Ci-dessous, les différences entre deux révisions de la page.
| Les deux révisions précédentesRévision précédenteProchaine révision | Révision précédente | ||
| animation:seminaires:2015:accueil [2015/10/05 13:08] – [...........] cicaluga | animation:seminaires:2015:accueil [2017/03/10 10:01] (Version actuelle) – [What's new under the Sun?] cicaluga | ||
|---|---|---|---|
| Ligne 2: | Ligne 2: | ||
| ====== Séminaires/ | ====== Séminaires/ | ||
| + | ===== New wine into old wineskins: collisionless shocks in plasmas ===== | ||
| + | {{: | ||
| + | 11 décembre 2015 de 14h à 15h - Salle de Conférence, | ||
| + | |||
| + | **Antoine BRET**, Universidad Castilla La Mancha, ETSI Industriales, | ||
| + | |||
| + | |||
| + | Organisateurs : \\ | ||
| + | |||
| + | * Rolf Walder | ||
| + | * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon, France) \\ | ||
| + | |||
| + | **(19 participants)** | ||
| + | |||
| + | In 1808, Poisson realized that the conservation equations of a fluid through an interface offer 2 solutions: one continuous, when nothing changes, and another one, discontinuous, | ||
| + | |||
| + | Of course, the real world does not display any mathematical discontinuity. Since binary collisions are the only microscopic mechanisms capable of altering the fluid properties, the shock transition region in a fluid is a few mean-free-path thick. | ||
| + | |||
| + | How is it then that the Earth bow shock in the solar wind has its front about 100 km thick, while the mean-free-path at the same location is about the Sun-Earth distance? It just happens that plasmas, that is, charged fluids, can sustain shock waves through purely collective electromagnetic means, even in the absence of binary collisions. The talk will review our current knowledge of these entities, focusing in particular on the way they can be formed, and their fulfillment of the Rankine-Hugoniot conditions. | ||
| + | \\ | ||
| + | ===== Modelling a Multienzymatic Complex : Theoretical Strategies ===== | ||
| + | {{: | ||
| + | 30 octobre 2015 de 14h à 15h - Grande salle du CBP (LR6 C 023), ENS Lyon, France \\ | ||
| + | |||
| + | **Serge ANTONCZAK**, | ||
| + | |||
| + | |||
| + | Organisateurs : \\ | ||
| + | |||
| + | * Elise Dumont, Tangui Le Bahers (Laboratoire de Chimie, ENS de Lyon) \\ | ||
| + | * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon, France) \\ | ||
| + | |||
| + | **(28 participants)** | ||
| + | |||
| + | In each living system, the concentration of functional biological entities (e.g. proteins, | ||
| + | enzymes, peptides…) is incredibly high. Some transient complex-structures may appear and, | ||
| + | depending on the affinity the protagonists exhibit for each other, may subsist during | ||
| + | sufficiently long timescales that may lead to new functional systems called metabolons. | ||
| + | Experiments have demonstrated that some metabolons, lie at the vicinity of the membrane. \\ | ||
| + | The product of an enzymatic reaction becoming the substrate for the neighbour | ||
| + | enzyme, it only has to “jump” from an active site to the next one, diminishing unnecessary | ||
| + | diffusion processes and loss of energy during solvation and desolvation processes, yielding to | ||
| + | an enhanced catalytic efficiency. Being able to precisely describe the overall architecture of | ||
| + | these macromolecular assemblies has then become a key to understand the underlying | ||
| + | biological mechanisms and for developing new therapeutic strategies.\\ | ||
| + | So far, our investigations focused on an assembly composed by three enzymes | ||
| + | considered as key steps in the biosynthesis of anthocyanins and condensed tannins, namely | ||
| + | F3’H, DFR and LAR, in interaction with a model of membrane. In this presentation, | ||
| + | discussed the theoretical strategies carried out i) to characterise the enzymatic reaction | ||
| + | (QM/MM-MD simulations) ii) to define the way the substrates and the products enter in or are | ||
| + | released from the active site (brut force MD, Umbrella Sampling protocols…) iii) to design an | ||
| + | enzyme complex in interaction (ATTRACT docking protein/ | ||
| + | the interaction of this assembly with a model of membrane (OPM protocol).\\ | ||
| ===== Towards Climate-Dependent Sub-Grid-Scale Parameterizations in Atmospheric Models ===== | ===== Towards Climate-Dependent Sub-Grid-Scale Parameterizations in Atmospheric Models ===== | ||
| {{: | {{: | ||
| Ligne 13: | Ligne 66: | ||
| * Antoine Venaille (Laboratoire de Physique, ENS de Lyon, France) \\ | * Antoine Venaille (Laboratoire de Physique, ENS de Lyon, France) \\ | ||
| * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon, France) \\ | * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon, France) \\ | ||
| + | |||
| + | **(52 participants)** | ||
| Climate system models use a multitude of parameterization schemes for small-scale processes. These should respond to externally forced climate variability in an appropriate manner so as to reflect the response of the parameterized process to a changing climate. Indications are that they might not satisfy this condition to full satisfaction. The most attractive route to master the challenge of achieving such a behavior would be provided by theoretical understanding sufficiently deep to enable the à-priori design of climate-sensitive parameterization schemes. | Climate system models use a multitude of parameterization schemes for small-scale processes. These should respond to externally forced climate variability in an appropriate manner so as to reflect the response of the parameterized process to a changing climate. Indications are that they might not satisfy this condition to full satisfaction. The most attractive route to master the challenge of achieving such a behavior would be provided by theoretical understanding sufficiently deep to enable the à-priori design of climate-sensitive parameterization schemes. | ||
