Gabriel George Katul
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Previous Organizations / Institutes
The organizations / institutes from the scholar's other articles in the past ten years
Research Subjects
Gabriel George Katul has a total of 1000 co-authors. Here are the top co-authors by number of shared publications:
- Davide Poggi
Department of Environment, Land and Infrastructure Engineering (DIATI), Politecnico di Torino, Turin, Italy
40 shared publications Ram Oren
Nicholas School of the Environment, Duke University, Durham, NC, United States
39 shared publicationsAmilcare Porporato
Department of Civil and Environmental Engineering, Princeton University, Princeton, NJ, USA
36 shared publications- Mario Siqueira
Universidade de Brasília
36 shared publications - Elie Bou-Zeid
Department of Civil and Environmental Engineering Princeton University Princeton NJ USA
26 shared publications - Paul Christopher Stoy
Biological Systems Engineering, University of Wisconsin-Madison, Madison, WI, USA
25 shared publications
Latest Publications
- 2 September 2026
- Published by Springer Nature
- p. 497-534
Phloem Catastrophe: Identifying Plant Tipping Points Through Bifurcation Analysis
- 2 September 2026
- Published by Springer Nature
- p. 497-534
Phloem Catastrophe: Identifying Plant Tipping Points Through Bifurcation Analysis
- Open Access
- 21 August 2026
- Published by American Geophysical Union (AGU) in Earth's Future
- Vol. 14 (8)
Climate‐Induced Severe Water Scarcity Events as Harbingers of Global Wheat Price
This study connects the dots between global extent of severe water scarcity (SWS) events and spikes in food price. The authors start with three staple crops (rice, wheat, and maize) using a empirical but crop specific characterization of severe water scarcity occurrence, which is defined based on the area of land cultivated with each studied crop that on a given year is under SWS conditions. Water scarcity is estimated based on 1, 3, and 12 months standardized precipitation evapotranspiration index during crop specific sensitive periods (SPs). SPs coincide with the 4 months prior to harvest. A SWS‐wheat price relationship model was developed for period 2001–2021 and tested for 1986–2000 and 2022–2024 with future projections calculated under climate change using climate model simulations from CMIP5 and CMIP6 up to 2100. The results show a marked increase in wheat prices driven by increasing SWS area, which is in turn a function of greenhouse gas emissions. The results indicate that the meanglobal mean temperature increase by 3°C (compared to 1951–1980) could lead to the tripling of the mean global wheat price compared to 2010 (after deflating).
- 21 August 2026
- Published by American Geophysical Union (AGU) in Earth's Future
- Vol. 14 (8)
Open AccessClimate‐Induced Severe Water Scarcity Events as Harbingers of Global Wheat Price
This study connects the dots between global extent of severe water scarcity (SWS) events and spikes in food price. The authors start with three staple crops (rice, wheat, and maize) using a empirical but crop specific characterization of severe water scarcity occurrence, which is defined based on the area of land cultivated with each studied crop that on a given year is under SWS conditions. Water scarcity is estimated based on 1, 3, and 12 months standardized precipitation evapotranspiration index during crop specific sensitive periods (SPs). SPs coincide with the 4 months prior to harvest. A SWS‐wheat price relationship model was developed for period 2001–2021 and tested for 1986–2000 and 2022–2024 with future projections calculated under climate change using climate model simulations from CMIP5 and CMIP6 up to 2100. The results show a marked increase in wheat prices driven by increasing SWS area, which is in turn a function of greenhouse gas emissions. The results indicate that the meanglobal mean temperature increase by 3°C (compared to 1951–1980) could lead to the tripling of the mean global wheat price compared to 2010 (after deflating).
