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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

 

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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

 

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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

 

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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.

 

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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

 

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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.

 

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