| Ligne 32: | Ligne 87: | ||
| **Jacky EVEN** (Fonctions Optiques pour les Technologies de l’information & INSA de Rennes) \\ | **Jacky EVEN** (Fonctions Optiques pour les Technologies de l’information & INSA de Rennes) \\ | ||
| **Mikaël KEPENEKIAN** (Institut des Sciences Chimiques de Rennes & CNRS) \\ | **Mikaël KEPENEKIAN** (Institut des Sciences Chimiques de Rennes & CNRS) \\ | ||
| + | |||
| + | **(27 participants)** | ||
| Organisateurs : \\ | Organisateurs : \\ | ||
| Ligne 51: | Ligne 108: | ||
| * Julien Vovelle (Institut Camille Jordan, Université Claude Bernard Lyon 1)\\ | * Julien Vovelle (Institut Camille Jordan, Université Claude Bernard Lyon 1)\\ | ||
| * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon) \\ | * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon) \\ | ||
| + | |||
| + | **(31 participants)** | ||
| On s’intéresse dans ce travail à l' | On s’intéresse dans ce travail à l' | ||
| Ligne 67: | Ligne 126: | ||
| * Julien Vovelle (Institut Camille Jordan, Université Claude Bernard Lyon 1) \\ | * Julien Vovelle (Institut Camille Jordan, Université Claude Bernard Lyon 1) \\ | ||
| * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon) \\ | * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon) \\ | ||
| + | |||
| + | **(31 participants)** | ||
| L' | L' | ||
| Ligne 78: | Ligne 139: | ||
| * Annamaria Kiss (Laboratoires Joliot-Curie, | * Annamaria Kiss (Laboratoires Joliot-Curie, | ||
| * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon) \\ | * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon) \\ | ||
| + | |||
| + | **(39 participants)** | ||
| Temporal networks are commonly used to represent systems where connections between elements are active only for restricted periods of time, such as telecommunication, | Temporal networks are commonly used to represent systems where connections between elements are active only for restricted periods of time, such as telecommunication, | ||
| Ligne 91: | Ligne 154: | ||
| * Stephane Labrosse, Caroline Fitoussi, Benoit Tauzin, Nicolas Coltice (Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement) \\ | * Stephane Labrosse, Caroline Fitoussi, Benoit Tauzin, Nicolas Coltice (Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement) \\ | ||
| * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon) \\ | * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon) \\ | ||
| + | |||
| + | **(30 participants)** | ||
| La diversité des compositions chimiques des basaltes à la surface de la Terre suggère que les roches du manteau Terrestre sont hétérogènes. Si une partie de ces hétérogénéités peut être attribuée à des processus constants de différenciation et de recyclage, certaines signatures géochimiques indiquent la préservation de matériel primordial sur plusieurs milliards d' | La diversité des compositions chimiques des basaltes à la surface de la Terre suggère que les roches du manteau Terrestre sont hétérogènes. Si une partie de ces hétérogénéités peut être attribuée à des processus constants de différenciation et de recyclage, certaines signatures géochimiques indiquent la préservation de matériel primordial sur plusieurs milliards d' | ||
| Ligne 109: | Ligne 174: | ||
| * Christian Perez et Jean-Yves L' | * Christian Perez et Jean-Yves L' | ||
| * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon, France) \\ | * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon, France) \\ | ||
| + | |||
| + | **(31 participants)** | ||
| In order to design and operates the future reactor for nuclear fusion | In order to design and operates the future reactor for nuclear fusion | ||
| Ligne 138: | Ligne 205: | ||
| good performance up to 1,835,008 threads (the complete Juqueen Blue | good performance up to 1,835,008 threads (the complete Juqueen Blue | ||
| Gene/Q at Jülich). | Gene/Q at Jülich). | ||
| - | |||
| ===== What's new under the Sun? ===== | ===== What's new under the Sun? ===== | ||
| {{: | {{: | ||
| Ligne 150: | Ligne 216: | ||
| * Antoine Venaille (Laboratoire de Physique, ENS de Lyon, France) \\ | * Antoine Venaille (Laboratoire de Physique, ENS de Lyon, France) \\ | ||
| * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon, France) \\ | * Cerasela Calugaru (Centre Blaise Pascal, ENS de Lyon, France) \\ | ||
| + | |||
| + | **(52 participants)** | ||
| We will discuss our recent progress to model in 3-D the solar global interior dynamics using the anelastic spherical harmonic (ASH) code. We will show | We will discuss our recent progress to model in 3-D the solar global interior dynamics using the anelastic spherical harmonic (ASH) code. We will show | ||
| Ligne 158: | Ligne 226: | ||
| When comparing with asymptotic formulations and an adiabatic oscillation code we find a good overall agreement and confirm that | When comparing with asymptotic formulations and an adiabatic oscillation code we find a good overall agreement and confirm that | ||
| those waves are indeed gravity waves. We then discuss their properties and visibility at the surface and compare with recent observations. \\ | those waves are indeed gravity waves. We then discuss their properties and visibility at the surface and compare with recent observations. \\ | ||
| - | |||