- Open Access
- 17 August 2026
- Published by American Geophysical Union (AGU) in Journal of Advances in Modeling Earth Systems
- Vol. 18 (8)
Food, Energy, and Health Implications of Agrivoltaic Farms
The benefits of agrivoltaics (AV) are documented, with empirical evidence for their suitability for collocated energy generation, crop cultivation, and water savings, even for staple crops. What is lacking is a holistic modeling framework to design and optimize AV systems for specific crop types, micro‐environments, and panel configurations. To this end, a multiphysics model that simultaneously solves momentum, energy, and mass exchanges among interacting components, and determines the implications of AV on photosynthesis, water use, power generation, and worker thermal stress is introduced. The model is tested against field data from California and Minnesota. Its applications are illustrated for a representative AV scenario using weather data from central New Jersey, showcasing the multifaceted benefits of AV for a tomato farm under photovoltaic panels. In this scenario, the model predicts a 5.6 reduction in average daytime panel temperature (compared to a common photovoltaic installation), recovering 15% of the thermal energy losses. Despite a 47% reduction in light for the setup modeled here, net carbon assimilation declined by 31%. Daytime crop leaf temperature cooled by 1.84, and these reductions offset some of the decline in carbon assimilation. Another benefit is the reduction in transpiration losses by 22.4% compared to an open crop field. Finally, the average perceived temperature experienced by workers was reduced by approximately 4.46 during working hours. While these are illustrative results for a particular crop and climate, they demonstrate how the model enables integrated assessment and optimization of AV benefits across varying climates, crops, and photovoltaic technologies.
- 17 August 2026
- Published by American Geophysical Union (AGU) in Journal of Advances in Modeling Earth Systems
- Vol. 18 (8)
Open AccessFood, Energy, and Health Implications of Agrivoltaic Farms
The benefits of agrivoltaics (AV) are documented, with empirical evidence for their suitability for collocated energy generation, crop cultivation, and water savings, even for staple crops. What is lacking is a holistic modeling framework to design and optimize AV systems for specific crop types, micro‐environments, and panel configurations. To this end, a multiphysics model that simultaneously solves momentum, energy, and mass exchanges among interacting components, and determines the implications of AV on photosynthesis, water use, power generation, and worker thermal stress is introduced. The model is tested against field data from California and Minnesota. Its applications are illustrated for a representative AV scenario using weather data from central New Jersey, showcasing the multifaceted benefits of AV for a tomato farm under photovoltaic panels. In this scenario, the model predicts a 5.6 reduction in average daytime panel temperature (compared to a common photovoltaic installation), recovering 15% of the thermal energy losses. Despite a 47% reduction in light for the setup modeled here, net carbon assimilation declined by 31%. Daytime crop leaf temperature cooled by 1.84, and these reductions offset some of the decline in carbon assimilation. Another benefit is the reduction in transpiration losses by 22.4% compared to an open crop field. Finally, the average perceived temperature experienced by workers was reduced by approximately 4.46 during working hours. While these are illustrative results for a particular crop and climate, they demonstrate how the model enables integrated assessment and optimization of AV benefits across varying climates, crops, and photovoltaic technologies.
- Open Access
- 20 July 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1039, A2
Stratification, turbulence organisation and pressure-strain effects on surface-layer turbulence anisotropy
At large scales, the Reynolds stress tensor exhibits notable anisotropy, a key feature of all wall-bounded turbulent flows. Yet, how the drivers of this anisotropy evolve with shearing and thermal stratification in the atmospheric surface layer (ASL) remains a daunting challenge for theory and models alike. Here, the velocity variance budgets are used to explore the evolution of anisotropy in the daytime ASL close to the surface, a region known to be problematic for large-eddy simulations. A special focus is placed on the importance of slow and rapid pressure-strain correlations, and the role of transport on partitioning the turbulent kinetic energy among the velocity components. Results obtained from near-surface observations of four datasets over flat and horizontally homogeneous terrain show persistent anisotropy over a wide range of flux Richardson numbers italic Ri Subscript f ${\textit{Ri}}_{\!f}$ and wall-normal distances, and highlight the importance of different processes in three distinct flow regimes, roughly related to dynamic ( StartAbsoluteValue italic Ri Subscript f Baseline EndAbsoluteValue much less than 1 $|{\textit{Ri}}_{\!f}|\ll 1$ ), dynamic-convective ( StartAbsoluteValue italic Ri Subscript f Baseline EndAbsoluteValue tilde 1 $|{\textit{Ri}}_{\!f}|\sim 1$ ) and convective ( StartAbsoluteValue italic Ri Subscript f Baseline EndAbsoluteValue much greater than 1 $|{\textit{Ri}}_{\!f}|\gg 1$ ) regimes of the ASL. In particular, close to the surface in the dynamic-convective regime, a drop in wall-normal velocity variance and a substantial increase of spanwise velocity variance are shown to result from the increasing role of pressure transport and rapid distortion, related to turbulence organisation. This behaviour is not captured by the classic Rotta closure but requires the inclusion of both rapid pressure-strain and transport terms. In all regimes, wall blocking is found to influence turbulence close to the surface, thus requiring the adoption of an anisotropic Rotta model to accommodate its effects.- 20 July 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1039, A2
