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Giant ice bulldozers: How ancient glaciers helped life evolve

Phys.org: Earth science - Tue, 02/25/2025 - 22:00
New Curtin University research has revealed how massive ancient glaciers acted like giant bulldozers, reshaping Earth's surface and paving the way for complex life to flourish.

Competing effects of global warming and sea surface temperature explain recent strengthening of the Walker circulation

Phys.org: Earth science - Tue, 02/25/2025 - 20:58
The Walker circulation, an atmospheric circulation pattern in the tropics, has accelerated in recent years, puzzling climate scientists who had anticipated the opposite. Researchers from the Max Planck Institute for Meteorology and the University of Tokyo have found out why by revealing the competing effects between global warming and the sea surface temperature pattern effect.

Seismometers reveal Earth's longest-runout undersea sediment flows in unprecedented detail

Phys.org: Earth science - Tue, 02/25/2025 - 19:23
Turbidity currents are an important natural process that often goes unnoticed: these powerful currents beneath the ocean surface carve deep submarine canyons, create huge sediment deposits and can damage submarine cables and pipelines. Although the phenomenon has been known for about 100 years, its high-energy nature has made it almost impossible to measure directly—any instruments placed in its path would be destroyed by its immense force, much like avalanches on land.

Characterizing PPP ambiguity resolution residuals for precise orbit and clock corrections integrity monitoring

GPS Solutions - Tue, 02/25/2025 - 00:00
Abstract

To meet the high-precision and high-integrity positioning demands of safety–critical applications, monitoring the quality of precise satellite products in global navigation satellite system (GNSS) precise point positioning (PPP) is crucial. This work employs ionosphere-free (IF) PPP with ambiguity resolution (PPP-AR) phase residuals to construct test statistics for monitoring the quality of precise satellite corrections. By utilizing precise satellite orbit and clock products from CODE, WUM, and GRG, the PPP-AR phase residuals were first analyzed with sample moments, Allan variance and power spectral density (PSD). The key findings are as follows: (1) The skewness and kurtosis results indicate that ambiguity-fixed phase residuals deviate from an ideal zero-mean Gaussian distribution and exhibit a super-Gaussian distribution. (2) Allan variance and PSD analysis reveal that flicker noise dominates the phase residuals. (3) The noise amplitudes are similar for all satellites, but certain differences are observed among different GNSS systems and satellite types. (4) The noise level of phase residuals is influenced by the receiver types, antenna types, and precise products from different analysis centers. Leveraging the error characteristics, the two-step Gaussian overbounding (OB) method was employed to estimate the corresponding OB parameters of the phase residuals. The overbounding results demonstrate that, under similar conditions, phase residuals can be bounded by the calculated bound within the acceptable integrity risk after removing the detected outliers. Anomaly monitoring experiments further show that phase residuals can effectively capture anomalies in precise satellite corrections, with the set threshold successfully detecting such anomalies.

Calibration of h'Es from VIPIR2 ionosondes in Japan

Earth,Planets and Space - Tue, 02/25/2025 - 00:00
The measurement of virtual height of the sporadic E layer (h'Es) is very sensitive to the type of ionosonde used and the calibration processes. The ionosondes used by the national institute of communication an...

Solar System Elemental Abundances from the Solar Photosphere and CI-Chondrites

Space Science Reviews - Mon, 02/24/2025 - 00:00
Abstract

Solar photospheric abundances and CI-chondrite compositions are reviewed and updated to obtain representative solar system abundances of the elements and their isotopes. The new photospheric abundances obtained here lead to higher solar metallicity. Full 3D NLTE photospheric analyses are only available for 11 elements. A quality index for analyses is introduced. For several elements, uncertainties remain large. Protosolar mass fractions are H (X = 0.7060), He (Y = 0.2753), and for metals Li to U (Z = 0.0187). The protosolar (C+N)/H agrees within 13% with the ratio for the solar core from the Borexino experiment. Elemental abundances in CI-chondrites were screened by analytical methods, sample sizes, and evaluated using concentration frequency distributions. Aqueously mobile elements (e.g., alkalis, alkaline earths, etc.) often deviate from normal distributions indicating mobilization and/or sequestration into carbonates, phosphates, and sulfates. Revised CI-chondrite abundances of non-volatile elements are similar to earlier estimates. The moderately volatile elements F and Sb are higher than before, as are C, Br and I, whereas the CI-abundances of Hg and N are now significantly lower. The solar system nuclide distribution curves of s-process elements agree within 4% with s-process predictions of Galactic chemical evolution models. P-process nuclide distributions are assessed. No obvious correlation of CI-chondritic to solar elemental abundance ratios with condensation temperatures is observed, nor is there one for ratios of CI-chondrites/solar wind abundances.

Contribution of microtopography off the Ryukyu Islands to coastal sea-level amplification during the 2022 Tonga meteotsunami

Earth,Planets and Space - Mon, 02/24/2025 - 00:00
The January 2022 Tonga volcanic eruption generated atmospheric pressure waves that propagated over the ocean’s surface and triggered a meteotsunami. This meteotsunami caused significant amplitudes exceeding 10...

