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The devastating 26 to 28 September 2024 rainfall event in Nepal

EOS - Tue, 08/12/2025 - 06:57

The most severe rainfall event ever recorded in Nepal impacted about 2.6 million people, causing losses of US$370 million and about 270 lives.

Between 26 and 28 September 2024, a devastating late monsoon rainfall event in Nepal triggered hundreds of landslides. In landslide terms, this was the most serious event recorded in Nepal outside of a major earthquake – economic losses are estimated to have been 1% of the country’s GDP and about 270 people were killed or left missing.

An initial analysis (Lamichhane et al. 2025 – the paper is behind a paywall, but the link should allow you to access it) has just been published in the journal Landslides – a very welcome paper. The authors, the majority of whom are Nepali, deserve praise for the speed at which this has been compiled, its comprehensive analysis and the diligence with which they have provided location information for the major events they describe. This is a model that others should seek to follow.

A substantial part of the paper examines the rainfall event itself. In central Nepal, 25 weather stations recorded their highest ever 24 hour rainfall. One station, at Godavari in Lalitpur District, recorded 311.6 mm. Peak hourly intensities were also high by Nepal standards – Godavari recorded 26.8 mm between 7 and 8 pm on 28 September 2024 – again, an unusually high figure for Nepal. Over the three day period, Godavari recorded 366.0 mm of rainfall.

Lamichhane et al. (2025) rightly highlight that the disaster was probably the consequence of a rainfall event that occurring in the late monsoon period, when the ground is already saturated, and that then involved high rainfall intensities, a high 24 hour rainfall total and a high 72 hour rainfall total. This is a toxic combination.

Lamichhane et al. (2025) then describe some of the more serious landslide events. The greatest losses occurred were caused by the Jhyaple Khola landslide, situated on the Tribhuvan Rajpath highway. The location is [27.71146, 85.20236] – the site is shown in the Google Earth image below, with the marker showing the point at which the landslide struck the road:-

Google Earth image of the site of the Jhyaple Khola landslide in Nepal, collected on 12 December 2023.

This is a Google Earth image of the site after the landslide:-

Google Earth image of the aftermath of the Jhyaple Khola landslide in Nepal, collected on 7 June 2025.

And here is a slider to allow you to compare the two:-

This landslide occurred at about 4 am on 28 September 2024. Unfortunately, two buses were at the site, trapped behind an earlier landslide.

Both buses were struck, killing 35 people. Lamichhane et al. (2025) describe the landslide as a 3 m deep debris flow that was rich with large pieces of woody debris. They rightly point out that the failure originated about 80 m above the road, but I would also highlight that the source appears to be another section of road. It is unclear to me as to whether the failure was on the cut slope above the road or a fill slope below it. That road appears on images from 2004, so it is not new.

Lamichhane et al. (2025) detail many other examples of landslides across Central Nepal, and even these are just a fraction of the total. Whilst the rainfall was unprecedented, they rightly highlight the anthropogenic issues that were the root of the disaster:-

“Major landslides and debris flow sites were linked to intense rainfall, unregulated sand mining, poorly managed rivers, haphazard road construction, and highly weathered slopes.”

In addition, they note that the following about the aftermath of the incident:-

“Despite involvement from various agencies, the disaster response fell short, underscoring the need for a more proactive approach to mitigation and management. Public response to rainfall warnings from agencies like Nepal’s Department of Hydrology and Meteorology (DHM) was also insufficient, contributing to tragic fatalities.

Nepal will face many more events like this in the coming years, and indeed an even larger rainfall event is probably just around the corner. Lamichhane et al. (2025) demonstrates that immediate action is needed. Sadly, I have low confidence that this occur. It feels inevitable that I will describe another event of this type on this blog in the coming years.