Open AccessStratification, turbulence organisation and pressure-strain effects on surface-layer turbulence anisotropy
At large scales, the Reynolds stress tensor exhibits notable anisotropy, a key feature of all wall-bounded turbulent flows. Yet, how the drivers of this anisotropy evolve with shearing and thermal stratification in the atmospheric surface layer (ASL) remains a daunting challenge for theory and models alike. Here, the velocity variance budgets are used to explore the evolution of anisotropy in the daytime ASL close to the surface, a region known to be problematic for large-eddy simulations. A special focus is placed on the importance of slow and rapid pressure-strain correlations, and the role of transport on partitioning the turbulent kinetic energy among the velocity components. Results obtained from near-surface observations of four datasets over flat and horizontally homogeneous terrain show persistent anisotropy over a wide range of flux Richardson numbers italic Ri Subscript f ${\textit{Ri}}_{\!f}$ and wall-normal distances, and highlight the importance of different processes in three distinct flow regimes, roughly related to dynamic ( StartAbsoluteValue italic Ri Subscript f Baseline EndAbsoluteValue much less than 1 $|{\textit{Ri}}_{\!f}|\ll 1$ ), dynamic-convective ( StartAbsoluteValue italic Ri Subscript f Baseline EndAbsoluteValue tilde 1 $|{\textit{Ri}}_{\!f}|\sim 1$ ) and convective ( StartAbsoluteValue italic Ri Subscript f Baseline EndAbsoluteValue much greater than 1 $|{\textit{Ri}}_{\!f}|\gg 1$ ) regimes of the ASL. In particular, close to the surface in the dynamic-convective regime, a drop in wall-normal velocity variance and a substantial increase of spanwise velocity variance are shown to result from the increasing role of pressure transport and rapid distortion, related to turbulence organisation. This behaviour is not captured by the classic Rotta closure but requires the inclusion of both rapid pressure-strain and transport terms. In all regimes, wall blocking is found to influence turbulence close to the surface, thus requiring the adoption of an anisotropic Rotta model to accommodate its effects. - Open Access
- 7 July 2026
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 53 (13)
Directional Dynamics of Fog: Irreversibility and Causal Coupling With Turbulence
Fog prediction remains challenging because the physical processes governing its life cycle evolve across time scales and do not follow reversible or stationary dynamics. Using high‐frequency visibility observations from Sable Island, Canada, this study analyzes fog intensity and turbulent kinetic energy (TKE) for their time irreversibility and causal relations. Fog intensity exhibits temporal asymmetry in all stages, while TKE remains nearly reversible. The lead–lag structure between the two variables is stage dependent: TKE leads fog intensity during formation, the coupling becomes symmetric during the mature phase, and fog intensity leads TKE during dissipation. Notably, during fog formation, the strength of fog's intrinsic irreversibility increases linearly with the strength of its causal linkage to TKE, revealing that fog initiation is governed by a directional sequence of turbulence–moisture interactions. These findings demonstrate that fog is a non‐equilibrium, time‐asymmetric system, and that capturing its stage‐dependent directionality is required for enhanced fog prediction.
- 7 July 2026
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 53 (13)
Open AccessDirectional Dynamics of Fog: Irreversibility and Causal Coupling With Turbulence
Fog prediction remains challenging because the physical processes governing its life cycle evolve across time scales and do not follow reversible or stationary dynamics. Using high‐frequency visibility observations from Sable Island, Canada, this study analyzes fog intensity and turbulent kinetic energy (TKE) for their time irreversibility and causal relations. Fog intensity exhibits temporal asymmetry in all stages, while TKE remains nearly reversible. The lead–lag structure between the two variables is stage dependent: TKE leads fog intensity during formation, the coupling becomes symmetric during the mature phase, and fog intensity leads TKE during dissipation. Notably, during fog formation, the strength of fog's intrinsic irreversibility increases linearly with the strength of its causal linkage to TKE, revealing that fog initiation is governed by a directional sequence of turbulence–moisture interactions. These findings demonstrate that fog is a non‐equilibrium, time‐asymmetric system, and that capturing its stage‐dependent directionality is required for enhanced fog prediction.
