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        <title>NPG - recent papers</title>


    <link rel="self" href="https://npg.copernicus.org/articles/"/>
    <id>https://npg.copernicus.org/articles/</id>
    <updated>2026-06-08T15:13:02+02:00</updated>
    <author>
        <name>Copernicus Publications</name>
    </author>
        <entry>
            <id>https://doi.org/10.5194/npg-33-303-2026</id>
            <title type="html">Nonlinear quantitative relationship between the duration and occurrence frequency of droughts
            </title>
            <link href="https://doi.org/10.5194/npg-33-303-2026"/>
            <summary type="html">
                &lt;b&gt;Nonlinear quantitative relationship between the duration and occurrence frequency of droughts&lt;/b&gt;&lt;br&gt;
                Pengcheng Yan, Guolin Feng, Cailing Zhao, Ping Yang, Hao Wu, and Dongdong Zuo&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 303&#8211;312, https://doi.org/10.5194/npg-33-303-2026, 2026&lt;br&gt;
                In this study, we examine the relationship between drought duration and frequency across China using daily data. We find a clear double-logarithmic relationship between the duration and the frequency. We also show that droughts in dry northwestern areas tend to last for months, while those in wet southeastern regions are shorter but more frequent. This pattern holds across all drought intensities. Overall, our findings offer a simple tool for drought risk assessment and water management.
            </summary>
            <content type="html">
                &lt;b&gt;Nonlinear quantitative relationship between the duration and occurrence frequency of droughts&lt;/b&gt;&lt;br&gt;
                Pengcheng Yan, Guolin Feng, Cailing Zhao, Ping Yang, Hao Wu, and Dongdong Zuo&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 303&#8211;312, https://doi.org/10.5194/npg-33-303-2026, 2026&lt;br&gt;
                <p>This study aims to quantify the relationship between the duration and occurrence frequency of droughts in China, particularly focusing on different drought intensities. By analyzing daily meteorological drought composite index (MCI) data from 1897 meteorological stations across China spanning from 1961 to 2020, the study reveals a significant double-logarithmic relationship between drought duration and occurrence frequency. The results show that shorter drought durations are associated with higher occurrence frequencies, while longer durations correspond to lower frequencies. This relationship is characterized by parameter <span class="inline-formula"><i>k</i></span&gt; or <span class="inline-formula"><i>b</i></span>. Spatially, the values of the parameter exhibit a gradient from northwest to southeast, with higher values in arid and semi-arid regions and lower values in humid and semi-humid regions. Notably, the parameter <span class="inline-formula"><i>k</i></span&gt; aligns well with precipitation isolines, effectively distinguishing arid, semi-arid, and humid regions. Additionally, droughts in arid and semi-arid regions tend to last longer (often exceeding 60&amp;#8201;d), while those in humid and semi-humid regions are shorter but more frequent. These findings provide critical insights for optimizing water resource management, agricultural planning, and disaster mitigation strategies, enhancing societal resilience to drought impacts.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-08T15:13:02+02:00</published>
            <updated>2026-06-08T15:13:02+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-33-267-2026</id>
            <title type="html">Structural joint modeling of magnetotelluric data and Rayleigh wave dispersion curves using Pareto-based particle swarm optimization: an example to delineate  the crustal structure of the southeastern part  of the Biga Peninsula in western Anatolia
            </title>
            <link href="https://doi.org/10.5194/npg-33-267-2026"/>
            <summary type="html">
                &lt;b&gt;Structural joint modeling of magnetotelluric data and Rayleigh wave dispersion curves using Pareto-based particle swarm optimization: an example to delineate  the crustal structure of the southeastern part  of the Biga Peninsula in western Anatolia&lt;/b&gt;&lt;br&gt;
                Ersin Büyük, Ekrem Zor, and Mustafa Cengiz Tapırdamaz&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 267&#8211;302, https://doi.org/10.5194/npg-33-267-2026, 2026&lt;br&gt;
                <span data-olk-copy-source="MessageBody">We introduce a Pareto-based multi-objective particle swarm optimization framework for joint modeling of magnetotelluric and Rayleigh wave dispersion data from the southeastern Biga Peninsula. The approach uses a shared structural parameterization without enforcing a fixed petrophysical link between resistivity and velocity. The study shows that magnetotelluric data are more affected by model trade-offs, whereas Rayleigh wave dispersion is more sensitive in data space.</span>
            </summary>
            <content type="html">
                &lt;b&gt;Structural joint modeling of magnetotelluric data and Rayleigh wave dispersion curves using Pareto-based particle swarm optimization: an example to delineate  the crustal structure of the southeastern part  of the Biga Peninsula in western Anatolia&lt;/b&gt;&lt;br&gt;
                Ersin Büyük, Ekrem Zor, and Mustafa Cengiz Tapırdamaz&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 267&#8211;302, https://doi.org/10.5194/npg-33-267-2026, 2026&lt;br&gt;
                <p>It is widely acknowledged that the joint inversion of magnetotelluric and seismological datasets enhances the quality of the crustal structure solution, even when the physical correlation between electrical resistivity and seismic velocity is weak or indirect. The structurally coupled joint inversion approach has received considerable attention over the past two decades for its ability to estimate such parameters by penalizing their cross-gradient vectors at similar spatial positions. Despite this interest, various structural couplings and different physical directions (incremental or decremental) have been partially overlooked. We hereby propose an approach for the joint inversion of magnetotelluric&amp;#160;(MT) and Rayleigh wave dispersion&amp;#160;(RWD) data to estimate uncorrelated parameters by integrating particle swarm optimization&amp;#160;(PSO) and the Pareto optimality approach. We used the optimality framework of these methods to overcome the difficulties associated with traditional joint inversion algorithms and to obtain optimal solutions that account for both similar and contrasting physical sensitivities. The significant correlation between the inverted and synthetic models under both noise-free and noisy datasets, together with the consistent results obtained from comparison with a traditional derivative-based joint inversion algorithm, further strengthened our confidence in applying the proposed modeling approach to the field data from the southeastern Biga Peninsula, western Anatolia. The models inverted from the field data corroborate the efficacy of the presented method. A notable characteristic of the proposed methodology is its capacity to estimate uncorrelated physical parameters, such as electrical resistivity and seismic velocity, without the imposition of penalties. Therefore, the presented method not only offers advantages in joint inversion but also allows modelers to observe and analyze model parameters having different sensitivities that may indicate different physical directions.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-02T15:13:02+02:00</published>
            <updated>2026-06-02T15:13:02+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-33-233-2026</id>
            <title type="html">Boosting ensembles for statistics of tails at  conditionally optimal advance split times
            </title>
            <link href="https://doi.org/10.5194/npg-33-233-2026"/>
            <summary type="html">
                &lt;b&gt;Boosting ensembles for statistics of tails at  conditionally optimal advance split times&lt;/b&gt;&lt;br&gt;
                Justin Finkel and Paul A. O'Gorman&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 233&#8211;265, https://doi.org/10.5194/npg-33-233-2026, 2026&lt;br&gt;
                Estimating small probabilities of high-impact extreme weather events is a persistent computational challenge, motivating techniques such as <q>rare event sampling</q&gt; and <q>ensemble boosting</q>: lightly perturbing simulated moderate events into more extreme ones. We formulate a new, flexible sampling strategy and characterizes a critical parameter &amp;#8211; the <q>advance split time</q>, dictating when to perturb &amp;#8211; in a simple atmospheric turbulence model, with generalizable entropy-based criteria.
