surface height, there are applications like sea ice related activities that could benefit of faster execution times. In this presentation, an adapted and redesigned Omega-K algorithm for Sentinel-6 is presented. FF-SAR Omega-K and Backprojection have been used to process Sentinel-6 data over the Crete transponder, evidencing that both FF-SAR methods are capable to achieve the expected theoretical along-track resolution. Moreover, open ocean data from Sentinel-6 has been processed for both algorithms and results have been compared.

How to cite: Hernández, S., Gibert, F., Broquetas, A., Garcia-Mondéjar, A., Kleinherenbrink, M., and Roca, M.: ¿Why should we process Fully-Focused Radar Altimetry data in near real time? Improving the computational efficiency of FF-SAR using Omega-K based algorithm., EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-701, https://doi.org/10.5194/egusphere-egu23-701, 2023.

14:50–15:00
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EGU23-3689
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ECS
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On-site presentation
Qi Huang, Malcolm McMillan, Alan Muir, Joe Phillips, and Thomas Slater

Sea level rise is among the most pressing environmental, social and economic challenges facing humanity, and requires timely and reliable information for adaptation and mitigation. The ice sheets of Greenland and Antarctica currently contribute approximately one third of global sea level rise, yet monitoring their coastal regions, which are often populated by numerous, highly dynamic outlet glaciers remains a challenge. One of the principal methods for monitoring ice sheet change is that of satellite radar altimetry, which provides a near continuous 30-year record of surface elevation and volume change. However, this technique can suffer from incomplete measurements and larger uncertainties over rugged coastal topography, where the instrument may fail to track the ice surface, or may record multiple distinct reflections within the illuminated ground footprint. In these situations, current Level 2 processing approaches can be sub-optimal, leading to inaccuracies being introduced into the resulting elevation measurements. Therefore, this study aims to explore new approaches to retrieving elevation measurements, comprising (1) multipeak waveform retracking and (2) a refined slope correction approach over complex regions. The developed approaches offer the potential for multiple elevation retrievals from a single waveform, and in turn the opportunity to increase both the reliability and quantity of elevation measurements.

Within the study, these processing techniques were developed and evaluated across Russell Glacier and the whole Greenland as two typical test cases, based upon Sentinel-3 SAR altimeter acquisitions over ice sheet regions that exhibit complex topography. Laser altimeters including Airborne Topographic Mapper (ATM) and Ice, Cloud, and Land Elevation Satellite-2 (IceSat-2) data were used as independent validation sources. Ice sheet wide analysis showed that the developed approaches were capable of delivering equally high accuracy for multiple elevation retrievals with comparable dispersion (~ 1 m) but much lower bias (~ 0.5 m) and outliers (~ 4%) compared to standard Level-2 products (~ 4 m bias and ~ 20% outliers). The developed approaches have the potential to further extend the capability of satellite radar altimetry over complex glaciological targets, and to improve the accuracy and coverage of altimeter measurements across these regions.

How to cite: Huang, Q., McMillan, M., Muir, A., Phillips, J., and Slater, T.: New approaches to processing radar altimetry waveforms over complex ice sheet topography, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-3689, https://doi.org/10.5194/egusphere-egu23-3689, 2023.

15:00–15:10
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EGU23-12885
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On-site presentation
Tadea Veng and Felix Müller

The sea surface slope can be determined from satellite altimetry and used to determine geostrophic surface currents. If these currents change over time, heat transport in the oceans will change as well, with potential impacts on continental temperatures. In Europe these temperatures are partly
influenced by geostrophic currents in the Arctic Ocean and it is therefore of great interest to know whether these currents have changed in the past 10-20 years. 

One of the primary altimetry missions used for observing the Arctic region is CryoSat-2. Its advantages include a high inclination angle and the use of altimetric interferometry. The CryoSat-2 SARin acquisition mode has the highest spatial resolution and mostly covers coastal areas. 

Altimetric sea surface measurements are sparse in the Arctic, due to the presence of sea ice, reduced data quality near the coast, and limited satellite coverage near the pole. The detection of leads (openings in the sea ice) allows for measurements of the sea surface, even in the presence
of sea ice. Reliably detecting locations of leads is therefore the first step in determining the sea surface slope in the Arctic Ocean. This study aims to increase the number of accurately detected leads, by designing and implementing an unsupervised machine learning algorithm for CryoSat-2 SARin data

Sea ice and leads have different scattering properties, resulting in different altimetry waveform shapes. By defining a set of quantitative features to describe the waveform shape, the waveforms can be clustered based on similarities within this feature space. The features are chosen to provide
a clear distinction between sea ice and leads. A great advantage of the unsupervised classification is that no pre-labelled data are required. When new data are made available, waveforms can be assigned to an existing cluster by the K-nearest-neighbour method. Therefore, the creation of the
clusters has to be done only once. 