- 30 May 2026
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research: Atmospheres
- Vol. 131 (11)
Scaling Laws for the Longitudinal Turbulent Heat Flux in the Atmospheric Surface Layer
The longitudinal turbulent heat flux is central to the description of vertical momentum and energy transport in stratified atmospheric boundary layers, yet its scaling behavior with respect to thermal stratification remains uncertain in comparison to better‐studied quantities such as the vertical heat flux. Here, the scaling laws of the longitudinal heat flux and its co‐spectrum in the atmosphere close to the surface as a function of wall normal distance and thermal stratification are experimentally evaluated. Measurements were conducted under varying stability regimes ranging from unstable to slightly stable at two sites. The first experiment included five high‐temporal resolution (100 Hz) velocity and temperature sensors as well as a triaxial sonic anemometer all positioned within 2 m above a bare soil surface. The second experiment included a single triaxial sonic anemometer positioned at 5 m above the surface of a grass‐covered forest clearing. The analysis first examines the Reynolds‐averaged Navier‐Stokes equations for the longitudinal heat flux and applies similarity theory to identify the dominant terms. This analysis is then used to inform a co‐spectral budget, which is used to deduce the appropriate scaling laws at large and inertial subrange scales. The proposed theory aims to reconcile discrepancies reported across field, laboratory, and numerical studies, and highlights the importance of non‐conserved scale‐wise flux transfer mechanisms unique to longitudinal heat flux in turbulent flows even when the longitudinal heat flux transport term is small.
- 30 May 2026
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research: Atmospheres
- Vol. 131 (11)
Scaling Laws for the Longitudinal Turbulent Heat Flux in the Atmospheric Surface Layer
The longitudinal turbulent heat flux is central to the description of vertical momentum and energy transport in stratified atmospheric boundary layers, yet its scaling behavior with respect to thermal stratification remains uncertain in comparison to better‐studied quantities such as the vertical heat flux. Here, the scaling laws of the longitudinal heat flux and its co‐spectrum in the atmosphere close to the surface as a function of wall normal distance and thermal stratification are experimentally evaluated. Measurements were conducted under varying stability regimes ranging from unstable to slightly stable at two sites. The first experiment included five high‐temporal resolution (100 Hz) velocity and temperature sensors as well as a triaxial sonic anemometer all positioned within 2 m above a bare soil surface. The second experiment included a single triaxial sonic anemometer positioned at 5 m above the surface of a grass‐covered forest clearing. The analysis first examines the Reynolds‐averaged Navier‐Stokes equations for the longitudinal heat flux and applies similarity theory to identify the dominant terms. This analysis is then used to inform a co‐spectral budget, which is used to deduce the appropriate scaling laws at large and inertial subrange scales. The proposed theory aims to reconcile discrepancies reported across field, laboratory, and numerical studies, and highlights the importance of non‐conserved scale‐wise flux transfer mechanisms unique to longitudinal heat flux in turbulent flows even when the longitudinal heat flux transport term is small.
- Open Access
- 20 April 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1033
On the wall-normal velocity variance in canonical wall-bounded turbulence
The variance and spectra of wall-normal velocities are investigated for direct numerical simulations of turbulent flow in a channel, pipe and zero-pressure-gradient boundary layer across a decade of friction Reynolds numbers. Spectra along the spanwise wavenumber have a pronounced peak well described by the turbulent dissipation rate and the local shear stress throughout the bottom half of the boundary layer. Deviations in the local stress from the surface shear velocity $U_\tau$ account for almost all of the differences in wall-normal velocity variance observed across different canonical flows, including for plane Couette flow. The dependence on the local stress is attributed to the fact that wall-normal motions are predominately ‘active’ per Townsend’s attached eddy hypothesis and directly contribute to the local shear stress, noting this hypothesis assumes simplified ideal conditions with constant turbulent shear stress. A semi-empirical fit applied to the Reynolds-number dependence of the variance matches the simulations across the lower half of the boundary layer and aligns with observed values in the literature. The fit extrapolates to a value between 1.45 and 1.65 times the local shear stress in the high-Reynolds-number limit, consistent with previous predictions relative to $U_\tau$ including for the vertical velocity in the near-neutral atmospheric boundary layer. However, universality in the exact proportional constant is precluded by small discrepancies in the variances corresponding to dissimilarity in the low-wavenumber contributions across different flow configurations and wall-normal positions. We speculate the dissimilarity is due to relatively weak ‘inactive’ wall-normal motions that are excluded from Townsend’s original hypothesis.- 20 April 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1033