            </summary>
            <content type="html">
                &lt;b&gt;Boosting ensembles for statistics of tails at  conditionally optimal advance split times&lt;/b&gt;&lt;br&gt;
                Justin Finkel and Paul A. O'Gorman&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 233&#8211;265, https://doi.org/10.5194/npg-33-233-2026, 2026&lt;br&gt;
                <p>Climate science needs more efficient ways to study high-impact, low-probability extreme events, which are rare by definition and costly to simulate in large numbers. Rare event sampling&amp;#160;(RES), including ensemble boosting, offers a novel strategy to extract more information from those occasional simulated events, by applying small perturbations to turn a moderate event into a severe one which otherwise might not come for many more simulation-years. But how severe the events can become, and their estimated probabilities, depend sensitively on the details of the perturbation. In particular, for sudden and transient events like precipitation, performance of boosting depends sensitively on the choice of <i>advance split time</i>&amp;#160;(AST) of the perturbation. Heuristically, the perturbation must come early enough before the event to let the ensemble of simulations diversify, but not so early that they forget the special initial conditions that led to the extreme. In pursuit of guidelines for choosing the AST, we study the effect of AST in the task of sampling extreme fluctuations of a passive tracer in a quasigeostrophic turbulent channel flow. This model system is idealized, but captures key elements of midlatitude storm track dynamics while exposing similar algorithmic challenges. We formulate AST selection as a concrete optimization problem for statistical accuracy against a ground truth. Given that such a ground truth would not generally be available, we propose a proxy objective function to optimize in practice: <i>thresholded entropy</i>, which rewards ensembles with both a high mean and a large spread. We show that ensemble boosting, when given a well-chosen AST and equipped with methods to estimate probabilities, can accurately sample extremes at long return periods. We furthermore find evidence that thresholded entropy successfully identifies an optimal AST, which is roughly 1&amp;#8211;3 &amp;#160;ddy turnover timescales in the quasigeostrophic system. Moreover, this proxy captures the <i>variation</i&gt; of AST with the target location of the tracer within the flow field, suggesting it can generalize to more general chaotic systems including realistic climate models. Applying our boosting methodology at scale will require further development in adaptive optimization strategies, but our work here is an essential first step for establishing what must be optimized.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-28T15:13:02+02:00</published>
            <updated>2026-05-28T15:13:02+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-33-197-2026</id>
            <title type="html">Sandy beaches' chaos: shoreline-sandbar coupling inferred from observational time series
            </title>
            <link href="https://doi.org/10.5194/npg-33-197-2026"/>
            <summary type="html">
                &lt;b&gt;Sandy beaches' chaos: shoreline-sandbar coupling inferred from observational time series&lt;/b&gt;&lt;br&gt;
                Marius Aparicio, Sylvain Mangiarotti, Salomé Frugier, Laurent Lacaze, Marcan Graffin, and Rafael Almar&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 197&#8211;231, https://doi.org/10.5194/npg-33-197-2026, 2026&lt;br&gt;
                We studied how sandy beaches evolve by tracking the shoreline and offshore sandbars from satellites over many years. By rebuilding beach behavior directly from observations, we show that beaches follow organized but chaotic motion shaped by internal feedbacks. Beyond the seasonal rhythm imposed by waves, shorelines and sandbars exchange energy through the surf zone, producing repeated erosion and recovery cycles with limited predictability, explaining why beaches remain difficult to forecast.
            </summary>
            <content type="html">
                &lt;b&gt;Sandy beaches' chaos: shoreline-sandbar coupling inferred from observational time series&lt;/b&gt;&lt;br&gt;
                Marius Aparicio, Sylvain Mangiarotti, Salomé Frugier, Laurent Lacaze, Marcan Graffin, and Rafael Almar&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 197&#8211;231, https://doi.org/10.5194/npg-33-197-2026, 2026&lt;br&gt;
                <p>Sandy shoreline&amp;#8211;sandbar systems exhibit complex variability arising from the interplay between hydrodynamic forcing and intrinsic morphological feedbacks.  Using long-term satellite-derived shoreline and sandbar observations, we applied global polynomial modeling to reconstruct low-dimensional deterministic dynamics for 4&amp;#160;contrasting coastal sites.  The resulting autonomous models reproduce key morphodynamic features, including self-sustained shoreline oscillations, shoreline&amp;#8211;sandbar coupling, and intermittent transitions between quasi-stable configurations. Nonlinear stability analyses reveal that these systems behave as chaotic oscillators, characterized by locally divergent yet globally bounded trajectories.  Energetic episodes correspond to rapid shoreline&amp;#8211;sandbar exchanges, whereas long low-energy states reflect stable attractor confinement.  Together, these results demonstrate that sandy coasts are governed by deterministic but chaotic dynamics, in which internal coupling and self-organization control both variability and finite predictability.  The proposed framework offers a physically consistent and data-driven approach to characterize and compare coastal morphodynamics within a unified nonlinear dynamical perspective.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-04-21T15:13:02+02:00</published>
            <updated>2026-04-21T15:13:02+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-33-173-2026</id>
            <title type="html">Bayesian inference based on algorithms: MH, HMC, MALA and Lip-MALA for prestack seismic inversion
            </title>
            <link href="https://doi.org/10.5194/npg-33-173-2026"/>
            <summary type="html">
                &lt;b&gt;Bayesian inference based on algorithms: MH, HMC, MALA and Lip-MALA for prestack seismic inversion&lt;/b&gt;&lt;br&gt;
                Richard Perez-Roa, Saba Infante, Gabriel Barragan, and Raul Manzanilla&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 173&#8211;195, https://doi.org/10.5194/npg-33-173-2026, 2026&lt;br&gt;
                We explored four methods to improve how underground rock properties are estimated from seismic data. By comparing these methods on both simulated and real-world oilfield data, we found that techniques using gradient information give better accuracy but require more computing time. Our results help guide the choice of method depending on whether speed or precision is more important in subsurface exploration.
