ICTS TIFR Discussion Meeting 2011 Indian Institute of Science, Bangalore

Similar documents
International Center for Theoretical Sciences (ICTS-TIFR), Tata Institute of Fundamental Research, Bangalore, India.

Day 1 : Monday

Effects of Galerkin-truncation on Inviscid Equations of Hydrodynamics. Samriddhi Sankar Ray (U. Frisch, S. Nazarenko, and T.

Bottlenecks: an interplay of equilibrium statistical mechanics and turbulence

Summer School in Cosmology. Programme

Chalonge de Vega Meudon Workshop 2016

COMPLETE LIST OF PUBLICATIONS OF ARNAB RAI CHOUDHURI

15th High Energy Astrophysics Division Meeting Naples, Florida Sunday, 3 April :00 pm Registration, 3:00 pm 7:00 pm, Royal Palms Foyer Speaker

Statistical studies of turbulent flows: self-similarity, intermittency, and structure visualization

The Physics of Fluids and Plasmas

Local flow structure and Reynolds number dependence of Lagrangian statistics in DNS of homogeneous turbulence. P. K. Yeung

Technical Meeting on Modern Neutron Detection

OUTBREAK INVESTIGATION AND SPATIAL ANALYSIS OF SURVEILLANCE DATA: CLUSTER DATA ANALYSIS. Preliminary Programme / Draft_2. Serbia, Mai 2013

Program. São Paulo School Advanced Science on High Energy and Plasma Astrophysics in the CTA Era (SPSAS-HighAstro)

Space Science Training Week data driven modeling and forecasting

Modern Aspects of Superconductivity

Workshop MHD-Days 2015

GOTHAM Summer School Program

Fluctuation dynamo amplified by intermittent shear bursts

Session Chair: Kim Sneppen. Session Chair: Saraswathi Vishveshwara 08:30AM - 09:00AM: REGISTRATION

ScienceDirect. Buoyancy driven turbulence of moist air

Programme for WEM2011. Time Title of the talk Code Presenting Author. Day 0: Tuesday, November 22, 2011

"Microscopy Advanced Tools for Tomorrow s Materials"

Role of polymers in the mixing of Rayleigh-Taylor turbulence

Formation of Inhomogeneous Magnetic Structures in MHD Turbulence and Turbulent Convection

AASTCS 5: Radio Exploration of Planetary Habitability 7 12 May, 2017

3 rd WHU Summer Theory Institute

Science Academy s Lecture Workshop on Spectroscopic Techniques and Applications in Material Characterization-(STAMC-2016)

After the deadline for abstract submission, a summary of current activities is reported below.

Vortex Dynamos. Steve Tobias (University of Leeds) Stefan Llewellyn Smith (UCSD)

A simple subgrid-scale model for astrophysical turbulence

The 3rd International Intensive Course on UNESCO Global Geoparks Geoparks Management and Earth Heritage Interpretation

Preferential concentration of inertial particles in turbulent flows. Jérémie Bec CNRS, Observatoire de la Côte d Azur, Université de Nice

Module 6: Free Convections Lecture 26: Evaluation of Nusselt Number. The Lecture Contains: Heat transfer coefficient. Objectives_template

LOW FREQUENCY EMISSION IN GALAXY CLUSTERS- M ACSJ

AASTCS 5: Radio Exploration of Planetary Habitability 7 12 May, 2017

First day Programme (October 23, 2018)

Frontiers in Gamma Ray Spectroscopy FIG18

11. THE IAUX XXVIII GENERAL ASSEMBLY DAY BY DAY

5:00pm-8:00pm Ala Moana, Carnation

REPORT ON THE RADIONET3 NETWORKING ACTIVITY

Solar cycle & Dynamo Modeling

Framework programme of 5th International Olympiad on Astronomy and Astrophysics

ALERT Olek Zienkiewicz Winterschool 2018

The Junior College Multi-Disciplinary Conference: Research, Practice and Collaboration

Ecole Internationale Daniel Chalonge. The 15th Paris Cosmology Colloquium 2011

Length Learning Objectives Learning Objectives Assessment

The behaviour of small inertial particles in homogeneous and isotropic turbulence

Notes Friday, September 09, 2016

Dynamo action at low magnetic Prandtl numbers: mean flow vs. fully turbulent motion

ATELIER INFORMATION QUANTIQUE ET MÉCANIQUE STATISTIQUE QUANTIQUE WORKSHOP QUANTUM INFORMATION AND QUANTUM STATISTICAL MECHANICS