Open AccessOn the wall-normal velocity variance in canonical wall-bounded turbulence
The variance and spectra of wall-normal velocities are investigated for direct numerical simulations of turbulent flow in a channel, pipe and zero-pressure-gradient boundary layer across a decade of friction Reynolds numbers. Spectra along the spanwise wavenumber have a pronounced peak well described by the turbulent dissipation rate and the local shear stress throughout the bottom half of the boundary layer. Deviations in the local stress from the surface shear velocity $U_\tau$ account for almost all of the differences in wall-normal velocity variance observed across different canonical flows, including for plane Couette flow. The dependence on the local stress is attributed to the fact that wall-normal motions are predominately ‘active’ per Townsend’s attached eddy hypothesis and directly contribute to the local shear stress, noting this hypothesis assumes simplified ideal conditions with constant turbulent shear stress. A semi-empirical fit applied to the Reynolds-number dependence of the variance matches the simulations across the lower half of the boundary layer and aligns with observed values in the literature. The fit extrapolates to a value between 1.45 and 1.65 times the local shear stress in the high-Reynolds-number limit, consistent with previous predictions relative to $U_\tau$ including for the vertical velocity in the near-neutral atmospheric boundary layer. However, universality in the exact proportional constant is precluded by small discrepancies in the variances corresponding to dissimilarity in the low-wavenumber contributions across different flow configurations and wall-normal positions. We speculate the dissimilarity is due to relatively weak ‘inactive’ wall-normal motions that are excluded from Townsend’s original hypothesis. - Open Access
- 14 March 2026
- Published by Copernicus GmbH
Safe Operating Regimes for Phloem Carbon Transport: A Bifurcation Framework
A mathematical framework is developed to quantify the stability of phloem transport and delineate “safe operating” regimes using bifurcation analysis. Sucrose production is linked to leaf photosynthesis using stomatal optimality, while sucrose translocation follows pressure-driven flow based on the Munch mechanism. The model couples xylem water potential, osmotic driving force, hydraulic resistance (using a sucrose-dependent viscosity), and distributed sink removal along the transport pathway. Systematic variation of key carbon transport controls, such as xylem water potential and sink strength, reveals multiple equilibria and stability boundaries beyond which phloem transport becomes unstable to small carbon loading fluctuations. Phloem failure emerges through a saddle-node bifurcation, yielding two stable sucrose loading states separated by an unstable branch where the lower equilibrium falls within reported sucrose loading ranges. The resulting stability maps provide a mechanistic basis for phloem vulnerability and suggest that vascular safety requires coordination between photosynthetic supply (e.g., $V_{c,max}$), pathway length, and transport capacity as water potential declines. This stability map provides a mechanistic constraint that can inform trait-based ecosystem modeling and provide hypotheses about acclimation and vulnerability across environments.
- 14 March 2026
- Published by Copernicus GmbH
Open AccessSafe Operating Regimes for Phloem Carbon Transport: A Bifurcation Framework
A mathematical framework is developed to quantify the stability of phloem transport and delineate “safe operating” regimes using bifurcation analysis. Sucrose production is linked to leaf photosynthesis using stomatal optimality, while sucrose translocation follows pressure-driven flow based on the Munch mechanism. The model couples xylem water potential, osmotic driving force, hydraulic resistance (using a sucrose-dependent viscosity), and distributed sink removal along the transport pathway. Systematic variation of key carbon transport controls, such as xylem water potential and sink strength, reveals multiple equilibria and stability boundaries beyond which phloem transport becomes unstable to small carbon loading fluctuations. Phloem failure emerges through a saddle-node bifurcation, yielding two stable sucrose loading states separated by an unstable branch where the lower equilibrium falls within reported sucrose loading ranges. The resulting stability maps provide a mechanistic basis for phloem vulnerability and suggest that vascular safety requires coordination between photosynthetic supply (e.g., $V_{c,max}$), pathway length, and transport capacity as water potential declines. This stability map provides a mechanistic constraint that can inform trait-based ecosystem modeling and provide hypotheses about acclimation and vulnerability across environments.