In order to validate the algorithm, the classification results are compared with the outputs of lead detection algorithms based on other data sources. Due to the limited number of SARin observations, results from both optical imagery and SAR imagery are used for statistical robustness.

How to cite: Veng, T. and Müller, F.: SARin lead dectection algorithm for Cryosat-2 using unsupervised classification, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-12885, https://doi.org/10.5194/egusphere-egu23-12885, 2023.

15:10–15:20
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EGU23-11155
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ECS
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On-site presentation
Kirk M. Scanlan, Sebastian B. Simonsen, Anja Rutishauser, and Baptiste Vandecrux

Recent research has demonstrated how Greenland Ice Sheet (GrIS) near-surface density and wavelength-scale surface roughness can be estimated from satellite radar altimetry surface echo powers by way of the Radar Statistical Reconnaissance (RSR) technique, the adoption of a radar backscattering model (i.e., the small perturbation model, SPM) and calibration using in situ density profiles. Patterns in the estimated density results 1) highlight an inter-annual variability that covaries with known climatic drivers (e.g., extremely warm 2012 Greenland summer temperatures) and 2) suggest that density estimates derived from different frequency radar echoes (Ku-band from ESA CryoSat-2 and Ka-band from CNES/ISRO SARAL) correspond to different depths in the near-surface (with Ku-band densities being deeper than those from Ka). When expressed as fractions of their respective signal wavelengths, the CryoSat-2 and SARAL surface roughness estimates 1) exhibit good agreement, 2) recover anticipated surface roughness conditions (i.e., a smooth GrIS interior and rougher margin) and 3) demonstrate minimal temporal variability.

Here we present on-going work directed at validating both the use of the small perturbation model as well as the implied density-depth sensitivity in these new remote sensing observations. First, the suitability of the SPM is evaluated using the in situ density cores as well as airborne radar/laser altimetry measurements acquired along the EGIG line during the 2017 and 2019 ESA CryoVEx campaigns. Second, to quantify the depth range to which the satellite radar altimetry Ku- and Ka-band density estimates apply, we compare them against more than 400 contemporaneous (2011-2019) measured in situ density cores across the GrIS. These validation exercises are crucial to understanding the nature of these new satellite-based observations of the near-surface properties of the GrIS that, in turn, will facilitate more accurate estimations of the current and future GrIS mass balance.

How to cite: Scanlan, K. M., Simonsen, S. B., Rutishauser, A., and Vandecrux, B.: Validating Satellite Radar Altimetry-Derived Greenland Near-Surface Density and Surface Roughness using in situ and Airborne Datasets, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-11155, https://doi.org/10.5194/egusphere-egu23-11155, 2023.

15:20–15:30
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EGU23-13545
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ECS
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On-site presentation
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Maria T. Kappelsberger, Martin Horwath, Eric Buchta, Matthias O. Willen, Ludwig Schröder, Sanne B.M. Veldhuijsen, Peter Kuipers Munneke, and Michiel R. van den Broeke

On interannual to decadal timescales, surface mass balance (SMB) exerts an important control over variations in the overall mass balance of the Antarctic Ice Sheet (AIS). A proper characterization of this variability is required to determine statistically significant long-term trends in SMB in a robust manner. To do so, we quantify variations in SMB and firn thickness by combining results from multi-mission satellite altimetry and SMB/firn modelling at grid scale. The objective of this study is twofold: First, we characterise the errors in both the altimetry and firn model in a spatially and temporally highly-resolved way. Second, we introduce a new approach that sets the stage for inferring long-term trends in SMB and firn processes at grid scale by taking into account interannual firn thickness variations. We use observed altimetric elevation changes of the AIS from Schröder et al. (2019; doi: 10.5194/tc-13-427-2019) and Nilsson et al. (2022; doi: 10.5194/essd-14-3573-2022) and modelled elevation changes of the AIS from IMAU-FDM v1.2A over the period 05/1992 to 12/2017. We assume that the firn model is able to capture the timing of variations in SMB and firn processes, but not necessarily the amplitude of these variations. The location-dependent amplitude is adjusted to the altimetry observations. We detect highest absolute differences between modelled and observed amplitudes at lower elevations, near the AIS margins. In a relative sense, the largest mismatch in amplitude is found in the dry interior of the East AIS across wind glazed areas of e.g. megadune fields. About 37 % of the variance in altimetry is captured by the adjusted firn thickness variations while about 64 % cannot be explained and is still included in the residuals. These residuals contain both altimetry errors (time-variable penetration and scattering effects of radar signals, intermode and intermission offsets) and firn model errors, like real SMB and firn processes not captured by the model. We identify that the time series of altimetric residuals are highly correlated and conclude that we need to consider an appropriate noise model for determining long-term trends and their uncertainties.