Ecole Internationale Daniel Chalonge. The 18th Paris Cosmology Colloquium 2014

China University of Geosciences, Beijing, China

University of Bremen and Jacobs University Bremen, June 15 26, A: Simulation of biological systems and their functionalization

Ecole Internationale Daniel Chalonge. The 16th Paris Cosmology Colloquium 2012

Logistics 2/13/18. Topics for Today and Thur+ Helioseismology: Millions of sound waves available to probe solar interior. ASTR 1040: Stars & Galaxies

Theory and modelling of turbulent transport in astrophysical phenomena

Nanotechnology: Energy & Health

Small-Scale Dynamo and the Magnetic Prandtl Number

Final Program. Nanofluids: Fundamentals and Applications. September 16-20, 2007 Copper Mountain, Colorado. Co-Chairs

Gravitational Lensing. Einstein deflection angle Lens equation, magnification Galaxy lenses Cluster lenses Weak lensing Time delays in lenses

Final Agenda HEPP Colloquium 2013

Invited Lectures Delivered (Selected Only):

Logistics 2/14/17. Topics for Today and Thur. Helioseismology: Millions of sound waves available to probe solar interior. ASTR 1040: Stars & Galaxies

arxiv: v1 [physics.flu-dyn] 16 Nov 2018

web: Bangalore India, Research Associate at Department of Physics, Indian Institute of Science, Bangalore

Bifurcations and Chaos in Taylor-Green Dynamo

Numerical Study of Dynamo Action at Low Magnetic Prandtl Numbers

Role of thermal plumes on particle dispersion in a turbulent Rayleigh-Bénard cell

Plasma Physics for Astrophysics

DAνCo 2017 Plenary Session Program

45th Meeting of the DPS Block Schedule

Programme of the first annual meeting

TIME TABLE SLOT. BTech 1 st year

Heavy ions: Experiments Confront Theory

TA Instruments NEW AR-G2 INTRODUCING THE WORLD S FIRST MAGNETIC BEARING RHEOMETER! The World Leader in Thermal Analysis and Rheology Systems

Alfvén wave turbulence: new results with applications to astrophysics. Sébastien GALTIER Université Paris-Sud & Institut Universitaire de France

Flow visualization for a natural convection in a horizontal layer of water over a heated smooth and grooved surfaces

Similarity scaling of pressure fluctuation in turbulence

Introduction to the Chinese Giant Solar Telescope

Prediction of solar activity cycles by assimilating sunspot data into a dynamo model

Program. 17:15 18:00 Vanderlei Bagnato (São Carlos Brazil) New experiments in the investigation of quantum turbulence in a trapped superfluid

SRIHARI KESHAVAMURTHY

Lagrangian Statistics. of 3D MHD Convection. J. Pratt, W.-C. Müller. Boussinesq Simulation. Lagrangian. simulation. March 1, 2011

arxiv:physics/ v1 8 Sep 2005

Dynamo Simulations in Solar Convection Zone

Curriculum Vitae. Dr. Krishna Kumar. Address: Department of Physics Indian Institute of Technology Kharagpur , West Bengal, India

Introduction to the Summer Institute 2009

Workshop on Field Theoretic Aspects of Gravity (FTAG) XI-2016

WORKSHOP ON. Jointly organized by the. International Seabed Authority Kingston, Jamaica. Ministry of Earth Sciences, Government of India AGENDA

Institute of Geography and Spatial Management, Faculty of Geography and Geology, Jagiellonian University

Shell-to-shell energy transfer in magnetohydrodynamics. I. Steady state turbulence

Multi-Hazard Mitigation of Risks to Cultural Heritage

7th ENMIX WORKSHOP. Wednesday 03 April Thursday 04 April 2019 CNR - Headquarter. Scientific Programme

Solar Wind Turbulence

warwickphysics Physics Courses

Generation of magnetic fields by large-scale vortices in rotating convection

Course Syllabus for Spring 2016

THE DYNAMO EFFECT IN STARS

Euromech/Ercoftac Colloquium 589 Turbulent Cascades II Ecole Centrale de Lyon - Amphi 1 building W1

Transcription:

