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The Series Finale of Online Education: Coursera Acquires Udemy

$7.2 billion in combined revenue since 2020. $8 billion in lost market value. This merger marks the end of an era in online education.

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Explore the dynamics of magnetized fluids in plasma physics, astrophysics, and engineering applications. Learn core concepts like general relativistic magnetohydrodynamics, turbulence, and numerical modeling using Python and computational tools. Ideal for beginners on YouTube and Swayam, with a focus on real-world phenomena.

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Kavli Institute for Theoretical Physics
MHD Effects on Thermohaline Mixing in Stars - Adrian Fraser

Explores MHD effects on thermohaline mixing in stellar interiors, discussing recent advances in observational data, 1D models, and 3D simulations to improve understanding of stellar physics.
- YouTube
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International Centre for Theoretical Sciences
Introduction to Numerical Relativistic Hydrodynamics - Lecture 2

Explore advanced concepts in numerical relativistic hydrodynamics, focusing on mathematical formulations and computational techniques for modeling high-energy astrophysical phenomena.
- YouTube
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International Centre for Theoretical Sciences
Introduction to Numerical Relativistic Hydrodynamics - Lecture 5

Explore advanced concepts in numerical relativistic hydrodynamics, focusing on computational techniques for modeling high-energy astrophysical phenomena and gravitational wave sources.
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International Centre for Theoretical Sciences
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Explore modern numerical methods for solving Einstein's equations in computational relativity, essential for modeling gravitational waves from black hole and neutron star mergers.
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Kavli Institute for Theoretical Physics
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Explore polarised properties of magnetised accretion onto black holes, focusing on Sagittarius A* and M87. Learn about magnetic field structures, linear polarization, and future observations in astrophysics.
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Society for Industrial and Applied Mathematics
Magnetohydrodynamic Turbulence - Weak Solutions and Conserved Quantities

Explore magnetohydrodynamic turbulence, weak solutions, and conserved quantities in ideal systems. Analyze the mathematical structures behind Taylor-Woltjer relaxation theory and Faraday systems.
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Explore advanced concepts in numerical relativistic hydrodynamics, focusing on computational techniques for modeling high-energy astrophysical phenomena and gravitational wave sources.
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Center For Computational Relativity and Gravitation
HARM3D and NUC: Numerical Simulations in Relativistic Astrophysics

Explore HARM3D and NUC in relativistic astrophysics, focusing on computational techniques for modeling extreme cosmic events and gravitational phenomena.
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GRaMX: A New GPU-Accelerated Dynamical Spacetime GRMHD Code

Explore GRaMX, a cutting-edge GPU-accelerated dynamical spacetime GRMHD code, and its applications in computational relativity and gravitation.
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Erwin Schrödinger International Institute for Mathematics and Physics (ESI)
Waves and Wind-Driven Flows in the Ocean - Lecture 1

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Waves and Wind-Driven Flows in the Ocean - Lecture 4

Explore Kelvin-Stuart vortices' stability in fluid mechanics, plasma physics, and planetary rings. Analyze nonlinear stability and linear instability for various perturbations.
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Waves and Wind-Driven Flows in the Ocean - Lecture 3

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