School on Astrophysical Fluid Dynamics | (smr 1865)
Go to day
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08:30 - 10:45
REGISTRATION AND ADMINISTRATIVE FORMALITIES
(All visitors are kindly requested to register with the
Secretary outside the Giambiagi Lecture Hall). Those receiving financial support or reimbursements will then have to see our Finance Office in the Fermi Building (after registration).
Extra shuttle bus runs will be provided from the Adriatico to the Fermi Building and back for this purpose.
- 08:30 REGISTRATION AND ADMINISTRATIVE FORMALITIES (All visitors are kindly requested to register with the Secretary outside the Giambiagi Lecture Hall). Those receiving financial support or reimbursements will then have to see our Finance Office in the Fermi Building (after registration). Extra shuttle bus runs will be provided from the Adriatico to the Fermi Building and back for this purpose. 2h15'
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10:45 - 11:00
Inauguration and opening remarks by Professor K.R. Sreenivasan, Director of ICTP.
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10:45
Inauguration and opening remarks by Professor K.R. Sreenivasan, Director of ICTP.
15'
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10:45
Inauguration and opening remarks by Professor K.R. Sreenivasan, Director of ICTP.
15'
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11:00 - 12:30
Occurrence and character of astrophysical fluids:
(1) temperatures, densities, ionisation and composition of stars, interplanetary medium, ISM, ICM, IGM; (2) distribution of magnetic field; (3) heating and cooling of gas; (4) evolution of cosmic gas from big bang to present day
Tutors: T.D. Saini & S.K. Sethi
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11:00
Occurrence and character of astrophysical fluids:
(1) temperatures, densities, ionisation and composition of stars, interplanetary medium, ISM, ICM, IGM; (2) distribution of magnetic field; (3) heating and cooling of gas; (4) evolution of cosmic gas from big bang to present day
1h30'
Speaker: Instructor: Dipankar BHATTACHARYA (IUCAA, Pune, India) Material: lecture notes
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11:00
Occurrence and character of astrophysical fluids:
(1) temperatures, densities, ionisation and composition of stars, interplanetary medium, ISM, ICM, IGM; (2) distribution of magnetic field; (3) heating and cooling of gas; (4) evolution of cosmic gas from big bang to present day
1h30'
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12:30 - 14:00
Lunch Break
- 12:30 Lunch Break 1h30'
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14:00 - 15:30
Numerical simulations in astrophysics: the PLUTO code
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14:00
Numerical simulations in astrophysics: the PLUTO code
1h30'
Speaker: Instructors: Silvano MASSAGLIA & Andrea MIGNONE (University of Torino, Italy) Material: lecture notes
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14:00
Numerical simulations in astrophysics: the PLUTO code
1h30'
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15:30 - 15:45
Coffee Break
- 15:30 Coffee Break 15'
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15:45 - 17:00
Basic numerical discretization method: (1) differentiation; (2) integration; (3) interpolation
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15:45
Basic numerical discretization method: (1) differentiation; (2) integration; (3) interpolation
1h15'
Speaker: Instructors: Silvano MASSAGLIA & Andrea MIGNONE
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15:45
Basic numerical discretization method: (1) differentiation; (2) integration; (3) interpolation
1h15'
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08:30 - 10:45
REGISTRATION AND ADMINISTRATIVE FORMALITIES
(All visitors are kindly requested to register with the
Secretary outside the Giambiagi Lecture Hall). Those receiving financial support or reimbursements will then have to see our Finance Office in the Fermi Building (after registration).
Extra shuttle bus runs will be provided from the Adriatico to the Fermi Building and back for this purpose.