ICTS TIFR Discussion Meeting 2011 Indian Institute of Science, Bangalore PROGRAMME 12 16 December 2011 Venue Auditorium Centre for Nanoscience and Engineering (CeNSE), IISc. 12 December 2011 Monday 08:30 9:00 am REGISTRATION 09-9:30 am - Welcome RAHUL PANDIT, JAYWANT H ARAKERI, URIEL FRISCH Overview of ICTS H R KRISHNAMURTHY - R Govindarajan, JNCASR Bangalore 09:30 10:15 am 10:15 11:00 am R Narasimha JNCASR, Bangalore P K Yeung Georgia Tech. USA Big computing for insight: The challenge of turbulent shear flows Petascale computing for studies of turbulent mixing and dispersion: current status and future prospectsm 11:00 11:30 am COFFEE - R Govindarajan, JNCASR Bangalore 11:30 am 12:15 pm J Bec Observatoire de la Côte d Azur France Direct numerical simulations of particles suspended in a turbulent flow 12:15 01:30 pm LUNCH 01:30 02:15 pm - K R Sreenivasan,NYU, USA 02:15 04:00 pm Free 04:00 05:00 pm Faculty Hall Subrahmanyam Chandrasekhar lecture by Uriel Frisch Observatoire de la Côte d Azur, France

13 December 2011 Tuesday : Sriram Ramaswamy, K R Sreenivasan, NY Univ., USA Considerations on resolution requirements for threedimensional turbulence J Schumacher Technische Univ. Germany Numerical challenges for supercomputations in dry and moist high-rayleigh number convection : Sriram Ramaswamy, M E Brachet CNRS France On new developments of the analyticity-strip method applied to the Taylor-Green vortex 11:45 am 12:30 pm J H Arakeri Flow structure and scaling laws in Rayleigh-Benard and in convection in tubes at high Rayleigh numbers 12:30 2:00 pm LUNCH : Rahul Pandit, 02:00 02:45 pm J van der Hoeven CNRS France Multi-precision computations and high performance: a delicate marriage 02:45 03:30 pm S Chakrabarty Niels Bohr Institute, Denmark Higher precision versus higher Reynolds number: Case of Nelkin scaling in Burgulence 03:30 4:00 pm COFFEE 04:00 05:00 pm : Uriel Frisch, OCA, Nice France

14 December 2011 Wednesday : Arnab Rai Choudhuri, 09:45 10:30 am A Pouquet NCAR, USA M Verma IIT Kanpur Some issues in MHD turbulence Object-oriented Pseudo-spectral code TARANG for turbulence simulation : Arnab Rai Choudhuri, G Sahoo Systematics of the magnetic prandtle number Max Planck Institute, dependence of MHD turbulence Goettingen, Germany 11:45 am 12:45 pm : P K Yeung, Georgia Tech. USA 12:45 pm 2:00 pm LUNCH FREE

15 December 2011 Thursday : J Mathew, K Itakura JAMESTec. Japan The architecture and the application performance of the Earth Simulator S Musacchio Nice Sophia-Antipolis, France Numerical simulations of turbulent fluid layers : J Mathew, T Ishihara High-performance computing of canonical Nagoya University high- Reynolds-number turbulent flows 11:45 am 12:30 pm P Perlekar Technische Universitei, Eindhoven Discrete population dynamics in turbulence 12:30 1:45 pm LUNCH : J Bec, OCA,Nice 01:45 02:30 pm Z-S She Peking University, China A mean-field theory working side-by-side with simulations 02:30 03:15 pm S S Ray Observatoire de la Côte d Azur, France A resonance phenomenon for the Galerkintruncated Burgers and Euler equations 03:15 4:00 pm COFFEE 04:00 5:30 pm : L Biferale Rome, Italy

16 December 2011 Friday : V Krishan, Indian Institute of Astrophysics, Bangalore 09:00 09:45 am L Biferale Rome, Italy P Sharma Studies of helicity in three-dimensional fluid turbulence Role of Turbulence in Galaxy Clusters and Accretion Flows 10:30 11:00 am COFFEE : V Krishan, Indian Institute of Astrophysics, Bangalore 11:00 am 11:45 pm R S Nanjundiah Turbulence in Climate Studies 11:45 am 12:30 pm D Mitra NORDITA Sweden Search for the solar dynamo in a computer 12:30 2:00 pm LUNCH : V Krishan, Indian Institute of Astrophysics, Bangalore 02:00 02:45 pm R Pandit Turbulent flows with polymer additives 02:45 03:30 pm COFFEE 03:30 5:00 pm : A Pouquet, NCAR, USA