magnetic pressure

"They use magnetic pressure, and we're a big cylinder of metal."

The compression factor is limited by the magnetic pressure in the primary wind.

Magnetic pressure is an energy density associated with a magnetic field.

The magnetic pressure force is readily observed in an unsupported loop of wire.

Magnetic pressure is used to counteract the effects of the gravitational and any other accelerations.

The terms on the right hand side add up to about pR, where p is the larger of the plasma pressure or the magnetic pressure.

In contrast, magnetic tension force is determined by how much the magnetic pressure changes with distance.

"Magnetic pressure we can counter with plasma pressure, right?"

Thus, management of magnetic pressure is a significant challenge in the design of ultrastrong electromagnets.

Focused- Jordin sent, "Seeing some movement in the magnetic pressure zone.

Because of the high magnetic pressure, a high-strength synthetic fiber has to be wound around the wire layers.

Any magnetic field has an associated magnetic pressure contained by the boundary conditions on the field.

Magnetic pressure can also be used to propel projectiles; this is the operating principle of a railgun.

The magnetic pressure of a magnetic field on a superconductor can be calculated by:

Also, excessive magnetic pressure within an ultra-strong electromagnet can cause a magnetic explosion.

This gradient in field strength gives rise to a magnetic pressure force that tends to stretch the wire uniformly outward.

In more intuitive units it's useful to remember that at 1T the magnetic pressure is approximately 4 atmospheres, or kg/cm.

His ankles ached with the memory of slamming into the cosmic string's sheen of magnetic pressures.

Interplay between magnetic pressure and ordinary gas pressure is important to magnetohydrodynamics and plasma physics.

Magnetic pressure should tend to remove field concentrations, causing the sunspots to disperse, but sunspot lifetimes are measured in days or even weeks.

Photon bubbles would develop spontaneously in radiation-dominated atmospheres when the magnetic pressure exceeds the gas pressure.

The magnetic pressure is the energy density of the magnetic field and it increases as magnetic field lines convene with each other.

(b) Towards the bottom, outward kinetic pressures balance inwards magnetic pressure, and the total pressure is constant.

A plasmoid has an internal pressure stemming from both the gas pressure of the plasma and the magnetic pressure of the field.

Tangential discontinuities are discontinuities for which the total pressure (sum of the thermal and magnetic pressures) is conserved.