How to cite: Kappelsberger, M. T., Horwath, M., Buchta, E., Willen, M. O., Schröder, L., Veldhuijsen, S. B. M., Kuipers Munneke, P., and van den Broeke, M. R.: Antarctic firn thickness variations from multi-mission satellite altimetry and firn modelling, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-13545, https://doi.org/10.5194/egusphere-egu23-13545, 2023.

15:30–15:40
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EGU23-11956
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On-site presentation
Christian Schwatke, Michał Halicki, and Daniel Scherer

Water surface slope (WSS) of rivers is a key parameter in hydrological modelling, which allows for estimation of the transport and erosion capacity of a river, its flow velocity and discharge. On a local scale, WSS can be measured with a GNSS receiver installed on a boat, using remote sensing techniques (e.g. airborne lidar) or from a Digital Elevation Model (DEM). The most accurate method to measure WSS avoiding high-cost field campaigns is based on Water Surface Elevations (WSE) measured at in-situ stations. However, in poorly gauged rivers the neighboring gauges can be up to hundreds of kilometers apart, which inhibits a proper river profile observation. The gap in decreasing number of gauge readings is partially filled with satellite altimetry over rivers. Altimetry based WSE can be used to estimate WSS between neighboring measurements. Here, we present an innovative approach for estimating high-resolution WSS derived from multi-mission satellite altimetry for the largest Polish rivers.

In this study, we used measurements from 9 altimetry missions: CryoSat-2, Envisat, ICESat-2, Jason-2/-3, SARAL, Sentinel-3A/-B, and Sentinel-6A. These observations cover the years from 2002 to 2022. We extracted the river centerlines from the global “SWOT Mission River Database” (SWORD). In order to validate the obtained results, we used WSE from 81 gauges, which are maintained by the Institute of Meteorology and Water Management – National Research Institute (Instytut Meteorologii i Gospodarki Wodnej – Państwowy Instytut Badawczy, IMGW-PIB). These measurements are referenced to the Kronsztadt’86 vertical datum and they range from 01.2016 to 05.2022. Additionally, we used the reach-scale “ICESat-2 River Surface Slope” (IRIS) and the DEM-derived WSS values from SWORD.

To obtain WSS, we first determined WSE at each satellite pass crossing the studied river. Next, we split rivers into sections without dams and reservoirs. The Support Vector Regression (SVR) has been applied to reject outliers. Then, water levels were assigned to a given river kilometer (bin). For each of them a median WSE has been calculated. Finally, WSS were calculated at river sections between bins, excluding those disrupted by hydraulic structures. Finally, we weighted the section-wise WSS inversely proportional to the length of each section and applied a Least Square Adjustment with an additional Laplace condition to obtain bin-wise WSS for each river kilometer.

To assess the accuracy of the proposed approach, we compared the obtained WSS with the slopes between IMGW-PIB gauges. For large rivers (Vistula, Odra, Warta), the multi-mission approach revealed high accuracy with preliminary Root Mean Squared Error (RMSE) below 30 mm/km. For smaller, mountain rivers (San, Dunajec) the preliminary errors were slightly larger (RMSE ~100 mm/km). We also compared our accuracies with those of the slopes based on DEM models, lidar data, ICESat-2 altimetry, and SWORD database. In general, the multi-mission approach revealed the highest accuracy. The research is supported by the National Science Centre, Poland, through the project no. 2020/38/E/ST10/00295.

How to cite: Schwatke, C., Halicki, M., and Scherer, D.: High-resolution water surface slope of Polish rivers from two decades of multi-mission satellite altimetry measurements, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-11956, https://doi.org/10.5194/egusphere-egu23-11956, 2023.