            </summary>
            <content type="html">
                &lt;b&gt;Bayesian inference based on algorithms: MH, HMC, MALA and Lip-MALA for prestack seismic inversion&lt;/b&gt;&lt;br&gt;
                Richard Perez-Roa, Saba Infante, Gabriel Barragan, and Raul Manzanilla&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 173&#8211;195, https://doi.org/10.5194/npg-33-173-2026, 2026&lt;br&gt;
                <p>Seismic inversion for estimating elastic properties is a key technique for reservoir characterization after drilling. The choice of inversion method strongly influences the accuracy, efficiency, and reliability of results. Bayesian inference based on Markov Chain Monte Carlo (MCMC) algorithms provides a robust framework for incorporating data uncertainty and prior geological knowledge. In this study, we compare the performance of four inversion methods &amp;#8211; Metropolis-Hastings (MH), Hamiltonian Monte Carlo (HMC), the Metropolis-Adjusted Langevin Algorithm (MALA), and its variant Lip-MALA &amp;#8211; in prestack seismic inversion using both synthetic models and real data from an eastern Venezuelan hydrocarbon reservoir. Results indicate that gradient-based methods (HMC, MALA, Lip-MALA) outperform MH in velocity estimation, while density inversion remains more challenging. MH and MALA achieve shorter execution times, whereas HMC and Lip-MALA improve accuracy at higher computational cost. This analysis evaluates mean values and standard deviation (SD) estimates for P-wave velocity, S-wave velocity, and density, with quality assessed through correlation metrics, objective function behavior, seismic traces, and Root Mean Square Error (RMSE). A two-dimensional inversion with real data further demonstrates algorithms performance under complex geological conditions. The findings highlight trade-offs between accuracy and efficiency, providing practical guidelines for selecting inversion method in seismic reservoir characterization.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-04-20T15:13:02+02:00</published>
            <updated>2026-04-20T15:13:02+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-33-157-2026</id>
            <title type="html">Spatiotemporal variation in rainfall predictability  in Serbia under a changing climate
            </title>
            <link href="https://doi.org/10.5194/npg-33-157-2026"/>
            <summary type="html">
                &lt;b&gt;Spatiotemporal variation in rainfall predictability  in Serbia under a changing climate&lt;/b&gt;&lt;br&gt;
                Tatijana Stosic, Ivana Tošić, Antonio Samuel Alves da Silva, Vladimir Djurdjević, and Borko Stosic&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 157&#8211;172, https://doi.org/10.5194/npg-33-157-2026, 2026&lt;br&gt;
                In this work we address the change in rainfall predictability in Serbia due to climate change, using a novel entropy-based method that highlights both small and large fluctuations. The study is performed on data from 14 stations from 1961&amp;#8211;2020. While rainfall average remains rather stable between two subperiods, the predictability of large and small fluctuations has changed, suggesting that climate change has affected rainfall dynamics in ways not observable by standard statistical methods.
            </summary>
            <content type="html">
                &lt;b&gt;Spatiotemporal variation in rainfall predictability  in Serbia under a changing climate&lt;/b&gt;&lt;br&gt;
                Tatijana Stosic, Ivana Tošić, Antonio Samuel Alves da Silva, Vladimir Djurdjević, and Borko Stosic&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 157&#8211;172, https://doi.org/10.5194/npg-33-157-2026, 2026&lt;br&gt;
                <p>This study examines whether the predictability of precipitation dynamics in Serbia has been influenced by climate change. We apply Generalized Weighted Permutation Entropy&amp;#160;(GWPE) to evaluate the temporal structure of daily precipitation series using the parameter&amp;#160;<span class="inline-formula"><i>q</i></span>, which filters subsets of small (<span class="inline-formula"><i>q</i><0</span>) and large (<span class="inline-formula"><i>q</i>>0</span>) fluctuations. The analysis covers data from 14&amp;#160;weather stations between&amp;#160;1961 and&amp;#160;2020. Entropy values for <span class="inline-formula"><i>q</i>=0</span&gt; and <span class="inline-formula"><i>q</i>=2</span>, corresponding to Permutation Entropy and Weighted Permutation Entropy respectively, remained stable spatially and temporally. In contrast, GWPE values for <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M6" display="inline" overflow="scroll" dspmath="mathml"><mrow><mi>q</mi><mo>=</mo><mo>-</mo><mn mathvariant="normal">10</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="42pt" height="12pt" class="svg-formula" dspmath="mathimg" md5hash="3fcdc37d4596c2da325db65fa78e9ebf"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="npg-33-157-2026-ie00001.svg" width="42pt" height="12pt" src="npg-33-157-2026-ie00001.png"/></svg:svg></span></span&gt; and <span class="inline-formula"><i>q</i>=10</span>, representing the predictability of small and large fluctuations, exhibited significant spatial and temporal variation between two 30-year subperiods. Entropy values for <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M8" display="inline" overflow="scroll" dspmath="mathml"><mrow><mi>q</mi><mo>=</mo><mo>-</mo><mn mathvariant="normal">10</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="42pt" height="12pt" class="svg-formula" dspmath="mathimg" md5hash="355870bc7c868af8cb11cc1129272890"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="npg-33-157-2026-ie00002.svg" width="42pt" height="12pt" src="npg-33-157-2026-ie00002.png"/></svg:svg></span></span&gt; were consistently lower, indicating that small precipitation fluctuations are more predictable than large ones. In several locations, significant changes in entropy occurred despite relatively stable annual precipitation amounts. In others, annual totals varied while entropy remained constant. These findings suggest that climate change has influenced the predictability of precipitation in Serbia. By filtering fluctuations across scales, GWPE effectively reveals underlying changes that may be masked by standard statistical measures.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-03-24T15:13:02+01:00</published>
            <updated>2026-03-24T15:13:02+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-33-123-2026</id>
            <title type="html">Beyond static forecasts: a dynamic stress gradient framework for high-resolution aftershock prediction and mitigation
            </title>
            <link href="https://doi.org/10.5194/npg-33-123-2026"/>
            <summary type="html">
                &lt;b&gt;Beyond static forecasts: a dynamic stress gradient framework for high-resolution aftershock prediction and mitigation&lt;/b&gt;&lt;br&gt;
                Boi-Yee Liao&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 123&#8211;155, https://doi.org/10.5194/npg-33-123-2026, 2026&lt;br&gt;
                After major earthquakes, smaller shocks often follow, yet predicting where they will occur remains difficult. This study introduces a new method for tracking changes in underground stress after a large earthquake. Using the 2018 Hualien earthquake in Taiwan as a case study, we found that areas with strong stress differences provide clearer signals of future aftershocks than stress magnitude alone. This approach can improve short-term earthquake risk assessment and disaster response planning.
            </summary>
            <content type="html">
                &lt;b&gt;Beyond static forecasts: a dynamic stress gradient framework for high-resolution aftershock prediction and mitigation&lt;/b&gt;&lt;br&gt;
                Boi-Yee Liao&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 123&#8211;155, https://doi.org/10.5194/npg-33-123-2026, 2026&lt;br&gt;
                <p>Accurate forecasting of aftershock distributions is vital for effective post-earthquake emergency response, early warning systems, and long-term seismic hazard mitigation. This study introduces a novel nonlinear, multiscale framework for modeling the evolution of Coulomb stress following a major earthquake. The proposed approach integrates rate-and-state friction laws, a KPP-type reaction&amp;#8211;diffusion equation, and the Banach fixed-point theorem to simulate the dynamic redistribution of stress in space and time. Central to the model are two time-dependent parameters &amp;#8211; <span class="inline-formula"><i>&amp;#945;</i>(<i>t</i>)</span>, which governs the decay of stress memory consistent with Omori's law, and <span class="inline-formula"><i>&amp;#946;</i>(<i>t</i>)</span>, which modulates the nonlinear diffusion and reaction dynamics. Applied to the 2018 Hualien earthquake in Taiwan, the framework resolves stress changes and their gradients at depths of 6&amp;#8211;25&amp;#8201;km. Results indicate that stress gradients are more predictive of aftershock occurrences within the first 50&amp;#8201;d and at depths shallower than 12&amp;#8201;km, while stress changes play a dominant role at greater depths and later times. Validation using AUC and Molchan error metrics demonstrates the model's strong spatial forecasting capability. The framework's adaptive convergence and modular structure support real-time seismic hazard assessment and integration into PSHA workflows, offering a promising tool for aftershock modeling and disaster resilience planning.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-03-19T15:13:02+01:00</published>
            <updated>2026-03-19T15:13:02+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-33-103-2026</id>
            <title type="html">Inferring the role of Interdecadal Pacific Oscillation phase on tropical-extratropical teleconnection dependencies
            </title>
            <link href="https://doi.org/10.5194/npg-33-103-2026"/>
            <summary type="html">
                &lt;b&gt;Inferring the role of Interdecadal Pacific Oscillation phase on tropical-extratropical teleconnection dependencies&lt;/b&gt;&lt;br&gt;
                Mark A. Collier, Dylan Harries, and Terence J. O'Kane&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 103&#8211;122, https://doi.org/10.5194/npg-33-103-2026, 2026&lt;br&gt;
                Here we apply Bayesian methods to reconstructed and simulated climate model data over past decades to determine the role of long timescale phase dependencies, and extratropical teleconnections, on the major drivers of tropical climate variability.