- Open Access
- 13 March 2026
- Published by Copernicus GmbH
Global Potential of Agrivoltaics for Sustainable Food and Energy Transitions
The dual challenge of meeting rising global food demand while accelerating the clean energy transition requires innovative land-use strategies. Agrivoltaics—the co-location of solar photovoltaics and agriculture—offers a transformative solution, yet global adoption has been hindered by a lack of standardized sunlight requirements for crops. Here, we introduce a framework to quantify crop-specific light requirements using the Daily Light Integral (DLI). We define two distinct thresholds: a “theoretical” DLI and a “real-world” DLI. Applying these thresholds to the world’s four staple crops (wheat, maize, rice, and soybean), we assess the global potential for co-generation without compromising food security. Our analysis reveals that even under conservative design scenarios SC40 that prioritize food security, agrivoltaic systems could generate over 100,000 TWh of electricity annually. Soybean and wheat demonstrate the highest compatibility, particularly in the Middle East, South Asia, and the Americas. These findings outline a quantitative pathway for sustainable land-use transitions, showing that multifunctional landscapes can simultaneously mitigate climate change, reduce water use, and strengthen rural resilience. Agrivoltaics exemplifies the water–energy–food–environment nexus at scale by improving land-use efficiency, creating favorable microclimates, and reducing evaporative demand.
- 13 March 2026
- Published by Copernicus GmbH
Open AccessGlobal Potential of Agrivoltaics for Sustainable Food and Energy Transitions
The dual challenge of meeting rising global food demand while accelerating the clean energy transition requires innovative land-use strategies. Agrivoltaics—the co-location of solar photovoltaics and agriculture—offers a transformative solution, yet global adoption has been hindered by a lack of standardized sunlight requirements for crops. Here, we introduce a framework to quantify crop-specific light requirements using the Daily Light Integral (DLI). We define two distinct thresholds: a “theoretical” DLI and a “real-world” DLI. Applying these thresholds to the world’s four staple crops (wheat, maize, rice, and soybean), we assess the global potential for co-generation without compromising food security. Our analysis reveals that even under conservative design scenarios SC40 that prioritize food security, agrivoltaic systems could generate over 100,000 TWh of electricity annually. Soybean and wheat demonstrate the highest compatibility, particularly in the Middle East, South Asia, and the Americas. These findings outline a quantitative pathway for sustainable land-use transitions, showing that multifunctional landscapes can simultaneously mitigate climate change, reduce water use, and strengthen rural resilience. Agrivoltaics exemplifies the water–energy–food–environment nexus at scale by improving land-use efficiency, creating favorable microclimates, and reducing evaporative demand.
- Open Access
- 6 February 2026
- Published by Wiley
Intermittency buildup across precipitation cascades: Endogenous versus exogenous factors
The temporal variability of precipitation originates from the multiplicative effects of air uplift and vapor-to-liquid conversion. The latter is commonly represented by a product of conversion efficiency and water vapor fluctuations. How exogenous effects such as those related to uplift contribute to the precipitation variance and to the build-up of intermittency within the precipitation cascade is investigated. The analysis employs a large dataset of 5-minute precipitation time series collected in a domain characterized by a combination of orographic, frontal, and convective systems, each with at least 30 years in record length. Exogenous versus endogenous factors (i.e. those related to water vapor turbulent fluctuations) responsible for intermittency build-up across the precipitation cascade were explored using the so-called propagator kernel. This analysis shows that precipitation generation maintains its signature at scales one order of magnitude smaller than the integral time. This interaction between exogenous and endogenous factors appears more significant in high-elevation precipitation records. The overall effect of such interactions is to reduce the anomalous scaling at the sub-storm time scales.
- 6 February 2026
- Published by Wiley
Open AccessIntermittency buildup across precipitation cascades: Endogenous versus exogenous factors
The temporal variability of precipitation originates from the multiplicative effects of air uplift and vapor-to-liquid conversion. The latter is commonly represented by a product of conversion efficiency and water vapor fluctuations. How exogenous effects such as those related to uplift contribute to the precipitation variance and to the build-up of intermittency within the precipitation cascade is investigated. The analysis employs a large dataset of 5-minute precipitation time series collected in a domain characterized by a combination of orographic, frontal, and convective systems, each with at least 30 years in record length. Exogenous versus endogenous factors (i.e. those related to water vapor turbulent fluctuations) responsible for intermittency build-up across the precipitation cascade were explored using the so-called propagator kernel. This analysis shows that precipitation generation maintains its signature at scales one order of magnitude smaller than the integral time. This interaction between exogenous and endogenous factors appears more significant in high-elevation precipitation records. The overall effect of such interactions is to reduce the anomalous scaling at the sub-storm time scales.