Posters on site: Thu, 27 Apr, 16:15–18:00 | Hall X2

Chairpersons: Annette Eicker, Louise Sandberg Sørensen, Roelof Rietbroek
Satellite Altimetry
X2.65
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EGU23-9347
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ECS
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Joe Phillips and Mal McMillan

Although much progress has been made into satellite-based observations of Antarctic ice sheet (AIS) change in recent decades, to further reduce remaining uncertainties in existing methodologies, we need to better understand limitations in source data quality. Whilst a range of techniques exist for remote observation of the cryosphere, our understanding of ice sheet change is largely informed by satellite observations, with the longest continuous record coming from satellite radar altimetry. This technique derives information relating to the topographic and electromagnetic scattering characteristics of the ice surface, by emitting radar pulses and recording the timing and shape of the backscattered echoes. 

Launched in 2016, the Copernicus Sentinel-3 (S3) mission is the most recent in a 25-year long series of satellite altimetry missions, comprised of twin satellites dedicated to water surface topography, temperature and optical radiometry over land and ocean. S3 carries a Ku-band synthetic aperture radar altimeter (SRAL), which utilises delay-doppler processing to generate high-resolution (~300 m) along-track measurements every 27 days, thereby maximising information retrieval over more variable terrain surfaces that are challenging for conventional pulse limited altimeter systems. Whilst S3 provides high accuracy and sub-decimetre precision over oceans and uniform terrain, performance over more complex topography is challenging, with waveforms strongly diverging from their theoretical shape, as well as difficulties in capturing returns and successfully locating the true echoing point within the satellite beam footprint. As these issues significantly complicate the reliable retrieval of surface elevation information, handling them is one of the major challenges associated with processing altimetry data over regions of high-interest, complex topography, such as the Antarctic peninsula, outlet glacier interiors, and coastal ice sheet regions. These concerns are further exacerbated by the fact that S3 has a much smaller range window than other missions (such as Cryosat-2) due its primary use in oceanography.  

Several validation studies have already been performed for S3 in the context of the cryosphere, including cyclical and annual reports by the Sentinel-3 Mission Performance Centre. Whilst these studies predominantly concentrate on measured elevation accuracy and precision, they do not always perform investigations into lower-level performance, and hence a comprehensive understanding of the origin of measurement variability. Here we therefore investigate S3 performance in more depth using REMA (Reference Elevation Model of Antarctica), a widely used, high-resolution digital elevation model that covers almost all of Antarctica.  Specifically, we investigate three components of performance, (1) echo capture within the L1b range window, (2) variations in the assumed echoing point, and (3) waveform correlation along-track. By comparing this information to ice sheet-wide REMA-derived surface slope and roughness statistics, we can assess the impact of ice sheet surface topography on S3 performance, at scale. By doing so, we hope to ultimately improve our understanding of S3 performance over ice sheets and provide insight useful for the design of future missions such as CRISTAL. 

How to cite: Phillips, J. and McMillan, M.: Assessment of Sentinel-3 Altimeter Performance over Antarctica, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-9347, https://doi.org/10.5194/egusphere-egu23-9347, 2023.

X2.66
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EGU23-16764
Veit Helm, Hanna Wenzel, and Angelika Humbert

Mass changes of the polar Ice Sheets and their contribution to global mean sea level is an essential climate variable, critical for adaptation planning and important to understand the earth system in a warming climate. To ensure long term continuation of ice elevation and change records ESA proposed the Copernicus Polar Ice and Snow Topography Altimeter mission (CRISTAL) to be launched in 2027. CRISTAL, for the first time, will carry a dual-frequency altimeter in Ku and Ka Band to monitor changes in the height of ice sheets and glaciers and thickness of and snow on sea ice. Therefore, with the upcoming CRISTAL mission it is absolutely necessary to focus on sensor specific characteristics and its impact on elevation change records beforehand. To tackle these questions, we determine surface elevation change rates with a focus on the last decade of laser and radar altimetry observations using ICESat2, CryoSat-2, Sentinel-3 and SARAL/Altika. We investigate ice sheet wide and regional differences of elevation change rates derived from the four missions in the period from 2019 to 2022 with focus on different sensor characteristics (Laser/Ku/Ka Band), different acquisition/processing strategies ((P)LRM, SAR, SARIn), retracking (TFMRA,ICE1,ICE2) and orbit geometry (81.5°/88°).