            </summary>
            <content type="html">
                &lt;b&gt;Inferring the role of Interdecadal Pacific Oscillation phase on tropical-extratropical teleconnection dependencies&lt;/b&gt;&lt;br&gt;
                Mark A. Collier, Dylan Harries, and Terence J. O'Kane&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 103&#8211;122, https://doi.org/10.5194/npg-33-103-2026, 2026&lt;br&gt;
                <p>Regime dependencies and Granger causal relationships between tropical and extratropical teleconnections are inferred using Bayesian structure learning. Using ERA5 data, an examination of the differences between the learned graphical structures during particular phases of the Interdecadal Pacific Oscillation (IPO) are used to infer the role of the background state on interactions between the major climate teleconnections. These relationships present a clear regime dependency on the phase of IPO. In the positive phase, IPO autocorrelations are weak whereas Indian Ocean Dipole (IOD) and El Ni&amp;#241;o Southern Oscillation (ENSO) autocorrelations and the influence of the Madden Julian Oscillation (MJO) are indicative of an enhanced Walker circulation. In contrast, during the negative phase, IPO autocorrelations are strongest with evidence of an enhanced role for extratropical teleconnections on the tropics. Exclusion of MJO removes important tropical-extratropical influences while increasing posterior edge weights between ENSO, the IPO and IOD. Our analysis reveals the dependence of the ENSO autocorrelation on the phase of the background IPO state, and the role of the MJO as being key to link the extratropical tropospheric modes Pacific North American and North Atlantic Oscillation (PNA, NAO) and equatorial surface ocean temperatures (IOD, ENSO) and as a consequence convection.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-03-04T15:13:02+01:00</published>
            <updated>2026-03-04T15:13:02+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-33-73-2026</id>
            <title type="html">MESMER-RCM: a probabilistic climate emulator for regional warming projections
            </title>
            <link href="https://doi.org/10.5194/npg-33-73-2026"/>
            <summary type="html">
                &lt;b&gt;MESMER-RCM: a probabilistic climate emulator for regional warming projections&lt;/b&gt;&lt;br&gt;
                Hao Pan, Lukas Gudmundsson, Mathias Hauser, Jonas Schwaab, Yann Quilcaille, and Sonia I. Seneviratne&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 73&#8211;83, https://doi.org/10.5194/npg-33-73-2026, 2026&lt;br&gt;
                Existing regional climate model (RCM) emulators mainly provide deterministic emulations, while internal RCM variability is typically not represented. We develop MESMER-RCM, a probabilistic RCM emulator for annual 2-m temperature, using a simple and physically interpretable approach. We demonstrate its ability to emulate both RCM trends and internal variability in a high-dimensional spatial setting, where existing approaches typically struggle.
            </summary>
            <content type="html">
                &lt;b&gt;MESMER-RCM: a probabilistic climate emulator for regional warming projections&lt;/b&gt;&lt;br&gt;
                Hao Pan, Lukas Gudmundsson, Mathias Hauser, Jonas Schwaab, Yann Quilcaille, and Sonia I. Seneviratne&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 73&#8211;83, https://doi.org/10.5194/npg-33-73-2026, 2026&lt;br&gt;
                <p>Regional Climate Model (RCM) emulators enable rapid and computationally efficient RCM projections given Global Climate Model (GCM) inputs, complementing dynamical downscaling by approximating physical representations with statistical models. However, while existing RCM emulators perform well in deterministic emulations, they do not sample internal RCM variability and remain computationally expensive. Here, we present MESMER-RCM, a probabilistic RCM emulator designed for spatially resolved annual 2&amp;#8201;m temperature. MESMER-RCM is a generative model that enables both data-efficient learning and interpretability. It can generate large ensembles of synthetic, yet physically plausible, RCM realizations, capturing the internal RCM variability at a fraction of the computational cost. This work offers a fast and reliable RCM emulation framework, supporting finer-scale what-if analyses of regional climate responses and informing local adaptation and mitigation strategies.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-02-12T15:13:02+01:00</published>
            <updated>2026-02-12T15:13:02+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-33-85-2026</id>
            <title type="html">Dynamic mode decomposition of extreme events
            </title>
            <link href="https://doi.org/10.5194/npg-33-85-2026"/>
            <summary type="html">
                &lt;b&gt;Dynamic mode decomposition of extreme events&lt;/b&gt;&lt;br&gt;
                Maša Ann, Jörn Behrens, and Jana Sillmann&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 85&#8211;102, https://doi.org/10.5194/npg-33-85-2026, 2026&lt;br&gt;
                We present a new framework based on Dynamic Mode Decomposition (DMD) to better detect outliers and model extremes. Unlike standard DMD, which focuses on average system behaviour, our approach targets rare, exceptional dynamics. Applied to climate data, it improves extreme event approximation and reveals meaningful spatiotemporal patterns. The method may generalise to other types of extremes.
            </summary>
            <content type="html">
                &lt;b&gt;Dynamic mode decomposition of extreme events&lt;/b&gt;&lt;br&gt;
                Maša Ann, Jörn Behrens, and Jana Sillmann&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 85&#8211;102, https://doi.org/10.5194/npg-33-85-2026, 2026&lt;br&gt;
                <p>Most data-driven methods, among them Dynamic Mode Decomposition (DMD), focus on analysing and reconstructing the average behaviour of a system. However, the primary interest often lies in the anomalous behaviour, known as extreme events. This is especially the case in climate research, where extreme events have significant economic and societal costs. Therefore, we extend a DMD method to account for extreme events by adding a penalisation term. This extension allows us to not only better reconstruct the extreme events, but also extract the spatiotemporal structures related to those extreme events. DMD was originally developed by Schmid and Sesterhenn <span class="cit" id="xref_paren.1">(<a href="#bib1.bibx32">Schmid and Sesterhenn</a>,&amp;#160;<a href="#bib1.bibx32">2008</a>)</span&gt; to enable the fluid dynamics community to identify spatiotemporal coherent structures (called <i>modes</i>) from high-dimensional data. In its essence DMD uses most relevant modes to filter the noise and reconstruct the original signal. We ask &amp;#8220;Is the noise really noise&amp;#8221;! Or can we attribute some of these dynamic modes, that result from the DMD, to extreme events? We applied this new method to the climate system, well known for its high-dimensionality. As a proof of concept, we applied the method to two well-studied European heatwaves: those of 2003 and 2010. Across both cases, our <i>extreme</i&gt; DMD improves reconstruction accuracy at extreme spatiotemporal points, achieving a 0.45&amp;#8201;<span class="inline-formula">%</span>&amp;#8211;0.85&amp;#8201;<span class="inline-formula">%</span&gt; relative reduction in error compared with standard DMD, a difference that is small in magnitude but statistically significant. The approach also reveals coherent spatial modes that contribute specifically to the development of heat extremes. This framework represents a general extension of DMD and can be applied to other high-dimensional dynamical systems where extreme events are of interest.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-02-12T15:13:02+01:00</published>
            <updated>2026-02-12T15:13:02+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-33-51-2026</id>
            <title type="html">On transversality and the characterization of finite  time hyperbolic subspaces in chaotic attractors
            </title>
            <link href="https://doi.org/10.5194/npg-33-51-2026"/>
            <summary type="html">
                &lt;b&gt;On transversality and the characterization of finite  time hyperbolic subspaces in chaotic attractors&lt;/b&gt;&lt;br&gt;
                Terence J. O'Kane and Courtney R. Quinn&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 51&#8211;72, https://doi.org/10.5194/npg-33-51-2026, 2026&lt;br&gt;
                Mathematical concepts and measures from dynamical systems theory are applied to identify commonalities across a diverse set of chaotic attractors to better understand the relationship between predictability, directions and rates of expansion and contraction of instabilities over finite time forecast horizons, and dimensionality. The patterns that emerge have broad implications for understanding many dynamical features of geophysical flows.
