{"id":24,"date":"2020-08-05T12:28:36","date_gmt":"2020-08-05T09:28:36","guid":{"rendered":"https:\/\/phsites.technion.ac.il\/frishman\/?page_id=24"},"modified":"2025-07-08T11:54:55","modified_gmt":"2025-07-08T08:54:55","slug":"research","status":"publish","type":"page","link":"https:\/\/phsites.technion.ac.il\/frishman\/research\/","title":{"rendered":"Research"},"content":{"rendered":"\n<p class=\"has-text-align-center\">Below you can find some of the projects I\u2019ve worked on as well as ongoing research.<\/p>\n\n\n\n<div class=\"wp-block-genesis-blocks-gb-columns gb-layout-service-3 gb-layout-columns-2 gb-2-col-wideleft gb-columns-center alignfull\" style=\"padding-top:1%;padding-right:5%;padding-bottom:1%;padding-left:5%\"><div class=\"gb-layout-column-wrap gb-block-layout-column-gap-5 gb-is-responsive-column\" style=\"max-width:1200px\">\n<div class=\"wp-block-genesis-blocks-gb-column gb-block-layout-column\"><div class=\"gb-block-layout-column-inner\">\n<h2 class=\"wp-block-heading\">Self-organization of turbulent flows<\/h2>\n\n\n\n<p>Turbulence is usually viewed as the breaking up of a large scale flow into ever smaller chaotic motions. A quantitative manifestation of this picture is the energy cascade, with energy flowing from large scales to increasingly smaller ones, where it is eventually dissipated by viscosity. <br>On the contrary, when most of the energy is concetrated in 2d modes, energy is transferred to progressively larger scales&#8211;in an inverse cascade. This process can then terminate in the self-organization of the turbulence into a large scale mean flow, a so-called condensate, on top of small scale fluctuations.<\/p>\n\n\n\n<p>Although such 2d turbulence may seem like an abstract concept, many natural flows are effectively restricted to two dimensions: planetary-scale flows in the ocean and atmosphere are an example, and they are often made up of coherent currents or vortices in combination with chaotic fluctuations.<\/p>\n\n\n\n<p>Our work is centered around the following questions: What are the rules of self-organization for the condensate? Which of its features are universal? What happens when the range of fluid-element interactions is below the energy injection scale? Recently, we have also started to explore condensates that have both 2d-like and 3d-like interactions.<\/p>\n\n\n\n<div class=\"wp-block-group has-background\" style=\"background-color:#f1f1f1\"><div class=\"wp-block-group__inner-container is-layout-constrained wp-block-group-is-layout-constrained\">\n<h3 class=\"wp-block-heading\">Read more<\/h3>\n\n\n\n<ul style=\"background-color:#f1f1f1\" class=\"wp-block-list has-background\">\n<li>Svirsky, A, and Frishman A. <em>&#8220;<a href=\"https:\/\/doi.org\/10.1103\/PhysRevLett.134.204001\">Out-of-equilibrium fluxes shape the self-organization of locally-interacting turbulence<\/a>\u201d.<\/em> Phys. Rev. Lett. <em>134(20), 204001 <\/em>(2025).<\/li>\n\n\n\n<li>Svirsky, A., Herbert, C. and Frishman, A. <em>\u201c<a href=\"https:\/\/doi.org\/10.1103\/PhysRevLett.131.224003\">Two-dimensional turbulence with local interactions: statistics of the condensate<\/a>.\u201d <\/em>Phys. Rev. Lett., 131(22), 224003&nbsp;(2023).<\/li>\n\n\n\n<li>Frishman, A. and Herbert C.&nbsp;<em>\u201c<a href=\"https:\/\/journals.aps.org\/prl\/abstract\/10.1103\/PhysRevLett.120.204505\">Turbulence Statistics in a Two-Dimensional Vortex Condensate<\/a>.\u201d<\/em>&nbsp; Phys. Rev. Lett.&nbsp;120.20: 204505 (2018).<\/li>\n\n\n\n<li class=\"has-black-color has-text-color has-link-color wp-elements-bd79ec52ec9a04768b899676d75a77e7\">Frishman A.\u00a0<em><a href=\"https:\/\/pubs.aip.org\/aip\/pof\/article\/29\/12\/125102\/990468\/The-culmination-of-an-inverse-cascade-Mean-flow\">\u201cThe culmination of an inverse cascade: mean flow and fluctuations.