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09:00 - 10:30
Introduction: equations of motion; Hydrostatic equilibrium: atmospheres; Steady flow of an ideal fluid; Bernoulli's equation and applications; Vorticity: Circulation theorem; Vortex lines
Tutors: S.K. Sethi & T.D. Saini
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09:00
Introduction: equations of motion; Hydrostatic equilibrium: atmospheres; Steady flow of an ideal fluid; Bernoulli's equation and applications; Vorticity: Circulation theorem; Vortex lines
1h30'
Speaker: Instructor: Sridhar SESHADRI (Raman Ressearch Institute, Bangalore, India) Material: lecture notes
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09:00
Introduction: equations of motion; Hydrostatic equilibrium: atmospheres; Steady flow of an ideal fluid; Bernoulli's equation and applications; Vorticity: Circulation theorem; Vortex lines
1h30'
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10:30 - 11:00
Coffee Break
- 10:30 Coffee Break 30'
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11:00 - 12:30
Hydrostatics of planets, stars and cluster gas motion in astrophysical fluids: (1) convection in stars; (2) stellar winds - de Laval nozzle, Parker solution; (3) transonic flows; (4) implosions (gravitational collapse) and explosions
Tutors: T.D. Saini & S.K. Sethi
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11:00
Hydrostatics of planets, stars and cluster gas motion in astrophysical fluids: (1) convection in stars; (2) stellar winds - de Laval nozzle, Parker solution; (3) transonic flows; (4) implosions (gravitational collapse) and explosions
1h30'
Speaker: Instructor: Dipankar BHATTACHARYA Material: lecture notes
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11:00
Hydrostatics of planets, stars and cluster gas motion in astrophysical fluids: (1) convection in stars; (2) stellar winds - de Laval nozzle, Parker solution; (3) transonic flows; (4) implosions (gravitational collapse) and explosions
1h30'
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12:30 - 14:00
Lunch Break
- 12:30 Lunch Break 1h30'
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14:00 - 15:30
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14:00
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1h30'
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14:00
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1h30'
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15:30 - 15:45
Coffee Break
- 15:30 Coffee Break 15'
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15:45 - 17:00
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15:45
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1h15'
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15:45
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1h15'
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09:00 - 10:30
Introduction: equations of motion; Hydrostatic equilibrium: atmospheres; Steady flow of an ideal fluid; Bernoulli's equation and applications; Vorticity: Circulation theorem; Vortex lines
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09:00 - 10:30
Potential flows, incompressible potential flows; Gravity waves and instability
Tutors: S.K. Sethi & T.D. Saini
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09:00
Potential flows, incompressible potential flows; Gravity waves and instability
1h30'
Speaker: Instructor: Sridhar SESHADRI
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09:00
Potential flows, incompressible potential flows; Gravity waves and instability
1h30'
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10:30 - 11:00
Coffee Break
- 10:30 Coffee Break 30'
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11:00 - 12:30
Shock waves in astrophysical fluids
Tutors: T.D. Saini & S.K. Sethi
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11:00
Shock waves in astrophysical fluids
1h30'
Speaker: Instructor: Dipankar BHATTACHARYA Material: lecture notes
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11:00
Shock waves in astrophysical fluids
1h30'
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12:30 - 14:00
Lunch Break
- 12:30 Lunch Break 1h30'
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14:00 - 15:30
Theory of linear advection equation: (1) discretization, stability, Upwind method, characteristics; (2) practice session with PLUTO code
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14:00
Theory of linear advection equation: (1) discretization, stability, Upwind method, characteristics; (2) practice session with PLUTO code
1h30'
Speaker: Instructors: Silvano MASSAGLIA & Andrea MIGNONE Material: lecture notes
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14:00
Theory of linear advection equation: (1) discretization, stability, Upwind method, characteristics; (2) practice session with PLUTO code
1h30'
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15:30 - 15:45
Coffee Break
- 15:30 Coffee Break 15'
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15:45 - 17:00
Theory of linear hyperbolic systems: (1) Riemann problem; (2) characteristic decomposition
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15:45
Theory of linear hyperbolic systems: (1) Riemann problem; (2) characteristic decomposition
1h15'
Speaker: Instructors: Silvano MASSAGLIA & Andrea MIGNONE
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15:45
Theory of linear hyperbolic systems: (1) Riemann problem; (2) characteristic decomposition
1h15'
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19:00 - 21:00
Reception - Buffet Dinner, Adriatico Guesthouse
Location: Adriatico Guest House Cafeteria - 19:00 Reception - Buffet Dinner, Adriatico Guesthouse 2h0'