            </summary>
            <content type="html">
                &lt;b&gt;On transversality and the characterization of finite  time hyperbolic subspaces in chaotic attractors&lt;/b&gt;&lt;br&gt;
                Terence J. O'Kane and Courtney R. Quinn&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 51&#8211;72, https://doi.org/10.5194/npg-33-51-2026, 2026&lt;br&gt;
                <p>We examine the local stable and unstable manifolds of chaotic attractors and their associated growth rates for the quantification of (non-)hyperbolicity in low dimensional nonlinear autonomous dissipative models. This is motivated by a desire for a deeper understanding of transversality and hyperbolicity to inform key challenges to prediction in spatially extended chaotic systems in geophysical flows. In particular, we apply local measures of chaos to quantify the relationship between transversality, dimension, and hyperbolicity on the subspaces of the attractors' invariant manifolds. We consider unstable directions and growth rates determined over finite time intervals, specifically those predicated on information over the past evolution i.e., finite time backwards Lyapunov vectors, and those that include information from both the past and future i.e., finite time covariant Lyapunov vectors. Our study reveals general properties across a diverse set of chaotic attractors at short, intermediate and extended forecast horizons associated with the emergence of distinct locally evolving regions of instability.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-02-11T15:13:02+01:00</published>
            <updated>2026-02-11T15:13:02+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-33-33-2026</id>
            <title type="html">Localization in the mapping particle filter
            </title>
            <link href="https://doi.org/10.5194/npg-33-33-2026"/>
            <summary type="html">
                &lt;b&gt;Localization in the mapping particle filter&lt;/b&gt;&lt;br&gt;
                Juan M. Guerrieri, Manuel Pulido, Takemasa Miyoshi, Arata Amemiya, and Juan J. Ruiz&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 33&#8211;49, https://doi.org/10.5194/npg-33-33-2026, 2026&lt;br&gt;
                <p align="left">This work extends the Mapping Particle Filter to account for local dependencies. Two localization methods are tested: a global particle flow with local kernels, and iterative local mappings based on correlation radius. Using a two-scale Lorenz-96 truth and a one-scale forecast model, experiments with full/partial and linear/nonlinear observations show Root Mean Square Error reductions using localized Gaussian mixture priors, achieving competitive performance against Gaussian filters.
            </summary>
            <content type="html">
                &lt;b&gt;Localization in the mapping particle filter&lt;/b&gt;&lt;br&gt;
                Juan M. Guerrieri, Manuel Pulido, Takemasa Miyoshi, Arata Amemiya, and Juan J. Ruiz&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 33&#8211;49, https://doi.org/10.5194/npg-33-33-2026, 2026&lt;br&gt;
                <p>Data assimilation involves sequential inference in  geophysical systems with nonlinear dynamics and observational operators. Non-parametric filters are a promising approach for data assimilation because they are able to represent non-Gaussian densities. The mapping particle filter is an iterative ensemble method that incorporates the Stein Variational Gradient Descent (SVGD) to produce a particle flow transforming state vectors from prior to posterior densities. At every pseudo-time step, the Kullback-Leibler divergence between the intermediate density and the target posterior is evaluated and minimized. However, for applications in geophysical systems, challenges persist in high dimensions, where sample covariance underestimation leads to filter divergence. This work proposes two localization methods, one in which a local kernel function is defined and the particle flow is global. The second method, given a localization radius, physically partitions the state vector and performs local mappings at each grid point. The performance of the proposed Local Mapping Particle Filters (LMPFs) is assessed in synthetic experiments. Observations are produced with a two-scale Lorenz system, while a one-scale Lorenz model is used as surrogate, introducing model error in the inference. The methods are evaluated with both full and partial observations, as well as with different linear and non-linear observational operators. The LMPFs with Gaussian mixtures in the prior density perform similarly to Gaussian filters such as the Ensemble Transform Kalman Filter (ETKF) and the Local Ensemble Transform Kalman Filter (LETKF) in most cases, and in some scenarios, they provide competitive performance in terms of analysis accuracy.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-01-26T15:13:02+01:00</published>
            <updated>2026-01-26T15:13:02+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-33-17-2026</id>
            <title type="html">Exploring urban heat islands with  a simple thermodynamic model
            </title>
            <link href="https://doi.org/10.5194/npg-33-17-2026"/>
            <summary type="html">
                &lt;b&gt;Exploring urban heat islands with  a simple thermodynamic model&lt;/b&gt;&lt;br&gt;
                Mijeong Jeon, Kyeongjoo Park, Woosok Moon, Jae-Jin Kim, and Jong-Jin Baik&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 17&#8211;32, https://doi.org/10.5194/npg-33-17-2026, 2026&lt;br&gt;
                Using a simple day-night thermodynamic model based on surface energy balance, this study explains key mechanisms of the urban heat island (UHI): reduced diurnal temperature range (DTR) due to high heat capacity and increased mean temperature from low albedo. The model captures the stronger nighttime UHI and reproduces observed patterns, showing its value in understanding UHI dynamics and urban effects.