\u201d<\/a>\u00a0<\/em>Physics of Fluids\u00a029.12: 125102. (2017).<\/li>\n<\/ul>\n<\/div><\/div>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-genesis-blocks-gb-column gb-block-layout-column\"><div class=\"gb-block-layout-column-inner\">\n<div style=\"height:50px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<figure class=\"wp-block-image size-large\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"480\" src=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/nice_plot-1024x480.jpg\" alt=\"The large scale flow can either form jets or vortices, depending on the distance of the dissipative scale from the forcing scale when energy in LQG turbulence\" class=\"wp-image-136\" srcset=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/nice_plot-1024x480.jpg 1024w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/nice_plot-300x141.jpg 300w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/nice_plot-768x360.jpg 768w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/nice_plot-1536x721.jpg 1536w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/nice_plot-2048x961.jpg 2048w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\" \/><figcaption class=\"wp-element-caption\">The large scale flow can either form jets or vortices, depending on the distance of the dissipative scale from the forcing scale in a local version of two dimensional turbulence  [Figure from Svirsky, A., and Frishman A.\u00a0Phys. Rev. Lett.\u00a0 134, 204001(2025)].<\/figcaption><\/figure>\n<\/div><\/div>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator has-css-opacity\" \/>\n\n\n\n<div class=\"wp-block-genesis-blocks-gb-columns gb-layout-service-3 gb-layout-columns-2 gb-2-col-wideleft gb-columns-center alignfull\" style=\"padding-top:1%;padding-right:5%;padding-bottom:1%;padding-left:5%\"><div class=\"gb-layout-column-wrap gb-block-layout-column-gap-5 gb-is-responsive-column\" style=\"max-width:1200px\">\n<div class=\"wp-block-genesis-blocks-gb-column gb-block-layout-column\"><div class=\"gb-block-layout-column-inner\">\n<h2 class=\"wp-block-heading\">Subcritical transition to turbulence<\/h2>\n\n\n\n<p>Fluid flow generically becomes turbulent when the Reynolds number, which is the relevant control parameter, is sufficiently increased. In flows where the base state is linearly stable, termed subcritical flows, this transition occurs directly to a turbulent state, with turbulence appearing intermittently in space and time. With increasing Reynolds number, the system transitions between several different phases until finally reaching the homogeneous turbulent state.<\/p>\n\n\n\n<p>Building on recent progress in the field, our work aims to understand the different possible phases and under which conditions they occur; the role of fluctuations and the mechanisms leading to transitions between phases and the generallity of the subcritical transition scenario.<\/p>\n\n\n\n<div class=\"wp-block-group has-very-light-gray-background-color has-background\"><div class=\"wp-block-group__inner-container is-layout-flow wp-block-group-is-layout-flow\">\n<h3 class=\"wp-block-heading\">Read more<\/h3>\n\n\n\n<ul style=\"background-color:#f1f1f1\" class=\"wp-block-list has-background\">\n<li>Svirsky, A., Grafke T. and Frishman A. <em>\u201cSelf-Replication of Turbulent Puffs: On the edge between chaotic saddles\u201d, <a href=\"https:\/\/doi.org\/10.48550\/arXiv.2505.05075\">arXiv:2505.05075<\/a><\/em>.<\/li>\n\n\n\n<li>Frishman, A. and Grafke T. <em>&#8220;<a href=\"https:\/\/doi.org\/10.1098\/rspa.2022.0218\">Mechanism for turbulence proliferation in subcritical flows<\/a>.&#8221;<\/em>&nbsp; Proceedings of the Royal Society A 478.2265: 20220218, (2022).