free physics video tutorials for all

 

 

Fields & Effects

 

Magnetic Fields 1

 

flux φ

flux density B

magnetic field straight wire

B straight wire

B solenoid

Helmholtz coils

 

 

fast revision: Magnetic field lines follow the direction of a free moving North Pole.

direction of a magnetic line of force

Magnetic Flux φ (phi)

By definition, magnetic flux is a measure of the strength of a magnetic field over a given area perpendicular to it.

The diagram below shows how the magnetic flux φ over an area A varies around the pole of a magnet.

magnetic flux around a magnet

 

back to top

 

Flux Density B

We can refine the idea of flux by making the area unity (1m2). This introduces a new concept - magnetic flux density B .

flux related to flux density

For normal area (area at right angles),

total magnetic flux = flux density x area

flux related to  flux density - equation #1

Units

The unit of flux is the Weber (Wb) and the unit of flux density is the Tesla (T).

A flux density of 1 Tesla is 1 Weber per square metre.

1 T = 1 Wbm-2

For an area A at an angle θ to the magnetic field, normal flux density has magnitude Bcosθ .

 

magnetic flux density and area

 

So the total normal flux over an area A at an angle θ to the field is given by :

magnetic flux

 

back to top

 

Magnetic fields around current-carrying conductors

The magnetic field around a current-carrying wire is a series of concentric field lines. The field is not uniform. The lines are not evenly spaced. The field is non-uniform, with lines tightly packed close to the wire and widely spaced away from it.

magnetic field around a straight wire

The direction of the lines of force is clockwise in the direction of the current direction.

The field around a plane circular coil resembles the field around a short bar magnet.

magnetic field around a single coil

 

The field around a solenoid resembles the field around a long bar magnet.

magnetic field around a solenoid

 

back to top

 

Flux density for a straight wire

The diagram below illustrates the flux density B at a point P a distance a away from the wire.

B for a straight wire

The magnetic flux density B is described by the equation :

long wire flux density equation

where μo is the permeability of free space.

Unfortunatel a full derivation of this equation cannot be given at present.

 

back to top

 

Flux density for an infinitely long solenoid

The diagram illustrates the flux density B in a solenoid with n turns and coil current I.

B for an infintely long solenoid

The magnetic flux density B is described by the equation :

flux density for a solenoid

where μo is the permeability of free space and n is the number of turns per unit length of the solenoid.

The value of B approximates to that of a real solenoid provided the solenoid's length is at least x10 its diameter.

The quantity nI is of significance. It is equal to the magnetic field strength H , with units of amp-turns/metre (Am-2) .
note: turns n has no units

field strength H in terms of turns and current - equation #1

 

back to top

 

Uniform magnetic fields - Helmholtz Coils

A single plane coil of radius r , turns N and current I produces magnetic flux density B at its centre.

B for a plane circular coil

flux density for a plane circular coil

where μo is the permeability of free space.

Helmholtz Coils produce a region of uniform magnetic field within a discrete volume. Two identical plane coils are aligned along a common axis and positioned a distance r apart, where r is the coil radius.

Helmholtz coils - diagram #1      

The current I passing through each coil is the same and in the same direction.

 helmholtz coils - diagram #2 

The magnetic flux density B in the volume of uniform field (shaded green) is given by :

Helmholtz coil equation

where μo is the permeability of free space.

Helmholtz coils are particularly useful for deflecting electron/ion beams. All charged particles follow a circular path when injected into a magnetic field at right angles to their motion. By measuring the radius of a path and whether the path is clockwise or anticlockwise, important information can be gleaned on the charge of a particle and its mass.

This method is particularly important in distinguishing α , β and γ particles from each other.

 

back to top

 

 

 

this week's promoted video

 

 from Physics Trek

 

 

creative commons license

All downloads are covered by a Creative Commons License.
These are free to download and to share with others provided credit is shown.
Files cannot be altered in any way.
Under no circumstances is content to be used for commercial gain.

 

 

 

 

©copyright a-levelphysicstutor.com 2024 - All Rights Reserved