            </summary>
            <content type="html">
                &lt;b&gt;Exploring urban heat islands with  a simple thermodynamic model&lt;/b&gt;&lt;br&gt;
                Mijeong Jeon, Kyeongjoo Park, Woosok Moon, Jae-Jin Kim, and Jong-Jin Baik&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 17&#8211;32, https://doi.org/10.5194/npg-33-17-2026, 2026&lt;br&gt;
                <p>The urban heat island (UHI), where urban areas experience higher near-surface temperatures than surrounding rural areas, has long been recognized as a serious issue in urban climatology due to global warming and rapid urbanization. This study investigates the key mechanisms of the UHI through a simple theoretical thermodynamic model. Using a simple day-night model based on the surface energy balance (SEB), we demonstrate that the UHI primarily results from two mechanisms: reduced diurnal temperature range (DTR) due to larger heat capacity of urban materials and increased mean temperature due to lower urban albedo. These mechanisms explain why the UHI intensity is stronger at night than during the day. The UHI intensity obtained from the theoretical model shows a qualitatively similar diurnal variation to that found in observations, supporting the applicability of the theoretical model for understanding the UHI. An analysis of temporal dynamics of UHIs in a megacity (Seoul) and a major city (Suwon) in South Korea shows that the long-term changes in the UHI in both cities are significantly correlated with those in the urban-rural difference in DTR, highlighting the role of urban heat storage in the UHI. In particular, this study emphasizes that well-known UHI mechanisms can be explained in a simple and intuitive manner through a time-integrated theoretical framework, underscoring the academic value of simplified models in interpreting complex urban climate processes. Moreover, this approach demonstrates broader applicability beyond UHI research, suggesting that such models can serve as practical tools in diverse climatic and environmental contexts.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-01-06T15:13:02+01:00</published>
            <updated>2026-01-06T15:13:02+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-33-1-2026</id>
            <title type="html">Impact of reduced non-Gaussianity on analysis and forecast accuracy by assimilating every-30&#8201;s radar observation with ensemble Kalman filter: idealized experiments of deep convection
            </title>
            <link href="https://doi.org/10.5194/npg-33-1-2026"/>
            <summary type="html">
                &lt;b&gt;Impact of reduced non-Gaussianity on analysis and forecast accuracy by assimilating every-30 s radar observation with ensemble Kalman filter: idealized experiments of deep convection&lt;/b&gt;&lt;br&gt;
                Arata Amemiya and Takemasa Miyoshi&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 1&#8211;16, https://doi.org/10.5194/npg-33-1-2026, 2026&lt;br&gt;
                The accurate estimation of atmospheric state variables from radar observation in rapidly growing deep convection, which causes heavy thunderstorms, is a major challenge. This study examines the advantage of incorporating radar observation data with very high frequency such as 30 s compared with the conventional case of 5 min, from a theoretical perspective.
            </summary>
            <content type="html">
                &lt;b&gt;Impact of reduced non-Gaussianity on analysis and forecast accuracy by assimilating every-30 s radar observation with ensemble Kalman filter: idealized experiments of deep convection&lt;/b&gt;&lt;br&gt;
                Arata Amemiya and Takemasa Miyoshi&lt;br&gt;
                    Nonlin. Processes Geophys., 33, 1&#8211;16, https://doi.org/10.5194/npg-33-1-2026, 2026&lt;br&gt;
                <p>This study investigates the impact of very high frequency data assimilation on analysis and forecast accuracy with the local ensemble transform Kalman filter for idealized deep convection. Previous studies showed that assimilating every 30&amp;#8201;s data from Phased Array Weather Radar (PAWR) alleviates the problem of strongly non-Gaussian error probability distribution due to rapid nonlinear evolution of deep convection in real-world cases. This study performs perfect model observing system simulation experiments to understand better the impact of assimilating radar reflectivity every 30&amp;#8201;s focusing on non-Gaussianity. The idealized experimental settings have unique advantage in verifications for unobserved variables since it was unclear in the previous studies with real-world data. The results show that every 30&amp;#8201;s data assimilation contributes to a significant improvement of the analysis accuracy, particularly for vertical velocity associated with strong convection, although the impact on the forecast accuracy is limited. We also find a significant reduction in the non-Gaussianity of first guess ensemble. The impact of assimilation frequency on reducing non-Gaussianity is enhanced when the uncertainty in background wind or stability is included in the initial ensemble perturbation.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-01-05T15:13:02+01:00</published>
            <updated>2026-01-05T15:13:02+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-32-489-2025</id>
            <title type="html">Nonlinear wavefield characteristics of seismic  translation and rotation in small-strain deformation  from moment tensor simulations
            </title>
            <link href="https://doi.org/10.5194/npg-32-489-2025"/>
            <summary type="html">
                &lt;b&gt;Nonlinear wavefield characteristics of seismic  translation and rotation in small-strain deformation  from moment tensor simulations&lt;/b&gt;&lt;br&gt;
                Wei Li, Yun Wang, Chang Chen, and Lixia Sun&lt;br&gt;
                    Nonlin. Processes Geophys., 32, 489&#8211;501, https://doi.org/10.5194/npg-32-489-2025, 2025&lt;br&gt;
                <span class="ng-star-inserted"><span class="ng-star-inserted">This study uses numerical simulations to investigate geometric nonlinearity in six-component seismic motions. Our results reveal the characteristic of these nonlinear effects: while their pattern in body waves is universal, their excitation efficiency shows a strong source-type dependency. It demonstrates that rotational components are highly sensitive to effects driven by S-waves, and that surface waves may be the primary carriers of these features.</span></span>
            </summary>
            <content type="html">
                &lt;b&gt;Nonlinear wavefield characteristics of seismic  translation and rotation in small-strain deformation  from moment tensor simulations&lt;/b&gt;&lt;br&gt;
                Wei Li, Yun Wang, Chang Chen, and Lixia Sun&lt;br&gt;
                    Nonlin. Processes Geophys., 32, 489&#8211;501, https://doi.org/10.5194/npg-32-489-2025, 2025&lt;br&gt;
                <p>Seismic rotational motions recorded in near-field and strong-motion observations show discrepancies with theoretical predictions derived from linear elastodynamic theory. To investigate potential nonlinear contributions, this study incorporates geometric nonlinear effects into wave propagation theory using the Green&amp;#8211;Lagrange strain tensor. A staggered-grid finite-difference method is used to simulate six-component (translational and rotational) wavefields generated by three basic moment-tensor source types: isotropic&amp;#160;(ISO), double-couple&amp;#160;(DC), and compensated linear vector dipole&amp;#160;(CLVD). The results demonstrate that nonlinear effects, as a secondary source, have a universal intensity pattern adhering to the physics of wave motion. However, the efficiency of exciting these effects and the modulation of wavefield attributes (such as P-wave polarization) depend strongly on source type. Simulations show that rotational components exhibit higher sensitivity to nonlinear effects driven by S-waves. Reference simulations of two moderate-to-strong earthquakes suggest that surface waves are the primary carriers of nonlinear features.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2025-12-05T15:13:02+01:00</published>
            <updated>2025-12-05T15:13:02+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-32-471-2025</id>
            <title type="html">On process-oriented conditional targeted covariance inflation (TCI) for 3D-volume radar data assimilation
            </title>
            <link href="https://doi.org/10.5194/npg-32-471-2025"/>
            <summary type="html">
                &lt;b&gt;On process-oriented conditional targeted covariance inflation (TCI) for 3D-volume radar data assimilation&lt;/b&gt;&lt;br&gt;
                Klaus Vobig, Roland Potthast, and Klaus Stephan&lt;br&gt;
                    Nonlin. Processes Geophys., 32, 471&#8211;488, https://doi.org/10.5194/npg-32-471-2025, 2025&lt;br&gt;
                We present a novel approach to targeted covariance inflation (TCI) which aims to improve the assimilation of 3D radar reflectivity and, possibly, short-term forecasts of reflectivity and precipitation. Using an operational numerical weather prediction framework, our numerical results show that TCI makes the system accurately generate new reflectivity cells and significantly improves the fractional skill score of forecasts over lead times of up to 6 h by up to 10 %.