<\/li>\n\n\n\n<li>Frishman, A. and Grafke, T. <em>\u201c<a href=\"https:\/\/doi.org\/10.1103\/PhysRevE.105.045108\">Dynamical landscape of transitional pipe flow<\/a>&#8220;,<\/em> Phys, Rev. E&nbsp; 105.4: 045108 (2022).<\/li>\n<\/ul>\n<\/div><\/div>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-genesis-blocks-gb-column gb-block-layout-column\"><div class=\"gb-block-layout-column-inner\">\n<div style=\"height:50px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<figure class=\"wp-block-image size-large\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"853\" src=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/many_gaps_zoom1-1024x853.png\" alt=\"laminar gaps randomly open and close in transitional turbulent pipe flow, the level of turbulence along the pipe as a function of time is shown\" class=\"wp-image-146\" srcset=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/many_gaps_zoom1-1024x853.png 1024w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/many_gaps_zoom1-300x250.png 300w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/many_gaps_zoom1-768x640.png 768w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/many_gaps_zoom1.png 1050w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\" \/><figcaption class=\"wp-element-caption\">Laminar gaps randomly open and close in transitional turbulent pipe flow, the level of turbulence along the pipe as a function of time is shown.<\/figcaption><\/figure>\n<\/div><\/div>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator has-css-opacity\" \/>\n\n\n\n<div class=\"wp-block-genesis-blocks-gb-columns gb-layout-service-3 gb-layout-columns-2 gb-2-col-equal gb-columns-center alignfull\" style=\"padding-top:1%;padding-right:5%;padding-bottom:1%;padding-left:5%\"><div class=\"gb-layout-column-wrap gb-block-layout-column-gap-5 gb-is-responsive-column\" style=\"max-width:1200px\">\n<div class=\"wp-block-genesis-blocks-gb-column gb-block-layout-column\"><div class=\"gb-block-layout-column-inner\">\n<h2 class=\"wp-block-heading\">Clouds and their fate<\/h2>\n\n\n\n<p>Clouds consist of water droplets; as these droplets collide and coallese they grow, until eventually they start falling out of the cloud, producing rain.&nbsp; What fraction of the water in a cloud will remain in it after it rains down? How long will it live? The answer to these questions depends on the initial charatcrestics of the cloud. Our work aims to construct a minimal coarse-grained description of this depdnence, using ideal models of the droplet population dynamics in the cloud.<\/p>\n\n\n\n<div class=\"wp-block-group has-very-light-gray-background-color has-background\"><div class=\"wp-block-group__inner-container is-layout-flow wp-block-group-is-layout-flow\">\n<h3 class=\"wp-block-heading\">Read more<\/h3>\n\n\n\n<ul style=\"background-color:#f1f1f1\" class=\"wp-block-list has-background\">\n<li>Kapon, S., Jeevanjee N. and Frishman A. &#8220;<em>Single-parameter effective dynamics of warm cloud precipitation<\/em>.&#8221;&nbsp;<em> <a href=\"https:\/\/doi.org\/10.48550\/arXiv.2409.05398\">arXiv:2409.05398<\/a><\/em>&nbsp;<\/li>\n<\/ul>\n<\/div><\/div>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-genesis-blocks-gb-column gb-block-layout-column\"><div class=\"gb-block-layout-column-inner\">\n<div style=\"height:50px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<figure class=\"wp-block-image size-large\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"288\" src=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/combined_plots_with_units-1024x288.png\" alt=\"\" class=\"wp-image-150\" srcset=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/combined_plots_with_units-1024x288.png 