Our findings show that trend estimates of individual missions diverge most strongly at the margins and areas of complex topography but also in the flat interior of ice sheets and are highly dependent on the choice of retracker. We show that in order to determine volume changes as consistently as possible across missions, a uniform processing is required that includes backscatter/leading edge correction to suppress the influence of time-varying radar penetration due to changes in volume scattering.

How to cite: Helm, V., Wenzel, H., and Humbert, A.: Comparison of recent multi mission elevation change rates of Greenland and Antarctica, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-16764, https://doi.org/10.5194/egusphere-egu23-16764, 2023.

X2.67
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EGU23-11409
Ludwig Schröder, Gunter Liebsch, Tobias Bauer, Lukas Rüsch, and Ulf Gräwe

The Federal Agency for Cartography and Geodesy (BKG) is the central service provider of topographic data, cartography, and geodetic reference systems for the German government. As the marine sector is constantly gaining importance, e.g. for the transport of goods or energy security, precise geodetic information become more and more important. In this context, BKG uses satellite altimetry to map and monitor the sea surface heights of the North and the Baltic Sea. In order to calibrate and validate the satellite observations, we performed measurements on the offshore research platform FINO2 as well as on two shipborne field campaigns during 2021 and 2022. In order to improve the spatial and temporal resolution of the altimetry data, we combine the altimetry observations with the output of a regional ocean model from Leibniz Institute for Baltic Sea Research (IOW). Here we present the first results of these activities and our strategy of combining satellite altimetry with different other observation techniques of sea level changes and land uplift to map and monitor elevation and elevation changes in the German coastal zone.

How to cite: Schröder, L., Liebsch, G., Bauer, T., Rüsch, L., and Gräwe, U.: Mapping Elevation and Elevation Changes in the German Coastal Zone, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-11409, https://doi.org/10.5194/egusphere-egu23-11409, 2023.

X2.68
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EGU23-14669
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ECS
Clémence Chupin, Valérie Ballu, Laurent Testut, and Yann-Treden Tranchant

The Lagoon surrounding New Caledonia is a site of high interest for satellite altimetry, both for classical nadir missions and for the new SWOT wide swath mission, with dedicated calibration/validation (Cal/Val) experiments planned in 2023 during its 1-D repeat orbit.

This poster provides updated results from the 3-weeks campaign GEOCEAN-NC 2019, where various geodetic sea-level observing systems were deployed in the Lagoon (e.g. GNSS Buoy, pressure sensor, CalNaGeo GNSS towed carpet). By combining these data, we reconstruct the dynamics of the lagoon at a point of interest where 3 altimetric tracks intersect (i.e. 1 Jason and 2 Sentinel-3a tracks), and then virtually transfer the Noumea tide gauge records at this particular location.  

With this approach, we reconstruct two long sea-level time series (i.e. in-situ and altimetry) in the heart of the Lagoon, enabling us to compute altimetry biases and inter-mission biases comparable to those of historical Cal/Val sites for the whole Jason 1/2/3 period and for Sentinel-3a. This update of our results allows us to extend the comparison with new data from year 2022, and consolidate the vertical reference frame used to link our sensors. It is also an opportunity to try to reconcile sea-level rise trends with vertical land movements of permanent GNSS stations, which remains an issue in this area.

How to cite: Chupin, C., Ballu, V., Testut, L., and Tranchant, Y.-T.: Geodetic instrumentation to validate altimetry sea-level measurements in the Noumea Lagoon – New results from the GEOCEAN-NC 2019 field mission, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-14669, https://doi.org/10.5194/egusphere-egu23-14669, 2023.

X2.69
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EGU23-15280
Matthieu Talpe, Philip Jales, Vu Nguyen, Jessica Cartwright, Takayuki Yuasa, and Oleguer Nogues-Correig

Spire Global operates a constellation of smallsats equipped with an advanced GNSS receiver designed to collect radio occultation observations and reprogrammed to detect surface reflections. Nguyen et al. [2020] demonstrated the feasibility of phase delay altimetry using coherent reflections, following a number of prior studies (e.g., Martín-Neira [1993], Cardellach et al. [2004]). Since then, Level 2 grazing angle altimetry products have been generated on an operational basis. As of January 2023, over 20 satellites continuously measure GNSS-R grazing angle reflection events in areas of high-coherence, i.e., calm waters and glaciated surfaces, yielding nearly 500,000 kms of altimetry tracks every day. The vertical resolution is on the order of decimeters, as demonstrated by comparisons against reference surface models composed of an MSS and ocean tides. 