            </summary>
            <content type="html">
                &lt;b&gt;On process-oriented conditional targeted covariance inflation (TCI) for 3D-volume radar data assimilation&lt;/b&gt;&lt;br&gt;
                Klaus Vobig, Roland Potthast, and Klaus Stephan&lt;br&gt;
                    Nonlin. Processes Geophys., 32, 471&#8211;488, https://doi.org/10.5194/npg-32-471-2025, 2025&lt;br&gt;
                <p>This paper addresses a major challenge in assimilating 3D radar reflectivity data with a localized ensemble transform Kalman filter (LETKF). In the case of observations with significant reflectivity and small or zero corresponding simulated reflectivities for all ensemble members, i.e., when the ensemble spread is vanishing, the filter ignores the observations based on its low-variance estimate for the background uncertainty. For such low-variance cases, the LETKF is insensitive to observations and their contribution to the analysis increment is effectively zero. Targeted covariance inflation (TCI) has been suggested to deal with the ensemble spread deficiency <span class="cit" id="xref_paren.1">(<a href="#bib1.bibx52">Yokota et&amp;#160;al.</a>,&amp;#160;<a href="#bib1.bibx52">2018</a>; <a href="#bib1.bibx10">Dowell and Wicker</a>,&amp;#160;<a href="#bib1.bibx10">2009</a>; <a href="#bib1.bibx50">Vobig et&amp;#160;al.</a>,&amp;#160;<a href="#bib1.bibx50">2021</a>)</span>. To actually make TCI work in a fully cycled convective-scale data assimilation framework, here we will introduce a <i>process-oriented approach</i&gt; to the TCI in combination with a <i>conditional approach</i&gt; formulating <i>criteria</i&gt; under which targeted covariance inflation is efficient.</p&gt;        <p>The <i>process-oriented conditional</i&gt; TCI addresses the challenge of underrepresented reflectivity in the prior by constructing artificially simulated reflectivities for each ensemble member based on current observations and typical convective processes. Furthermore, certain conditions are used to restrict this spread inflation process to a carefully selected minimal set of eligible observations, reducing the noise introduced into the system.</p&gt;        <p>We will describe the theoretical basis of the new TCI approach. Furthermore, we will present numerical results of a case study in an operational framework, for which the TCI is applied to radar observations at each hourly assimilation step throughout a data assimilation cycle. We are able to demonstrate that the TCI is able to clearly improve the assimilation of radar reflectivities, making the system dynamically generate reflectivity that would otherwise be missing. Related to this, we are able to show that the fractional skill score of radar reflectivity forecasts over lead times of up to 6&amp;#8201;h is significantly improved by up to 10&amp;#8201;%. All of the results are based on the German radar network and the ICON-D2 model covering central Europe.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2025-11-24T15:13:02+01:00</published>
            <updated>2025-11-24T15:13:02+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-32-457-2025</id>
            <title type="html"> Bottom&#8211;up approach for mitigating extreme events with limited intervention options: a case study with Lorenz 96 model
            </title>
            <link href="https://doi.org/10.5194/npg-32-457-2025"/>
            <summary type="html">
                &lt;b&gt; Bottom–up approach for mitigating extreme events with limited intervention options: a case study with Lorenz 96 model&lt;/b&gt;&lt;br&gt;
                Takahito Mitsui, Shunji Kotsuki, Naoya Fujiwara, Atsushi Okazaki, and Keita Tokuda&lt;br&gt;
                    Nonlin. Processes Geophys., 32, 457&#8211;469, https://doi.org/10.5194/npg-32-457-2025, 2025&lt;br&gt;
                Extreme weather poses serious risks, making prevention crucial. Using the Lorenz 96 model as a testbed, we propose a bottom-up approach to mitigate extreme events via local interventions guided by multi-scenario ensemble forecasts. Unlike control-theoretic methods, our approach selects the best control scenario from available options. It achieves a high success rate of 99.4% while maintaining reasonable costs, offering a practical strategy to reduce extremes under limited control.
            </summary>
            <content type="html">
                &lt;b&gt; Bottom–up approach for mitigating extreme events with limited intervention options: a case study with Lorenz 96 model&lt;/b&gt;&lt;br&gt;
                Takahito Mitsui, Shunji Kotsuki, Naoya Fujiwara, Atsushi Okazaki, and Keita Tokuda&lt;br&gt;
                    Nonlin. Processes Geophys., 32, 457&#8211;469, https://doi.org/10.5194/npg-32-457-2025, 2025&lt;br&gt;
                <p>Prediction and mitigation of extreme weather events are important scientific and societal challenges. Recently, Miyoshi and Sun (2022) proposed a control simulation experiment framework that assesses the controllability of chaotic systems under observational uncertainty, and within this framework, Sun et al.&amp;#160;(2023) developed a method to prevent extreme events in the Lorenz 96 model. However, since their method is primarily designed to apply control inputs to all grid variables, the success rate decreases to approximately 60&amp;#8201;% when applied to a single site, at least in a specific setting. Herein, we propose an approach that mitigates extreme events by updating local interventions based on multi-scenario ensemble forecasts. Our method achieves a high success rate, reaching 94&amp;#8201;% even when applying interventions at one site per step, albeit with a moderate increase in the intervention cost. Furthermore, the success rate increases to 99.4&amp;#8201;% for interventions at two sites. Unlike control-theoretic approaches adopting a top&amp;#8211;down strategy, which determine inputs by optimizing cost functions, our bottom&amp;#8211;up approach mitigates extreme events by effectively utilizing limited intervention options.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2025-11-04T15:13:02+01:00</published>
            <updated>2025-11-04T15:13:02+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-32-439-2025</id>
            <title type="html">Exploring the influence of spatio-temporal scale differences in coupled data assimilation
            </title>
            <link href="https://doi.org/10.5194/npg-32-439-2025"/>
            <summary type="html">
                &lt;b&gt;Exploring the influence of spatio-temporal scale differences in coupled data assimilation&lt;/b&gt;&lt;br&gt;
                Lilian Garcia-Oliva, Alberto Carrassi, and François Counillon&lt;br&gt;
                    Nonlin. Processes Geophys., 32, 439&#8211;456, https://doi.org/10.5194/npg-32-439-2025, 2025&lt;br&gt;
                We used a simple coupled model and a data assimilation method to find the correct initialisation for climate predictions. We aim to clarify when weakly or strongly coupled data assimilation (WCDA or SCDA) is best, depending on the system's dynamical characteristics (spatio-temporal) and data coverage. We found that WCDA is better in full data coverage. When we have a partially observed system, SCDA is better. This result depends on the temporal and spatial scale of the observed quantity.