1024w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/combined_plots_with_units-300x84.png 300w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/combined_plots_with_units-768x216.png 768w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/combined_plots_with_units-1536x433.png 1536w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/combined_plots_with_units-2048x577.png 2048w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\" \/><\/figure>\n\n\n\n<figure class=\"wp-block-image size-large\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"286\" src=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/combined_plots_no_theory-1024x286.png\" alt=\"Cloud observables collapse when presented as a function of a dimensionless parameter quantifying accretion vs rainfall\" class=\"wp-image-152\" srcset=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/combined_plots_no_theory-1024x286.png 1024w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/combined_plots_no_theory-300x84.png 300w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/combined_plots_no_theory-768x214.png 768w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/combined_plots_no_theory-1536x429.png 1536w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/combined_plots_no_theory-2048x571.png 2048w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\" \/><figcaption class=\"wp-element-caption\"><br>Cloud observables collapse when presented as a function of a dimensionless parameter quantifying accretion vs rainfall<\/figcaption><\/figure>\n\n\n\n<figure class=\"wp-block-image size-full\"><img loading=\"lazy\" decoding=\"async\" width=\"683\" height=\"167\" src=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/Cloudsbackground-picture.jpg\" alt=\"clouds\" class=\"wp-image-232\" srcset=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/Cloudsbackground-picture.jpg 683w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/Cloudsbackground-picture-300x73.jpg 300w\" sizes=\"auto, (max-width: 683px) 100vw, 683px\" \/><\/figure>\n<\/div><\/div>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator has-css-opacity\" \/>\n\n\n\n<div class=\"wp-block-genesis-blocks-gb-columns gb-layout-service-3 gb-layout-columns-2 gb-2-col-wideleft gb-columns-center alignfull\" style=\"padding-top:1%;padding-right:5%;padding-bottom:1%;padding-left:5%\"><div class=\"gb-layout-column-wrap gb-block-layout-column-gap-5 gb-is-responsive-column\" style=\"max-width:1200px\">\n<div class=\"wp-block-genesis-blocks-gb-column gb-block-layout-column\"><div class=\"gb-block-layout-column-inner\">\n<h2 class=\"wp-block-heading\">Universality in the breakup of a fluid bridge<\/h2>\n\n\n\n<p>The breakup of a fluid object is a singular and dramatic process. We explore how a cylindrical soap film bridge breaks when stretched, and find that it always forms one large central satellite bubble. We show that the size of this bubble is extremely reproducible, and grows with the stretching rate and with the initial bridge aspect ratio. We trace the robustness of the size to an underlying universal dynamical solution.<\/p>\n\n\n\n<div class=\"wp-block-group has-very-light-gray-background-color has-background\"><div class=\"wp-block-group__inner-container is-layout-flow wp-block-group-is-layout-flow\">\n<h3 class=\"wp-block-heading\">Read more<\/h3>\n\n\n\n<ul style=\"background-color:#f1f1f1\" class=\"wp-block-list has-background\">\n<li>Frishman A. and Lecoanet, D. <em><a href=\"https:\/\/journals.aps.org\/prfluids\/abstract\/10.1103\/PhysRevFluids.10.063604\">\u201cUniversality of satellites in the breakup of a stretched fluid bridge\u201d<\/a>,<\/em> Phys. Rev. Fluids 10.6 (2025): 063604<em> <\/em>(2025).