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09:00 - 10:30
Potential flows, incompressible potential flows; Gravity waves and instability
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09:00 - 10:30
Viscous fluids: viscous stress and strain tensors; Navier-Stokes equation: energy dissipation; incompressible fluids; Viscous diffusion of vorticity: boundary layers
Tutors: S.K. Sethi & T.D. Saini
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09:00
Viscous fluids: viscous stress and strain tensors; Navier-Stokes equation: energy dissipation; incompressible fluids; Viscous diffusion of vorticity: boundary layers
1h30'
Speaker: Instructor: Sridhar SESHADRI
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09:00
Viscous fluids: viscous stress and strain tensors; Navier-Stokes equation: energy dissipation; incompressible fluids; Viscous diffusion of vorticity: boundary layers
1h30'
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10:30 - 11:00
Coffee Break
- 10:30 Coffee Break 30'
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11:00 - 12:30
Accretion flows, disks, jets (basic treatment), description of astrophysical sources with accretion flows
Tutors: T.D. Saini & S.K. Sethi
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11:00
Accretion flows, disks, jets (basic treatment), description of astrophysical sources with accretion flows
1h30'
Speaker: Instructor: Dipankar BHATTACHARYA Material: lecture notes
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11:00
Accretion flows, disks, jets (basic treatment), description of astrophysical sources with accretion flows
1h30'
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12:30 - 14:00
Lunch Break
- 12:30 Lunch Break 1h30'
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14:00 - 15:30
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14:00
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1h30'
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14:00
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1h30'
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15:30 - 15:45
Coffee Break
- 15:30 Coffee Break 15'
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15:45 - 17:00
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15:45
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1h15'
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15:45
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1h15'
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09:00 - 10:30
Viscous fluids: viscous stress and strain tensors; Navier-Stokes equation: energy dissipation; incompressible fluids; Viscous diffusion of vorticity: boundary layers
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09:00 - 10:30
Scaling in the NS equations; Flow past obstacles: Stokes flow; Flow past a cylinder: transition to turbulence; Homogeneous, isotropic turbulence
Tutors: S.K. Sethi & T.D. Saini
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09:00
Scaling in the NS equations; Flow past obstacles: Stokes flow; Flow past a cylinder: transition to turbulence; Homogeneous, isotropic turbulence
1h30'
Speaker: Instructor: Sridhar SESHADRI
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09:00
Scaling in the NS equations; Flow past obstacles: Stokes flow; Flow past a cylinder: transition to turbulence; Homogeneous, isotropic turbulence
1h30'
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10:30 - 11:00
Coffee Break
- 10:30 Coffee Break 30'
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11:00 - 12:30
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11:00
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1h30'
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11:00
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1h30'
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12:30 - 14:00
Lunch Break
- 12:30 Lunch Break 1h30'
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14:00 - 15:30
Magnetohydrodynamics (MHD): (1) Riemann problem; (2) approx Riemann solver; (3) practice session (Sod shock tube) with PLUTO; (4) -div.B=0
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14:00
Magnetohydrodynamics (MHD): (1) Riemann problem; (2) approx Riemann solver; (3) practice session (Sod shock tube) with PLUTO; (4) -div.B=0
1h30'
Speaker: Silvano MASSAGLIA & Andrea MIGNONE Material: lecture notes
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14:00
Magnetohydrodynamics (MHD): (1) Riemann problem; (2) approx Riemann solver; (3) practice session (Sod shock tube) with PLUTO; (4) -div.B=0
1h30'
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15:30 - 15:45
Coffee Break
- 15:30 Coffee Break 15'
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15:45 - 17:00
Higher order extension
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15:45
Higher order extension
1h15'
Speaker: Silvano MASSAGLIA & Andrea MIGNONE
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15:45
Higher order extension
1h15'
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09:00 - 10:30
Scaling in the NS equations; Flow past obstacles: Stokes flow; Flow past a cylinder: transition to turbulence; Homogeneous, isotropic turbulence
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09:00 - 10:00
The physics of early galaxy formation
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09:00
The physics of early galaxy formation
1h0'
Speaker: Andrea Ferrara (S.I.S.S.A., Trieste, Italy) Material: lecture notes
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09:00
The physics of early galaxy formation
1h0'
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10:00 - 11:00
The fundamental importance of cooling flows for galaxy formation
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10:00