 

A growing number of studies have utilized these datasets to examine ocean surfaces, sea ice, ice caps, and inland water bodies. An overview of these scientific applications enabled by Spire’s products is provided, along with a description of the advantages and current disadvantages of GNSS-R altimetry as observed after nearly three years of operations. 

 

We will show a comparison between the cryospheric products from ICESat-2 and CryoSat-2 against Spire products with a focus on sea ice. The Spire constellation provides improved temporal and spatial coverage, due GNSS-R's bistatic geometry and the range of receiver orbits. The retrievals show particular sensitivity in the smoother young-ice surfaces. Decimeter-level sea ice signals are routinely detected and validated with SAR imagery. The Spire sea ice product could complement existing cryospheric products, particularly in light of the potential gap in measurements before the launch of CRISTAL. We will also discuss ongoing development to several aspects of the algorithm such as phase unwrapping and systematic, polar-wide sea ice freeboard extraction.

 

References

 

Cardellach, E., Ao, C. O., De la Torre Juárez, M., & Hajj, G. A. (2004). Carrier phase delay altimetry with GPS-reflection/occultation interferometry from low Earth orbiters. Geophysical Research Letters, 31(10), L10402.

Martín-Neira, M., (1993), A passive reflectometry and interferometry system (PARIS): Application to ocean altimetry, ESA J., vol. 17, no. 4, pp. 331–355.

Nguyen, V. A., et al. (2020), Initial GNSS Phase Altimetry Measurements From the Spire Satellite Constellation, Geophys. Res. Letters, vol. 47, no. 15.

How to cite: Talpe, M., Jales, P., Nguyen, V., Cartwright, J., Yuasa, T., and Nogues-Correig, O.: How can GNSS-R altimetry from the Spire constellation complement institutional altimetry missions?, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-15280, https://doi.org/10.5194/egusphere-egu23-15280, 2023.

Across Geodesy
X2.70
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EGU23-3036
Hee-Un Kim, Haseong Lee, So-Young Bang, Jimin Lee, and Sun-Cheon Park

On March 11, 2011, a magnitude 9.0 earthquake occurred in the Pacific Ocean off the Tohoku region, which greatly affected the crust of the Korean Peninsula. At the time of the Tohoku earthquake, the crust deformation of the Korean Peninsula moved about 30 mm in the eastward direction. This is the size corresponding to the annual average on the Korean Peninsula, and this displacement occurred in one day due to the earthquake. Therefore, in this study, the degree of impact of crustal movement on the Korean Peninsula before and after the Tohoku earthquake was analyzed using domestic and global GNSS observation data. The analysis was performed in two ways. The first was a time series analysis of the crustal movement on the Korean Peninsula based on the IGS observation station in order to globally observe the change in the crustal movement on the Korean Peninsula before and after the earthquake. Secondly, the movement of the inner crust of the Korean Peninsula was confirmed by analyzing the correlation of movement according to the distance from the epicenter. The analysis period is from January 1, 2005 to December 31, 2021. As a result, stations that moved in the southeast direction before the earthquake on the Korean Peninsula moved eastward after the earthquake. However, over time, it gradually moves in a southeasterly direction. The velocity was higher in the western region before the earthquake. At the time of the earthquake, the stations in the eastern area where closer to the epicenter moved more, but have since returned to a similar velocity to that before the earthquake. It seems to be recovering over time after the earthquake, but to be incompleted which means continuous monitoring is needed.

How to cite: Kim, H.-U., Lee, H., Bang, S.-Y., Lee, J., and Park, S.-C.: Velocity and displacement of Korean Peninsula after The 2011 Tohoku earthquake, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-3036, https://doi.org/10.5194/egusphere-egu23-3036, 2023.