<\/li>\n<\/ul>\n<\/div><\/div>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-genesis-blocks-gb-column gb-block-layout-column\"><div class=\"gb-block-layout-column-inner\">\n<div style=\"height:50px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<figure class=\"wp-block-video\"><video height=\"328\" style=\"aspect-ratio: 792 \/ 328;\" width=\"792\" controls src=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2025\/06\/Media1.mp4\"><\/video><\/figure>\n<\/div><\/div>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator has-css-opacity\" \/>\n\n\n\n<div class=\"wp-block-genesis-blocks-gb-columns gb-layout-columns-2 gb-2-col-wideleft gb-columns-center alignfull\" style=\"padding-top:2%;padding-right:5%;padding-bottom:1%;padding-left:5%\"><div class=\"gb-layout-column-wrap gb-block-layout-column-gap-5 gb-is-responsive-column\" style=\"max-width:1200px\">\n<div class=\"wp-block-genesis-blocks-gb-column gb-block-layout-column\"><div class=\"gb-block-layout-column-inner\">\n<h2 class=\"wp-block-heading\">Stochastic force inference <\/h2>\n\n\n\n<p>Particles in biological and soft matter systems undergo Brownian dynamics: their deterministic motion, induced by forces, competes with random diffusion due to thermal noise. More broadly, Brownian dynamics is a generic and simple model for dynamical systems with noise.&nbsp;<\/p>\n\n\n\n<p>Given only the noisy trajectories resulting from such dynamics \u2013 could we determine the equations that generated them? How would we do that in practice? Of particular interest are trajectories generated by an out-of-equilibrium process, in which case one would like to be able to identify the signatures of irreversibility and quantify it.<\/p>\n\n\n\n<p>Our proposed solutions, including a practical inference method, are based on ideas from information theory and stochastic thermodynamics.<\/p>\n\n\n\n<div class=\"wp-block-group has-very-light-gray-background-color has-background\"><div class=\"wp-block-group__inner-container is-layout-flow wp-block-group-is-layout-flow\">\n<h3 class=\"wp-block-heading\">    Read more<\/h3>\n\n\n\n<ul style=\"background-color:#f1f1f1\" class=\"wp-block-list has-background\">\n<li>Frishman, A. and Ronceray P.  <em>\u201c<a href=\"https:\/\/journals.aps.org\/prx\/abstract\/10.1103\/PhysRevX.10.021009\">Learning force fields from stochastic trajectories<\/a>.&#8221;<\/em> Phys. Rev. X&nbsp;10.2: 021009 (2020).<\/li>\n<\/ul>\n<\/div><\/div>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-genesis-blocks-gb-column gb-block-layout-column\"><div class=\"gb-block-layout-column-inner\">\n<div style=\"height:50px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<figure class=\"wp-block-image size-large\"><img loading=\"lazy\" decoding=\"async\" width=\"502\" height=\"576\" src=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2020\/08\/Stochastic-force-inference-prx10.jpg\" alt=\"Stochastic force inference with nonlinear force fields.\nFigure from Ronceray P. and Frishman, A. \u201cLearning force fields from stochastic trajectories.\u201d Phys. Rev. X 10.2: 021009 (2020).\" class=\"wp-image-25\" srcset=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2020\/08\/Stochastic-force-inference-prx10.jpg 502w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2020\/08\/Stochastic-force-inference-prx10-261x300.jpg 261w\" sizes=\"auto, (max-width: 502px) 100vw, 502px\" \/><figcaption class=\"wp-element-caption\">Stochastic force inference with nonlinear force fields.<br>Figure from Frishman, A. and Ronceray P.  Phys. Rev. X&nbsp;10, 021009 (2020).