The fundamental importance of cooling flows for galaxy formation
1h0'
Speaker: Pierluigi Monaco Material: lecture notes
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10:00
The fundamental importance of cooling flows for galaxy formation
1h0'
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11:00 - 11:30
Coffee Break
- 11:00 Coffee Break 30'
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11:30 - 12:30
History and dynamics of the intergalactic medium
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11:30
History and dynamics of the intergalactic medium
1h0'
Speaker: Ue-Li Pen (Canadian Institute for Theoretical Astrophysics, Toronto, Canada) Material: lecture notes
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11:30
History and dynamics of the intergalactic medium
1h0'
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12:30 - 14:00
Lunch Break
- 12:30 Lunch Break 1h30'
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14:00 - 15:00
Galactic outflows and the IGM
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14:00
Galactic outflows and the IGM
1h0'
Speaker: Kandaswamy Subramanian (IUCAA, Pune, India) Material: lecture notes
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14:00
Galactic outflows and the IGM
1h0'
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15:00 - 16:00
Magnetic fields: Implications for cosmology
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15:00
Magnetic fields: Implications for cosmology
1h0'
Speaker: Shiv Sethi (Raman Research Institute, Bangalore, India)
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15:00
Magnetic fields: Implications for cosmology
1h0'
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09:00 - 10:00
The physics of early galaxy formation
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09:00 - 10:30
(1) Accretion flows in astrophysics (1.1) Binary stars (1.2) Active galactic nuclei, quasars; (1.3) Young stellar objects
Tutor: G. Gogoberidze
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09:00
(1) Accretion flows in astrophysics (1.1) Binary stars (1.2) Active galactic nuclei, quasars; (1.3) Young stellar objects
1h30'
Speaker: Instructor: Andria ROGAVA (KU Leuven, Belgium) Material: lecture notes
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09:00
(1) Accretion flows in astrophysics (1.1) Binary stars (1.2) Active galactic nuclei, quasars; (1.3) Young stellar objects
1h30'
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10:30 - 11:00
Coffee Break (Group Photograph will be taken on the Terrace during the break)
- 10:30 Coffee Break (Group Photograph will be taken on the Terrace during the break) 30'
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11:00 - 12:30
Basic equation of MHD (a) magnetic fields in astrophysics: pictures and general stuff; (b) Maxwell equations - Ohms law - induction equation; (c) flux freezing and diffusion of magnetic fields; (d) examples and applications of flux freezing
Tutors: S. Sridhar & S.K. Sethi
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11:00
Basic equation of MHD (a) magnetic fields in astrophysics: pictures and general stuff; (b) Maxwell equations - Ohms law - induction equation; (c) flux freezing and diffusion of magnetic fields; (d) examples and applications of flux freezing
1h30'
Speaker: Instructor: Kandaswamy SUBRAMANIAN (IUCAA, Pune India) Material: lecture notes
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11:00
Basic equation of MHD (a) magnetic fields in astrophysics: pictures and general stuff; (b) Maxwell equations - Ohms law - induction equation; (c) flux freezing and diffusion of magnetic fields; (d) examples and applications of flux freezing
1h30'
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12:30 - 14:00
Lunch Break
- 12:30 Lunch Break 1h30'
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14:00 - 15:30
Nonlinear scalar equation: (1) Burger's equation; (2) shocks and rarefactions
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14:00
Nonlinear scalar equation: (1) Burger's equation; (2) shocks and rarefactions
1h30'
Speaker: Instructors: Silvano MASSAGLIA & Andrea MIGNONE Material: lecture notes
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14:00
Nonlinear scalar equation: (1) Burger's equation; (2) shocks and rarefactions
1h30'
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15:30 - 15:45
Coffee Break
- 15:30 Coffee Break 15'
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15:45 - 17:00
Euler equations: (1) characteristics, Riemann problem; (2) exact and approximate solution; (3) practice session (Sod shock tube) with PLUTO; (4) extension to multidimension; (5) practice session (2-D) with PLUTO
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15:45
Euler equations: (1) characteristics, Riemann problem; (2) exact and approximate solution; (3) practice session (Sod shock tube) with PLUTO; (4) extension to multidimension; (5) practice session (2-D) with PLUTO
1h15'
Speaker: Instructors: Silvano MASSAGLIA & Andrea MIGNONE
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15:45
Euler equations: (1) characteristics, Riemann problem; (2) exact and approximate solution; (3) practice session (Sod shock tube) with PLUTO; (4) extension to multidimension; (5) practice session (2-D) with PLUTO
1h15'
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09:00 - 10:30
(1) Accretion flows in astrophysics (1.1) Binary stars (1.2) Active galactic nuclei, quasars; (1.3) Young stellar objects
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09:00 - 10:30
(2) Spherical accretion (2.1) Collisionless (Zeldovich-Novikov) spherical accretion (2.2) Hydrodynamic (Bondi) spherical accretion
Tutor: G. Gogoberidze
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09:00