X2.71
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EGU23-16667
Band-pass filtering based on the Fourier basis pursuit spectrum
(withdrawn)
Guocheng Wang, Lintao Liu, Dong Ren, and Huiwen Hu
X2.72
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EGU23-15962
Judit Benedek, Dániel István Csáki, and Gábor Papp

Since the 1960s, the Institute of Earth Physics and Space Science (EPSS) in Sopron has been using different types of tiltmeters with nanoradian sensitivity to observe geodynamic phenomena (e.g. tides). In principle, the high sensitivity and the long term mechanical stability of the recently developed sensors (e.g. Lippmann-type tiltmeters) make it possible to detect rock tilts related to small seismo-tectonic deformations. On this research field the extensive use of networks of these devices is expected in the future. For the correct comparision of tilt values measured by different sensors, the instruments must be calibrated by suitable devices realizing simple and standardized metrological principles. Due to the high sensitivity of Lippmann tiltmeters, traditional comparators (e.g. level balances) can only be used to determine the sensors' characteristics on average over the entire measurement range. In the range below microradian theoretically the Newtonian (gravitational) method can be used to test the capabilities of the tilt sensors. The poster on the one hand shows the Lippmann tiltmeters and level balance joint measurement results. On the other hand the modell computation are discussed, which shows that the off-axis variation of the gravitational vector generated by the vertical movement of the cylindrical ring mass of the Mátyáshegy moving mass calibration device can provide for calibration a sufficiently accurate reference signal having (15±0.02) nrad peak-to-peak amplitude. It is just in the range of tilt induced by earth tide effect, which is a “standard” signal component in the time series recorded in observatory environment. 

How to cite: Benedek, J., Csáki, D. I., and Papp, G.: A review of traditional and new methods applicable for the calibration of high resolution tilt sensors, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-15962, https://doi.org/10.5194/egusphere-egu23-15962, 2023.

X2.73
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EGU23-11520
Maria Karbon, Santiago Belda, Esther Azcue Infanzon, Alberto Escapa, Juan Antonio Martinez Marin, Mariana Moreira, Victor Puente Garcia, and Jose Manuel Ferrandiz

Very Long Baseline Interferometry (VLBI) is a highly accurate method, used since the 1970s in astrophysics as well as in geodesy. It contributes significantly to the global international terrestrial reference frame (ITRF) and is the only space geodetic technique able to realize the international celestial reference frame (ICRF) as well as to observe the full set of Earth orientation parameters (EOP: polar motion, universal time, precession / nutation). The IVS (International VLBI Service for Geodesy and Astrometry) analysis center in Alicante UAVAC (University of Alicante VLBI) was established as an associate AC in 2018 at the department of Applied Mathematics at the University of Alicante, within the research group of space geodesy and space dynamics. Further, we have a close partnership with the IGN (Instituto Geográfico Nacional) and RAEGE (Red Atlántica de Estaciones Geodinámicas y Espaciales / Rede Atlântica de Estações Geodinâmicas e Espaciais). In the first quarter of 2022 we started with the first steps to become an operational AC, with the final goal to be a full contributor to future ICRF and ITRF realizations, as well as operational products like the IVS combined EOP products. In this report we introduce the community to our group, our technical setups in terms of hard- and soft-ware, as well as our preliminary products. We present the first results based on our reanalysis of the IVS-archives (1979-12.2022) using VieVS 3.2 (one of several software we plan on using), and show the main geodetic products, i.e. EOP, CRF and TRF.

 

How to cite: Karbon, M., Belda, S., Azcue Infanzon, E., Escapa, A., Martinez Marin, J. A., Moreira, M., Puente Garcia, V., and Ferrandiz, J. M.: Alicante IVS Analysis Center, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-11520, https://doi.org/10.5194/egusphere-egu23-11520, 2023.

Posters virtual: Thu, 27 Apr, 16:15–18:00 | vHall GMPV/G/GD/SM

Chairpersons: Andreas Kvas, Karina Nielsen
Accross Geodesy
vGGGS.6
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EGU23-1965
Inese Varna, Ansis Zarins, and Augusts Rubans

Digital zenith camera (DZC) VESTA (VErtical by STArs) was developed at the University of Latvia and has achieved an accuracy of 0.1 arcseconds.

Currently, a detailed analysis of optimal measurement conditions and potential error sources of DZC VESTA is performed. This study focuses on:

  • testing various parameters of DZC VESTA measurement session: session length, image binning, exposure time;
  • effect of external conditions: average number of observed stars, temperature, humidity, pressure, wind speed, sky, microseismic;
  • a significant error source is atmospheric anomalous refraction at the zenith - the amplitudes of the observed zenith coordinate fluctuations reach several arcseconds, and the final vertical deflection (VD) values have amplitudes of approximately 0.2-0.5 arcseconds during the overnight session.