<\/figcaption><\/figure>\n<\/div><\/div>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator has-css-opacity is-style-default\" \/>\n\n\n\n<div class=\"wp-block-genesis-blocks-gb-columns gb-layout-service-3 gb-layout-columns-2 gb-2-col-wideleft gb-columns-center alignfull\" style=\"padding-top:1%;padding-right:5%;padding-bottom:1%;padding-left:5%\"><div class=\"gb-layout-column-wrap gb-block-layout-column-gap-5 gb-is-responsive-column\" style=\"max-width:1200px\">\n<div class=\"wp-block-genesis-blocks-gb-column gb-block-layout-column\"><div class=\"gb-block-layout-column-inner\">\n<h2 class=\"wp-block-heading\">Lagrangian time irreversibility of turbulence<\/h2>\n\n\n\n<p>Turbulence is an out-of-equilibrium phenomena as evidenced by the flux of energy through scales. But how could you see that irreversibility if you are only watching particles in the flow? What is the manifestation of the energy flux, which is a property of the velocity field, for particles? What changes if the flow is compressible?<\/p>\n\n\n\n<div class=\"wp-block-group has-very-light-gray-background-color has-background\"><div class=\"wp-block-group__inner-container is-layout-flow wp-block-group-is-layout-flow\">\n<h3 class=\"wp-block-heading\">Read more<\/h3>\n\n\n\n<ul style=\"background-color:#f1f1f1\" class=\"wp-block-list has-background\">\n<li>Grafke, T., Frishman A., and Falkovich G. &#8220;<em><a href=\"https:\/\/journals.aps.org\/pre\/abstract\/10.1103\/PhysRevE.91.043022\">Time irreversibility of the statistics of a single particle in compressible turbulence<\/a><\/em>.&#8221; Phys. Rev. E&nbsp; 91.4, 043022, (2015).<\/li>\n\n\n\n<li>&nbsp;Frishman A. and Falkovich G. &#8220;<em><a href=\"https:\/\/journals.aps.org\/prl\/abstract\/10.1103\/PhysRevLett.113.024501\">A new type of anomaly in turbulence<\/a><\/em>&#8220;. Phys. Rev. Lett.113.02, 024501, (2014).<\/li>\n\n\n\n<li>Falkovich, G., and Frishman A. &#8220;<em><a href=\"https:\/\/journals.aps.org\/prl\/abstract\/10.1103\/PhysRevLett.110.214502\">Single Flow Snapshot Reveals the Future and the Past of Pairs of Particles in Turbulence<\/a><\/em>.&#8221; Phys. Rev. Lett.110.21 214502 (2013).<\/li>\n<\/ul>\n<\/div><\/div>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-genesis-blocks-gb-column gb-block-layout-column\"><div class=\"gb-block-layout-column-inner\">\n<div style=\"height:50px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<figure class=\"wp-block-image size-large\"><img loading=\"lazy\" decoding=\"async\" width=\"397\" height=\"395\" src=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2020\/08\/PNAS-111-21-7558-7563-2014.png\" alt=\"Picture from Xu, Haitao, et al. &quot;Flight\u2013crash events in turbulence.&quot; PNAS 111.21: 7558-7563 (2014)\" class=\"wp-image-27\" srcset=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2020\/08\/PNAS-111-21-7558-7563-2014.png 397w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2020\/08\/PNAS-111-21-7558-7563-2014-300x298.png 300w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2020\/08\/PNAS-111-21-7558-7563-2014-150x150.png 150w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2020\/08\/PNAS-111-21-7558-7563-2014-80x80.png 80w\" sizes=\"auto, (max-width: 397px) 100vw, 397px\" \/><figcaption class=\"wp-element-caption\">Image taken from Xu, Haitao, et al. &#8220;Flight\u2013crash events in turbulence.&#8221; <a href=\"https:\/\/www.pnas.org\/content\/111\/21\/7558\">PNAS 111.21: 7558-7563 (2014)<\/a>.