Reference

Lamichhane, K., Biswakarma, K., Acharya, B. et al. 2025 Preliminary assessment of September 2024 extreme rainfall–induced landslides in Central Nepal. Landslides. https://doi.org/10.1007/s10346-025-02577-w

Return to The Landslide Blog homepage Text © 2023. The authors. CC BY-NC-ND 3.0
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Нелинейная генерация течений волнами на поверхности жидкости

Успехи физических наук - Mon, 08/11/2025 - 21:00

С.С. Вергелес, А.А. Левченко, В.М. Парфеньев

Затухание поверхностных волн из-за вязкой диссипации сопровождается возбуждением медленных вихревых течений благодаря сохранению полного импульса. Мы представляем теоретическую модель для волн малой амплитуды, объясняющую эксперименты по генерации вихревых течений скрещенными волнами. Особое внимание уделено влиянию поверхностных загрязнений, которое учтено в рамках модели тонкой жидкой эластичной плёнки, приводящей к усилению диссипации волн и интенсификации вихревых течений. При увеличении амплитуды течений необходимо учитывать их взаимодействие с волнами. Предложена теоретическая схема, описывающая данное взаимодействие, с демонстрацией её применимости к классическим задачам: волнам Гуйона, распространению коротких волн навстречу течению и циркуляции Ленгмюра. В заключение описаны экспериментальные данные для турбулентного режима генерации течений, реализующегося при достаточно большой амплитуде волн, и обозначены открытые вопросы в этом направлении.

As the world churns: How bioturbation has shaped ocean floors over 540 million years

Phys.org: Earth science - Mon, 08/11/2025 - 20:06
The murky world at the bottom of the oceans is now a little clearer, thanks to a new study that tracks the evolution of marine sediment layers across hundreds of millions of years.

Kinetic full-wave analysis of injected electromagnetic wave in an inhomogeneous hot plasma

Physical Review E (Plasma physics) - Thu, 08/07/2025 - 10:00

Author(s): Shabbir A. Khan and Atsushi Fukuyama

Linear absorption of electromagnetic wave injected in a hot plasma is usually associated with non-normal incidence; here, it is shown that absorption can take place at normal incidence as well. By developing a kinetic model based on integral form of dielectric tensor in the presence of static electr…


[Phys. Rev. E 112, L023202] Published Thu Aug 07, 2025

Piecewise omnigenous stellarators with zero bootstrap current

Physical Review E (Plasma physics) - Wed, 08/06/2025 - 10:00

Author(s): Iván Calvo, José Luis Velasco, Per Helander, and Félix I. Parra

Until now, quasi-isodynamic magnetic fields have been the only known stellarator configurations that, at low collisionality, give small radial neoclassical transport and zero bootstrap current for arbitrary plasma profiles, the latter facilitating control of the magnetic configuration. The recently …


[Phys. Rev. E 112, L023201] Published Wed Aug 06, 2025

Demonstration of x-ray fluorescence spectroscopy as a sensitive temperature diagnostic for high-energy-density physics experiments

Physical Review E (Plasma physics) - Tue, 08/05/2025 - 10:00

Author(s): M. J. MacDonald, H. A. Scott, K. H. Ma, S. R. Klein, T. F. Baumann, R. W. Falcone, K. B. Fournier, C. M. Huntington, E. Johnsen, C. C. Kuranz, E. V. Marley, A. M. Saunders, M. P. Springstead, P. A. Sterne, M. R. Trantham, and T. Döppner

We present the use of x-ray fluorescence spectroscopy (XFS) to a sensitive temperature diagnostic in shocked foams at temperatures of 30–75 eV. Cobalt-doped foams were shock compressed using a planar drive at the OMEGA laser facility and photo-pumped with a Zn Heα x-ray source. Analysis of the resul…


[Phys. Rev. E 112, 025203] Published Tue Aug 05, 2025

Relaxation pathways in x-ray free-electron-laser heated iron

Physical Review E (Plasma physics) - Fri, 08/01/2025 - 10:00

Author(s): L. Ansia, P. Velarde, M. Fajardo, and G. O. Williams

Nonthermal photoionized plasmas are now established in the laboratory and require models that treat the atomic processes and electron distribution self-consistently. We investigate the effects of inelastic thermalization in iron under intense x-ray irradiation using the atomic model BigBarT, suited …


[Phys. Rev. E 112, 025201] Published Fri Aug 01, 2025

Impact of super-Gaussian electron distributions on plasma K-shell emission

Physical Review E (Plasma physics) - Fri, 08/01/2025 - 10:00

Author(s): H. P. Le, E. V. Marley, and H. A. Scott

Electron distributions in laser-produced plasmas will be driven toward a super-Gaussian distribution due to inverse bremsstrahlung absorption [Langdon, Phys. Rev. Lett. 44, 575 (1980)]. Both theoretical and experimental evidence suggest that fundamental plasma properties are altered by the super-Gau…