A new ensemble learning method based on signal source driver for GNSS coordinate time series prediction

GPS Solutions - Sun, 02/23/2025 - 00:00
Abstract

Accurately modeling and prediction the nonlinear motion of GNSS (Global Navigation Satellite System) coordinate time series holds significant theoretical and practical value for the study of geodynamics. A novel integrated network, named Ensemble Learning method based on Signal Source Driver (ELSSD), is proposed, which leverages the strengths of Long Short-Term Memory (LSTM) and Deep Self-Attention Neural Network (DSANN), while integrating GNSS loading data as an additional data source. Additionally, a multi-track synchronous sliding window data processing strategy is designed to address the challenge of multi-source data fusion input. The effectiveness of this algorithm is validated using GNSS coordinate time series from 186 global stations over a period of 10 years. Experimental results initially illustrate that, when accounting for displacement caused by environmental loading effects, there is a marked improvement in the modeling and prediction accuracy compared with GNSS input-only. Furthermore, the application of three ensemble network strategies-Bagging, Boosting, and Stacking-have further been demonstrated to enhance modeling and prediction accuracy. Compared with LSTM and DSANN networks, the proposed ELSSD algorithm achieves an average RMSE (Root Mean Square Error) of 3.6 mm for both modeling and prediction, with modeling accuracy improvements of 4.8% and 6.2%, while prediction accuracy improvements of 5.4% and 5.9%, respectively. With respect to the traditional Least Square method, there is an improvement of 22.1% and 27.9% in modeling and prediction accuracy, respectively. Regarding noise characteristics, there is a significant reduction in colored noise amplitude, with decreases of 36.7% and 36.0% observed in modeling and prediction, respectively. Simultaneously, the velocity uncertainty experiences an average reduction of 27.1% and 27.5%. The average velocity differences are measured at 0.06 mm/year and 0.24 mm/year, respectively. Hence, our findings suggest that the ELSSD algorithm emerges as an effective methodology for handling multi-source data input in GNSS coordinate time series, presenting promising practical applications in the field.

Effects in the upper atmosphere and ionosphere in the subauroral region during Victory Day 2024 Geomagnetic Storm (May 10–12, 2024)

Publication date: Available online 11 February 2025

Source: Advances in Space Research

Author(s): A.A. Chernyshov, M.V. Klimenko, I.A. Nosikov, O.P. Borchevkina, A.V. Timchenko, I.I. Efishov, A.A. Sinevich, I.A. Ryakhovsky, G.A. Yakimova, F.S. Bessarab, I.S. Yankovsky, D.V. Chugunin

Analysis of multipath effects on LEO ranging-based positioning using BPSK and BOC signals in urban areas

Publication date: 1 February 2025

Source: Advances in Space Research, Volume 75, Issue 3

Author(s): Qi Zhang, Bing Xu

A non-singular predefined-time sliding mode tracking control for space manipulators

Publication date: 1 February 2025

Source: Advances in Space Research, Volume 75, Issue 3

Author(s): Yuxin Yan, Hutao Cui, Peng Han

Study on the safe landing of a crew module considering horizontal velocity using a DEM-FEM coupling algorithm

Publication date: 1 February 2025

Source: Advances in Space Research, Volume 75, Issue 3

Author(s): Shaomin Liang, Yuntian Feng, Zhihua Wang

Attitude synchronization of chaotic satellites with unknown dynamics using a neural network based fixed time sliding mode controller

Publication date: 1 February 2025

Source: Advances in Space Research, Volume 75, Issue 3

Author(s): Özhan Bingöl

Efficient approach of painting asteroids for planetary defense using network data envelopment analysis

Publication date: 1 February 2025

Source: Advances in Space Research, Volume 75, Issue 3

Author(s): Sajjad Aslani Khiavi, Mahdi Jafari-Nadoushan

Numerical investigation of prediction method for propagation delay of low-frequency radio signal based on the Changhe-II and Loran-C navigation system in East Asia

Publication date: 1 February 2025

Source: Advances in Space Research, Volume 75, Issue 3

Author(s): Jian Wang, Chengsong Duan, Cheng Yang, Qiao Yu

Optical measurements of precipitating relativistic electron microbursts during geomagnetic disturbance and pulsating aurora

Publication date: 1 February 2025

Source: Advances in Space Research, Volume 75, Issue 3

Author(s): Pavel Klimov, Vera Nikolaeva, Konstantin Shchelkanov, Roman Saraev, Ksenia Sigaeva, Andrei Kotikov, Alexander Belov, Boris Kozelov, Alexei Murashov, Alexei Roldugin

On the identification of the spatiotemporal locations of solar wind structures during an intense geomagnetic storm

Publication date: 1 February 2025

Source: Advances in Space Research, Volume 75, Issue 3

Author(s): Victor U. Chukwuma, Bolarinwa J. Adekoya, Eugene O. Onori, Oluwafunmilayo O. Ometan, Aghogho Ogwala

Indian Network for Space Weather Impact Monitoring (InSWIM): An initiative to observe and model the low latitude ionosphere over the Indian longitudes

Publication date: 1 February 2025

Source: Advances in Space Research, Volume 75, Issue 3

Author(s): R.K. Choudhary, K.M. Ambili, C. Vineeth, Ajay Potdar, Md. Mosarraf Hossain, Tarun K. Pant

Did the “Tauktae” cyclone impact the upper atmosphere through traveling ionospheric disturbances? A case study over the Arabian Sea using measurements from InSWIM network stations

Publication date: 1 February 2025

Source: Advances in Space Research, Volume 75, Issue 3

Author(s): Swati Chowdhury, R.K. Choudhary, D. Bala Subrahamanyam

Ionospheric changes immediately before the 2023 February Kahramanmaras earthquakes, Turkey

Publication date: 1 February 2025

Source: Advances in Space Research, Volume 75, Issue 3

Author(s): Ihsan Naufal Muafiry, Irwan Meilano, Dudy D. Wijaya, Erman Sentürk, Kosuke Heki

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