<\/figcaption><\/figure>\n<\/div><\/div>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator has-css-opacity is-style-default\" \/>\n\n\n\n<div class=\"wp-block-genesis-blocks-gb-columns gb-layout-service-3 gb-layout-columns-2 gb-2-col-wideleft gb-columns-center alignfull\" style=\"padding-top:1%;padding-right:5%;padding-bottom:1%;padding-left:5%\"><div class=\"gb-layout-column-wrap gb-block-layout-column-gap-5 gb-is-responsive-column\" style=\"max-width:1200px\">\n<div class=\"wp-block-genesis-blocks-gb-column gb-block-layout-column\"><div class=\"gb-block-layout-column-inner\">\n<h2 class=\"wp-block-heading\">Lagrangian conservation laws<\/h2>\n\n\n\n<p>Conservation laws and symmetries play a central role in physics. Relatively recently, it was discovered that Lagrangian statistical conservation laws, related to the dynamics of particles, play a crucial role in the field theoretic description of turbulence. Their influence was demonstrated for the statistics of a field advected by the flow, and their form could be computed in simplified models for the velocity field. It remains unclear how to obtain such laws for a real turbulent velocity field, and what their influence could be on the field\u2019s statistics. We have made some attempts in that direction.<\/p>\n\n\n\n<div class=\"wp-block-group has-very-light-gray-background-color has-background\"><div class=\"wp-block-group__inner-container is-layout-flow wp-block-group-is-layout-flow\">\n<h3 class=\"wp-block-heading\">Read more<\/h3>\n\n\n\n<ul style=\"background-color:#f1f1f1\" class=\"wp-block-list has-background\">\n<li>Falkovich, G., and Frishman A. \u201c<em><a href=\"https:\/\/journals.aps.org\/prl\/abstract\/10.1103\/PhysRevLett.110.214502\">Single Flow Snapshot Reveals the Future and the Past of Pairs of Particles in Turbulence<\/a><\/em>.\u201d Phys. Rev. Lett.110.21 214502 (2013).<\/li>\n\n\n\n<li>Frishman, A., Boffetta, G., De Lillo, F., &amp; Liberzon, A. \u201c<em><a href=\"https:\/\/journals.aps.org\/pre\/abstract\/10.1103\/PhysRevE.91.033018\">Statistical conservation law in two-and three-dimensional turbulent flows<\/a>.\u201d&nbsp;<\/em>&nbsp;Phys. Rev. E&nbsp; 91.3, 033018, (2015).<\/li>\n<\/ul>\n<\/div><\/div>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-genesis-blocks-gb-column gb-block-layout-column\"><div class=\"gb-block-layout-column-inner\">\n<div style=\"height:50px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<figure class=\"wp-block-image size-large\"><img loading=\"lazy\" decoding=\"async\" width=\"608\" height=\"369\" src=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2020\/08\/PRL-86-424-2012.png\" alt=\"\" class=\"wp-image-30\" srcset=\"https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2020\/08\/PRL-86-424-2012.png 608w, https:\/\/phsites.technion.ac.il\/frishman\/wp-content\/uploads\/sites\/59\/2020\/08\/PRL-86-424-2012-300x182.png 300w\" sizes=\"auto, (max-width: 608px) 100vw, 608px\" \/><figcaption class=\"wp-element-caption\">Image taken from Celani, Vergassola. \u201cStatistical geometry in scalar turbulence.\u201d <a href=\"https:\/\/journals.aps.org\/prl\/abstract\/10.1103\/PhysRevLett.86.424\">PRL 86.3: 424 (2012)<\/a>.<\/figcaption><\/figure>\n<\/div><\/div>\n<\/div><\/div>\n\n\n\n<p style=\"font-size:14px\">\u00b7 <em>Banner Image Credit: NASA\/<a href=\"https:\/\/oceancolor.gsfc.nasa.gov\/\">Ocean Biology Processing Group<\/a>, NASA Goddard Space Flight Center<\/em> \u00b7<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Below you can find some of the projects I\u2019ve worked on as well as ongoing research. \u00b7 Banner Image Credit: NASA\/Ocean Biology Processing Group, NASA Goddard Space Flight Center \u00b7<\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_genesis_hide_title":false,"_genesis_hide_breadcrumbs":false,"_genesis_hide_singular_image":false,"_genesis_hide_footer_widgets":false,"_genesis_custom_body_class":"","_genesis_custom_post_class":"","_genesis_layout":"","footnotes":""},"class_list":{"0":"post-24","1":"page","2":"type-page","3":"status-publish","5":"entry"},"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.5 - 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