(2) Spherical accretion (2.1) Collisionless (Zeldovich-Novikov) spherical accretion (2.2) Hydrodynamic (Bondi) spherical accretion
1h30'
Speaker: Instructor: Andria ROGAVA Material: lecture notes
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09:00
(2) Spherical accretion (2.1) Collisionless (Zeldovich-Novikov) spherical accretion (2.2) Hydrodynamic (Bondi) spherical accretion
1h30'
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10:30 - 11:00
Coffee Break
- 10:30 Coffee Break 30'
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11:00 - 12:30
Basic MHD and MHD waves (a) The Lorentz force and MHD equations; (b) conservation of energy, magnetic helicity; (c) fast/slow and Alfven waves: Elsasser variables
Tutors: S. Sridhar & S.K. Sethi
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11:00
Basic MHD and MHD waves (a) The Lorentz force and MHD equations; (b) conservation of energy, magnetic helicity; (c) fast/slow and Alfven waves: Elsasser variables
1h30'
Speaker: Instructor: Kandaswamy SUBRAMANIAN
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11:00
Basic MHD and MHD waves (a) The Lorentz force and MHD equations; (b) conservation of energy, magnetic helicity; (c) fast/slow and Alfven waves: Elsasser variables
1h30'
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12:30 - 14:00
Lunch Break
- 12:30 Lunch Break 1h30'
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14:00 - 15:30
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14:00
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1h30'
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14:00
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1h30'
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15:30 - 15:45
Coffee Break
- 15:30 Coffee Break 15'
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15:45 - 17:00
Guideline for the problems
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15:45
Guideline for the problems
1h15'
Speaker: Grigol GOGOBERIDZE (KU Leuven, Belgium) Material: lecture notes
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15:45
Guideline for the problems
1h15'
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09:00 - 10:30
(2) Spherical accretion (2.1) Collisionless (Zeldovich-Novikov) spherical accretion (2.2) Hydrodynamic (Bondi) spherical accretion
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09:00 - 10:30
(3) Nonrelativistic accretion discs (3.1) Basics of disc accretion (3.2) Radiation mechanisms, variability, instabilities
Tutor: G. Gogoberidze
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09:00
(3) Nonrelativistic accretion discs (3.1) Basics of disc accretion (3.2) Radiation mechanisms, variability, instabilities
1h30'
Speaker: Instructor: Andria ROGAVA Material: Detailed Lecture Notes Presentation file
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09:00
(3) Nonrelativistic accretion discs (3.1) Basics of disc accretion (3.2) Radiation mechanisms, variability, instabilities
1h30'
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10:30 - 11:00
Coffee Break
- 10:30 Coffee Break 30'
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11:00 - 12:30
MHD applications (a) magneto rotational instability, dispersion relation for a simple case - estimates of growth rates - effects of damping - boundaries; (b) stationary axi-symmetric MHD flows
Tutors: S. Sridhar & S.K. Sethi
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11:00
MHD applications (a) magneto rotational instability, dispersion relation for a simple case - estimates of growth rates - effects of damping - boundaries; (b) stationary axi-symmetric MHD flows
1h30'
Speaker: Instructor: Kandaswamy SUBRAMANIAN Material: lecture notes
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11:00
MHD applications (a) magneto rotational instability, dispersion relation for a simple case - estimates of growth rates - effects of damping - boundaries; (b) stationary axi-symmetric MHD flows
1h30'
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12:30 - 14:00
Lunch Break
- 12:30 Lunch Break 1h30'
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14:00 - 15:30
Presentations by Participants
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14:00
Presentations by Participants
1h30'
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14:00
Presentations by Participants
1h30'
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15:30 - 15:45
Coffee Break
- 15:30 Coffee Break 15'
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15:45 - 17:00
Presentations by Participants
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15:45
Presentations by Participants
1h15'
-
15:45
Presentations by Participants
1h15'
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09:00 - 10:30
(3) Nonrelativistic accretion discs (3.1) Basics of disc accretion (3.2) Radiation mechanisms, variability, instabilities
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09:00 - 10:30
(4) Relativistic accretion discs (4.1) Basics of Schwarzschild and Kerr metrics (4.2) Stress-energy tensor, conservation equations (4.3) Relativistic (Novikov-Thorne) accretion disc
G. Gogoberidze
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09:00
(4) Relativistic accretion discs (4.1) Basics of Schwarzschild and Kerr metrics (4.2) Stress-energy tensor, conservation equations (4.3) Relativistic (Novikov-Thorne) accretion disc
1h30'
Speaker: Instructor: Andria ROGAVA
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09:00
(4) Relativistic accretion discs (4.1) Basics of Schwarzschild and Kerr metrics (4.2) Stress-energy tensor, conservation equations (4.3) Relativistic (Novikov-Thorne) accretion disc
1h30'
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10:30 - 11:00
