Testing the accuracy of our method by numerically stimulating hydrodynamic spherical bondi accretion.

Our numerical scheme utilizes the GRMHD code KHARMA[1], a performance-portable C++ implementation based on iharm3D; iharm3D is itself an extension of HARM.

The dominant outward energy transport mechanism is convection driven by magnetic reconnection in the magnetosphere near the BH.

To investigate the mechanism driving the turbulence, we explore the physics of the outward flow of energy.

The authors HC, RN, PN, KS, AR, and KC acknowledge support from the Gordon and Betty Moore Foundation and the John Templeton Foundation

This study examines near-inertial gravity wave propagation in deep Mediterranean Sea, focusing on transitions between stratified and homogeneous layers.

This study examines near-inertial gravity wave propagation in deep Mediterranean Sea, focusing on transitions between stratified and homogeneous layers.

This study examines near-inertial gravity wave propagation in deep Mediterranean Sea, focusing on transitions between stratified and homogeneous layers.

The vorticity has large variations across the mooring array (Fig. 2a). This is reflected in the NIW observations as large differences in the amplitude.

We begin with a detailed analysis of the simulation results for event 1, which occurred in the fall (Fig. 1c). This event is by far the most energetic NIW event

The authors use the PM model and the YBJ model to simulate the wind stress.

We extract observations of NIWs from data collected for the Ocean Surface Mixing, Ocean Submesoscale Interaction Study

The evolution of wind-generated near-inertial waves (NIWs) is known to be influenced by the mesoscale eddy field, yet it remains a challenge

The YBJ kinetic energy budget may be formed by multiplying (2) by −𝑀∗ /2 and adding the complex conjugate.

The evolution of the NIW field at the OSMOSIS site in the Northeast Atlantic Ocean is strongly modulated by mesoscale eddies.

The study was written by Scott Conn, Joseph Fitzgerald, and Jorn Callies. The authors compared five surface mixed layer models with a year of observations

The no-normal flow condition is imposed by requiring ∇𝑀 = 0 at 𝑧 = 0 (Young and Ben Jelloul 1997), which eliminates the advection and dissipation terms.

A short article about Boltzmann's Brain Theory and the Simulation Hypothesis.

Start your journey into the world of satellite imagery with this beginner's guide. Learn about key satellite programs and data access methods.

11/23/2024: Top 5 stories on the HackerNoon homepage!