            </summary>
            <content type="html">
                &lt;b&gt;Exploring the influence of spatio-temporal scale differences in coupled data assimilation&lt;/b&gt;&lt;br&gt;
                Lilian Garcia-Oliva, Alberto Carrassi, and François Counillon&lt;br&gt;
                    Nonlin. Processes Geophys., 32, 439&#8211;456, https://doi.org/10.5194/npg-32-439-2025, 2025&lt;br&gt;
                <p>Identifying the optimal strategy for initializing coupled climate prediction systems is challenging due to the spatio-temporal scale separation and disparities in the observational network. We aim to clarify when strongly coupled data assimilation (SCDA) is preferable to weakly coupled data assimilation (WCDA). We use a two-components coupled Lorenz-63 system, mimicking the atmosphere and the ocean, and the Ensemble Kalman Filter (EnKF) to compare WCDA and SCDA for diverse spatio-temporal scale separations and observational networks &amp;#8211; only in the atmosphere, the ocean, or both components. In the fully observed scenario, SCDA and WCDA yield similar performances. However, little differences are present, and we conjecture these are due to the SCDA being more sensitive to the approximations at the basis of the EnKF present in the cross-update &amp;#8211; linear analysis update and sampling error, and how they impact the cross-update between ocean and atmosphere. This sensitivity increases as the temporal scale separation increases and is stronger on the slow and large-scale components. When observations are only in one of the components, the spatio-temporal scale separation influences SCDA's performance. In this scenario, the largest improvements are found when the observed component has a smaller spatial scale. The fast-to-slow update has a larger benefit with a larger temporal scale separation. Meanwhile, with the slow-to-fast update, the improvement is limited to instances when the temporal scale separation is less than one-half. This suggests that SCDA of fast atmospheric observations can potentially improve the large and slow ocean component. Conversely, observations of the fine ocean can improve the large atmosphere at a comparable temporal scale. However, when both components are highly chaotic, and the observed component's spatial scale is the largest, SCDA does not improve over WCDA. In such a case, the cross-updates may become too sensitive to data assimilation approximations. We further validated that WCDA systematically outperforms uncoupled data assimilation (UCDA) in both components, legitimizing the transition toward WCDA.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2025-10-24T15:13:02+02:00</published>
            <updated>2025-10-24T15:13:02+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-32-411-2025</id>
            <title type="html">Quantifying variability in Lagrangian particle dispersal in ocean ensemble simulations: an information  theory approach
            </title>
            <link href="https://doi.org/10.5194/npg-32-411-2025"/>
            <summary type="html">
                &lt;b&gt;Quantifying variability in Lagrangian particle dispersal in ocean ensemble simulations: an information  theory approach&lt;/b&gt;&lt;br&gt;
                Claudio M. Pierard, Siren Rühs, Laura Gómez-Navarro, Michael Charles Denes, Florian Meirer, Thierry Penduff, and Erik van Sebille&lt;br&gt;
                    Nonlin. Processes Geophys., 32, 411&#8211;438, https://doi.org/10.5194/npg-32-411-2025, 2025&lt;br&gt;
                Particle-tracking simulations compute how ocean currents transport material. However, initializing these simulations is often ad hoc. Here, we explore how two different strategies (releasing particles over space or over time) compare. Specifically, we compare the variability in particle trajectories to the variability of particles computed in a 50-member ensemble simulation. We find that releasing the particles over 20 weeks gives variability that is most like that in the ensemble.
            </summary>
            <content type="html">
                &lt;b&gt;Quantifying variability in Lagrangian particle dispersal in ocean ensemble simulations: an information  theory approach&lt;/b&gt;&lt;br&gt;
                Claudio M. Pierard, Siren Rühs, Laura Gómez-Navarro, Michael Charles Denes, Florian Meirer, Thierry Penduff, and Erik van Sebille&lt;br&gt;
                    Nonlin. Processes Geophys., 32, 411&#8211;438, https://doi.org/10.5194/npg-32-411-2025, 2025&lt;br&gt;
                <p>Ensemble Lagrangian simulations aim to capture the full range of possible outcomes for particle dispersal. However, single-member Lagrangian simulations are most commonly available and only provide a subset of the possible particle dispersal outcomes. This study explores how to generate the variability inherent in Lagrangian ensemble simulations by creating variability in a single-member simulation. To obtain a reference for comparison, we performed ensemble Lagrangian simulations by advecting the particles from the surface of the Gulf Stream, around 35.61&amp;#176;&amp;#8201;N, 73.61&amp;#176;&amp;#8201;W, in each member to obtain trajectories capturing the variability of the full 50-member ensemble. Subsequently, we performed single-member simulations with spatially and temporally varying release strategies to generate comparable trajectory variability and dispersal and also with adding Brownian motion diffusion to the advection. We studied how these strategies affected the number of surface particles connecting the Gulf Stream with the eastern side of the subtropical gyre. We used an information theory approach to define and compare the variability in the ensemble with the single-member strategies. We defined the variability as the marginal entropy or average information content of the probability distributions of the position of the particles. We calculated the relative entropy to quantify the uncertainty of representing the full-ensemble variability with single-member simulations. We found that release periods of 12 to 20 weeks most effectively captured the full ensemble variability, while spatial releases with a 2.0&amp;#176; radius resulted in the closest match at timescales shorter than 10&amp;#8201;d. We found that adding relatively high amounts of Brownian motion diffusion (<span class="inline-formula"><i>K</i><sub><i>h</i></sub>=1000</span>&amp;#8201;<span class="inline-formula">m<sup>2</sup>&amp;#8201;s<sup>&amp;#8722;1</sup></span>) captures the entropy aspects of the full ensemble variability well but leads to an overestimation of connectivity. Our findings provide insights to improve the representation of variability in particle trajectories and define a framework for uncertainty quantification in Lagrangian ocean analysis.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2025-10-20T15:13:02+02:00</published>
            <updated>2025-10-20T15:13:02+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/npg-32-397-2025</id>
            <title type="html">Improving dynamical climate predictions with machine learning: insights from a twin experiment framework
            </title>
            <link href="https://doi.org/10.5194/npg-32-397-2025"/>
            <summary type="html">
                &lt;b&gt;Improving dynamical climate predictions with machine learning: insights from a twin experiment framework&lt;/b&gt;&lt;br&gt;
                Zikang He, Julien Brajard, Yiguo Wang, Xidong Wang, and Zheqi Shen&lt;br&gt;
                    Nonlin. Processes Geophys., 32, 397&#8211;409, https://doi.org/10.5194/npg-32-397-2025, 2025&lt;br&gt;
                Climate prediction is challenging due to systematic errors in traditional climate models. We addressed this by training a machine learning model to correct these errors and then integrating it with the traditional climate model to form an AI-physics hybrid model. Our study demonstrates that the hybrid model outperforms the original climate model on both short-term and long-term predictions of the atmosphere and ocean.
            </summary>
            <content type="html">
                &lt;b&gt;Improving dynamical climate predictions with machine learning: insights from a twin experiment framework&lt;/b&gt;&lt;br&gt;
                Zikang He, Julien Brajard, Yiguo Wang, Xidong Wang, and Zheqi Shen&lt;br&gt;
                    Nonlin. Processes Geophys., 32, 397&#8211;409, https://doi.org/10.5194/npg-32-397-2025, 2025&lt;br&gt;
                <p>Systematic errors in dynamical climate models remain a significant challenge to accurate climate predictions, particularly when modeling the nonlinear coupling between the atmosphere and ocean. Despite notable advances in dynamical climate modeling that have improved our understanding of climate variability, these systematic errors can still degrade prediction skills. In this study, we adopt a twin experiment framework with a reduced-order coupled atmosphere-ocean model to explore the utility of machine learning in mitigating these errors. Specifically, we train a data-driven model on data assimilation increments to learn and emulate the underlying dynamical climate model error, which is then integrated with the dynamical climate model to form a hybrid model. Comparison experiments show that the hybrid model consistently outperforms the standalone dynamical climate model in predicting atmospheric and oceanic variables. Further investigation using hybrid models that correct only atmospheric or only oceanic errors reveals that atmospheric corrections are essential for improving short-term predictions, while concurrently addressing both atmospheric and oceanic errors yields superior performance in long-term climate prediction.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2025-10-20T15:13:02+02:00</published>
            <updated>2025-10-20T15:13:02+02:00</updated>
        </entry>
</feed>