[Phys. Rev. E 112, 025202] Published Fri Aug 01, 2025

Experimental study of the rotation characteristics of magnetically driven vacuum-arc cathode spots

Physical Review E (Plasma physics) - Wed, 07/30/2025 - 10:00

Author(s): Yu-Xi Liu, Jin-Yue Geng, Hai-Xing Wang, Hao Yan, Xu-Hui Liu, Su-Rong Sun, Ao-wei Liu, and Tao Wu

Achieving uniform, stable, and reliable erosion of electrode materials is crucial for enhancing the performance and lifespan of vacuum-arc devices. This study investigates the rotation and erosion characteristics of cathode spots on Cu and Ti cathodes with various applied magnetic fields. The result…


[Phys. Rev. E 112, 015213] Published Wed Jul 30, 2025

Kilotesla magnetic field generation via ultraintense laser interaction with hollow microcapsule

Physical Review E (Plasma physics) - Mon, 07/28/2025 - 10:00

Author(s): S. Chintalwad and David J. Stark

We investigate the generation of kilotesla-level magnetic fields in laser-irradiated hollow conical targets through particle-in-cell simulations. This configuration proves effective in producing magnetic fields tens of kiloteslas in strength that persist on a picosecond timescale. Moreover, the holl…


[Phys. Rev. E 112, 015212] Published Mon Jul 28, 2025

Two-loop turbulent helical magnetohydrodynamics: Large-scale dynamo and energy spectrum

Physical Review E (Plasma physics) - Thu, 07/24/2025 - 10:00

Author(s): Michal Hnatič, Tomáš Lučivjanský, Lukáš Mižišin, Yurii Molotkov, and Andrei Ovsiannikov

We present a two-loop field-theoretic analysis of incompressible helical magnetohydrodynamics (MHD) in fully developed stationary turbulence. A key feature of helical MHD is the appearance of an infrared-unstable “masslike” term in the loop diagrams of the magnetic response function. Physically, thi…


[Phys. Rev. E 112, 015211] Published Thu Jul 24, 2025

Quantification of ion scattering by solar-wind current sheets: Pitch-angle diffusion rates

Physical Review E (Plasma physics) - Wed, 07/23/2025 - 10:00

Author(s): Zijin Zhang, Anton V. Artemyev, and Vassilis Angelopoulos

The transport of energetic particles in the heliosphere is profoundly influenced by interactions with coherent structures in the turbulent magnetic field of the solar wind, particularly current sheets. While prior studies have largely relied on idealized turbulence models, this work quantifies the r…


[Phys. Rev. E 112, 015209] Published Wed Jul 23, 2025

Weak decaying collective-excitation approximation for Yukawa one-component plasmas

Physical Review E (Plasma physics) - Wed, 07/23/2025 - 10:00

Author(s): Ilnaz I. Fairushin and Anatolii V. Mokshin

In this paper, the theoretical model of weak decaying collective excitations characteristic of many-particle systems with long-range interaction potentials is developed using the example of one-component strongly coupled Yukawa plasmas. The proposed model is based on the self-consistent relaxation t…


[Phys. Rev. E 112, 015210] Published Wed Jul 23, 2025

Nonlinear kinetic simulations of Jeans instability in a magnetized dusty plasma

Physical Review E (Plasma physics) - Mon, 07/21/2025 - 10:00

Author(s): Masaru Nakanotani, Luis Lazcano Torres, Gary P. Zank, and Edward Thomas, Jr.

The Jeans instability in a magnetized dusty plasma is considered a fundamental process in space, where magnetic fields are common. We investigate the Jeans instability in a magnetized dusty plasma using 1D and 2D particle-in-cell simulations, in which dust grains are treated as particles and the Poi…


[Phys. Rev. E 112, 015208] Published Mon Jul 21, 2025

Hot spot generation in hybrid $X$ pinches on a portable low-inductive KING generator

Physical Review E (Plasma physics) - Thu, 07/17/2025 - 10:00

Author(s): T. A. Shelkovenko, I. N. Tilikin, A. R. Mingaleev, V. M. Romanova, and S. A. Pikuz

The small-sized, low-voltage, and low-inductive KING generator (190–230 kA, 40 kV, 200–240 ns) was specially designed to work with X-pinches; however, it was unstable in its original design. In the present work, it is experimentally shown that an increase in the inductance of the output node of the …


[Phys. Rev. E 112, 015207] Published Thu Jul 17, 2025

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.

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