Coffee Break
- 10:30 Coffee Break 30'
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11:00 - 12:30
Origin of magnetic fields (a) The generalised Ohm's law; (b) the Biermann battery; (c) Dynamos - mean field dynamo - fluctuation dynamo; (d) application to galaxies and clusters
Tutors: S. Sridhar & S.K. Sethi
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11:00
Origin of magnetic fields (a) The generalised Ohm's law; (b) the Biermann battery; (c) Dynamos - mean field dynamo - fluctuation dynamo; (d) application to galaxies and clusters
1h30'
Speaker: Instructor: Kandaswamy SUBRAMANIAN
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11:00
Origin of magnetic fields (a) The generalised Ohm's law; (b) the Biermann battery; (c) Dynamos - mean field dynamo - fluctuation dynamo; (d) application to galaxies and clusters
1h30'
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12:30 - 14:00
Lunch Break
- 12:30 Lunch Break 1h30'
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14:00 - 15:30
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14:00
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1h30'
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14:00
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1h30'
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15:30 - 15:45
Coffee Break
- 15:30 Coffee Break 15'
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15:45 - 17:00
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15:45
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1h15'
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15:45
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1h15'
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09:00 - 10:30
(4) Relativistic accretion discs (4.1) Basics of Schwarzschild and Kerr metrics (4.2) Stress-energy tensor, conservation equations (4.3) Relativistic (Novikov-Thorne) accretion disc
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09:00 - 09:10
Welcome
- 09:00 Welcome 10'
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09:10 - 10:00
Numerical simulations of the MRI in the shearing box approximation
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09:10
Numerical simulations of the MRI in the shearing box approximation
50'
Speaker: Gianluigi BODO (Osservatorio Astronomico, Torino, Italy) Material: lecture notes
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09:10
Numerical simulations of the MRI in the shearing box approximation
50'
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10:00 - 10:50
Modelling MHD jets and outflows
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10:00
Modelling MHD jets and outflows
50'
Speaker: Kanaris TSINGANOS (University of Athens, Greece) Material: lecture notes
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10:00
Modelling MHD jets and outflows
50'
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10:50 - 11:20
Coffee Break
- 10:50 Coffee Break 30'
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11:20 - 12:10
Modelling accretion-ejection processes in magnetized young star environments
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11:20
Modelling accretion-ejection processes in magnetized young star environments
50'
Speaker: Rony KEPPENS (KU Leuven, Belgium) Material: lecture notes
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11:20
Modelling accretion-ejection processes in magnetized young star environments
50'
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12:10 - 14:30
Lunch Break
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12:10
Lunch Break
2h20'
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12:10
Lunch Break
2h20'
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14:30 - 15:20
Hydrodynamic and spectral properties of accretion and winds around compact objects: a shocking story
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14:30
Hydrodynamic and spectral properties of accretion and winds around compact objects: a shocking story
50'
Speaker: Sandip CHAKRABARTI (S.N. Bose National Centre for Basic Sciences, Kolkata, India) Material: lecture notes
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14:30
Hydrodynamic and spectral properties of accretion and winds around compact objects: a shocking story
50'
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15:20 - 16:10
Poynting jets and MHD winds from disks of rapidly rotating magnetized stars and black holes
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15:20
Poynting jets and MHD winds from disks of rapidly rotating magnetized stars and black holes
50'
Speaker: Richard V.E. LOVELACE (Cornell University, Ithaca, USA) Material: lecture notes
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15:20
Poynting jets and MHD winds from disks of rapidly rotating magnetized stars and black holes
50'
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16:10 - 16:40
Coffee Break
- 16:10 Coffee Break 30'
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16:40 - 17:30
Dynamics and dissipation in poynting flux dominated flows
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16:40
Dynamics and dissipation in poynting flux dominated flows
50'
Speaker: Maxim LYUTIKOV (Purdue University, West Lafayette, USA) Material: recording
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16:40
Dynamics and dissipation in poynting flux dominated flows
50'
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17:30 - 17:40
Concluding remarks
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17:30
Concluding remarks
10'
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17:30
Concluding remarks
10'
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09:00 - 09:10
Welcome