For measurement purpose, a test site with 4 points at a 50x50 meter distance was established and measurements there were started in May 2021. Moreover, it is planned to continue measurements at least for 2 years (till May 2023) to obtain vertical deflection time series at all 4 points of the test site, 1.9 years of regular measurements are completed so far. Several overnight measurement sessions were performed with two adjacent DZCs to investigate anomalous refraction. Preliminary analysis results of VD test site measurements will be presented.

This research has been supported by the European Regional Development Fund activity “Post-doctoral Research Aid”, project No.1.1.1.2/VIAA/4/20/666

How to cite: Varna, I., Zarins, A., and Rubans, A.: Digital zenith camera VESTA and vertical deflection test site measurement results, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-1965, https://doi.org/10.5194/egusphere-egu23-1965, 2023.

Satellite Altimetry
vGGGS.7
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EGU23-7328
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ECS
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Renée Mie Fredensborg Hansen, Henriette Skourup, Eero Rinne, Knut Vilhelm Høyland, Ioanna Merkouriadi, Jack Christopher Landy, and René Forsberg

The orbit manoeuvre, known as CRYO2ICE, that periodically aligned CryoSat-2 with ICESat-2, allows for unprecedented near-coincident radar and lidar observations targeted the polar regions. This is of particular interest to sea ice thickness studies, since snow on sea ice remains the largest contributor to altimetry-derived sea ice thickness uncertainties. To date, snow depth estimates from space have been acquired from passive microwave radiometers, and by using dual-frequency observations (Ku- and Ka-band, or laser and Ku-band). However, until now, dual-frequency observations have only been based on monthly averaged estimates at basin-scales, and while passive microwave-derived snow estimates are provided daily, they are only reliable over first-year ice. CRYO2ICE presents the possibility of investigating along-track snow depth on sea ice using observations at two different frequencies, along with an opportunity for further investigation of penetration capabilities and footprint-related issues of high interest to the altimetry community.

Some of the most noticeable differences between CryoSat-2 and ICESat-2 are found in their measurement configuration and sampling rates. This difference in measurement configuration between retrieving surface elevation using conventional ways, such as re-tracking of the synthetic aperture radar (SAR) waveform of CryoSat-2 in comparison to re-tracking the surface from high-density photon clouds of ICESat-2, as well as the difference in sampling rates, presents additional challenges. Here, we investigate the challenge of binning these different type of observation strategies into comparable observations and what we can expect from the CRYO2ICE observations over sea ice. We examine near-coincident radar and laser freeboards from CryoSat-2 and ICESat-2 (CRYO2ICE observations) and the resulting snow depth observations in the Arctic. We utilise three CryoSat-2 products (Baseline-D, CCI and LARM) representing a variety of re-trackers used in sea ice altimetry studies, and the ATL10 product from ICESat-2. Our focus is on how the CryoSat-2 and ICESat-2 derived freeboards respond along-track to various ice and snow conditions, and how this affects the possibility to retrieve snow depth.

This study investigates the freeboards and the derived snow depth in relation to changes in surface roughness, sea ice concentration and sea ice lead identifications. Here, we find inconsistencies in the radar freeboard estimates across the changing ice conditions. By comparison with sea ice concentration, identified leads and roughness estimates, the inconsistencies relate to retrieval methodology of CryoSat-2 (re-tracking to a backscattering interface using a threshold-based re-tracker or a physical re-tracker) and binning methodology (posing the question of when CRYO2ICE observations are truly comparable). Other inconsistencies relate to how the condition of the surface impacts the radar signal. We also present comparisons of radar and laser freeboards with daily estimates of snow depth based on passive-microwave observations (AMSR-2) and snow evolution models (SnowModel-LG). Here, large discrepancies are observed: AMSR-2 observations show little variation over first-year ice, compared to both estimates from SnowModel-LG and CRYO2ICE observations. CRYO2ICE snow depths are comparable across the used CryoSat-2 products but shows significantly larger variation compared to SnowModel-LG estimates. Future work includes delving more into the changing ice conditions and their impact on the radar signal.

How to cite: Hansen, R. M. F., Skourup, H., Rinne, E., Høyland, K. V., Merkouriadi, I., Landy, J. C., and Forsberg, R.: Arctic freeboards and snow depths from near-coincident CryoSat-2 and ICESat-2 (CRYO2ICE) observations during the winter 2020-2021: An examination across changing sea ice conditions, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-7328, https://doi.org/10.5194/egusphere-egu23-7328, 2023.