Course11510612465 lectures
Fluid Dynamics for Astrophysics
Prof. Prasad Subramanian · IISER Pune
Lectures
Week 1
- Introduction to the course
- Continuum hypothesis, distribution function and stress-viscosity relation
- Continuum hypothesis, distribution function and stress-viscosity relation - Recap
- Fluid Kinematics
- Fluid Kinematics - Recap
Week 2
- Conservation laws: Mass conservation and incomprehensibility
- Conservation laws: Momentum conservation and Euler equation
- Conservation laws - Recap
- Potential flows
- Bernoulli constant, its applications and voracity equation
Week 3
- Recap - Potential flows, Bernoulli constant and its applications
- Voracity dynamics -- Kelvin's voracity theorem and Magus effect
- Navier-Stokes equation
- Navier-Stokes equation (contd.) and energy equation
- Energy equation in a conservative form
- Boundary conditions in Navier-Stokes equation, d'Alembert's paradox
- Poiseuille flow, deriving viscosity from microscopics
Week 4
- Dimensionless numbers -- Mach number, Reynolds number
- DimDimensionless numbers contd -- plasma beta, magnetic Reynolds number, Alfven Mach number, Prandl numberensionless numbers -- Mach number, Reynolds number
- Reynolds number and dynamic similarity
- Reynolds number recap, Low Re flows, and drag on a sphere (Stokes law)
- High Re flows -- turbulent drag law, vortex shedding and drag crisis
Week 5
- Lift on a body, introduction to compressible flows
- Compressible flows -- derivation of sound speed and dispersion relation
- Subsonic and supersonic flows
- Propagation of sonic information, shock tube problem and piston problem
- Criterion for neglect of compressibility, method of characteristics
Week 6
- Shock thickness
- Shock thickness recap, shock jump conditions
- Shock jump conditions (contd), transonic 1D flows, converging/diverging channels
- Coverging/diverging channels, de Laval nozzle and its application to astrophysical jets
- Spherically symmetric transonic flows
- Spherically symmetric transonic flows (contd)
Week 7
- Solar wind : Parker's solution
- Solar wind : Modifications in Parker's solution
- Spherical accretion onto a compact object : Eddington luminosity and accretion rate
- Spherical accretion onto a compact object : Solutions for flow properties
- Spherical accretion (contd), disk accretion--Roche lobe overflow
Week 8
- Disk accretion : Mass conservation and vertical hydrostatic equilibrium
- Disk accretion : Removal of angular momentum, Shakura-Sunyaev viscosity parameter
- Disk accretion : Viscous dissipation and the energy equation, two-temperature criterion
- Particle acceleration in astrophysical settings : Shocks and non-thermal energy distribution
- Particle acceleration in astrophysical settings : Diffusive shock acceleration
Week 9
- Spherical blast waves : Bomb explosion and supernova explosion
- Spherical blast waves : Sedov-Taylor solution
- Spherical blast waves : Sedov-Taylor solution (contd.)
- Magnetohydrodynamics (MHD) : Introduction
- Magnetohydrodynamics (MHD) : The induction equation
Week 10
- Magnetohydrodynamics (MHD) : Currents in MHD, momentum equation and magnetic stress tensor
- Magnetohydrodynamics (MHD) : Magnetic stresses and magnetic buoyancy
- Magnetohydrodynamics (MHD) : Plasma beta, force-free fields and potential configurations
- Magnetohydrodynamics (MHD) : Magnetic flux-freezing
- Magnetohydrodynamics (MHD) : Magnetic flux-freezing (contd.), magnetic dynamos
- Magnetohydrodynamics (MHD) : Dynamo theory
Week 11
- Magnetohydrodynamics (MHD) : Waves in MHD - Alfven waves
- Magnetohydrodynamics (MHD) : Waves in MHD - Alfven waves and magnetosonic waves
- Magnetohydrodynamics (MHD) : Waves in MHD - Magnetosonic waves
- Magnetohydrodynamics (MHD) : Shocks in MHD
- Magnetohydrodynamics (MHD) : Shocks in MHD - Shock jump conditions
Week 12
- Non-ideal MHD : Introduction to magnetic reconnection
- Non-ideal MHD : Magnetic reconnection - The Sweet-Parker model
- Non-ideal MHD : Magnetic reconnection - The Petscheck model
- Sun's atmosphere : Solar corona and the coronal heating problem
- Solar eruptions : Coronal Mass Ejections (CMEs) and solar flares
Live Session
Syllabus and materials
At NPTEL, as the course publishes them.
Credits and licence
- Institution
- IISER Pune
- Department
- Physics
- Teacher
- Prof. Prasad Subramanian
- Level
- Undergraduate
- Language
- English
- Subjects
- Physics
- Source
- NPTEL
- Licence
- CC BY-NC-SA, as NPTEL states it. Non-commercial use only. NPTEL's terms
- Attribution
- NPTEL states: "Distributed under Creative Commons Attribution-ShareAlike / CC BY - NC - SA", beside a BY-NC-SA badge. Coordinated by IIT Madras.
- Who can watch
- NPTEL gives no rating. Invisible Network shows it to Teens profiles and older, judged from what the source says about it. How courses are placed
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