Tutorial 6 B  Hysteresis 

Leaning Objectives 
Distinguish between magnetic field strength and magnetic flux density. To link the quantities with energy by a graphical method. To learn about hysteresis loops. To consider the simple Steinmetz equation. 

Key Questions 
What is the difference between magnetic field strength and magnetic flux density? How can we demonstrate the energy per unit volume? What is hysteresis? How can we work it out? 

Energy in a Magnetic Field by Graphical Method In Alevel Physics, we tend to be rather slack and refer to the flux density as "magnetic field strength". However, in these notes I have been careful to refer to magnetic flux density, because there is another separate quantity called magnetic field strength or magnetising force. You will see this in many articles and textbooks at university level. So what is the difference?
We know the flux density, B, which is defined as the flux (field lines) that pass through a unit area. It is a vector quantity and is the quantity that is most widely used for practical physics and engineering.
The magnetic field strength or magnetic field intensity, H, which is defined as the force experienced by a unit North pole placed in a magnetic field. It is a vector quantity. It represents the force being generated by the source, i.e. the current. When generated magnetic fields pass through magnetic materials, there is a contribution by the material itself. So it's common to make the distinction between the the magnetic flux density and the magnetic field strength.
The initial driver for a magnetic field is an electric current. The current gives a magnetomotive force which is defined as the product between the current and the number of turns. It has the Physics code F_{m} and it's given by a simple formula:
F_{m} = NI
The units are ampturns. Turns are not a dimensional unit, so in unit analysis, the units are amps (A).
Like electromotive force, magnetomotive force NOT a force at all; it's a current.
It is measured in ampereturns, NOT Newton.
The magnetic field strength is the result of the magnetomotive force. The formal definition is as above, but it can also be described as the magnetomotive force per unit length, or the product between the current and the number of turns per unit length. The Physics code is H, and the formula is:
The unit is ampere per metre (A m^{1}). The term l for length is called the length of the flux path.
The magnetic field strength, H, is related to flux density, B, by this simple equation:
If a magnetic material of relative permeability m_{r} is added to make a core, the equation becomes:
If we plot a graph of magnetic flux density against magnetic field strength, we get a straight line through the origin, as the two quantities are are directly proportional.
The gradient is the permeability of free space, m_{0}, which has the value 4p × 10^{7} H m^{1}. The basic SI units for m_{0} (H m^{1}) are kg m s^{2} A^{2}.
If we increase the magnetic field strength by a tiny amount dH, the magnetic flux density increases by a corresponding tiny change in flux density, dB. The shaded area is approximately a rectangle if the increase dH is sufficiently small. The area is: A = (H × dB)
The area represents energy per unit volume. We can demonstrate this by unit analysis.
In basic SI units the Tesla (T) is kg s^{2} A^{1}. So if we multiply the units for dB by H (A m^{1}), we get kg s^{2} A^{1} × A m^{1} which give kg m^{1} s^{2}. The SI basic units for energy (J) are kg m^{2} s^{2}. So if we divide the energy by the volume, we get: kg m^{2} s^{2} ÷ m^{3} = kg m^{1} s^{2}
We can add up all the little rectangles to get the total area under the graph:
So the total energy per unit volume is the area of the triangle:
We know that:
Combining the two equations, we get:
Alternatively we we can say:
And we can therefore write:
Which is where we were before...
The term H for magnetic field strength appears in textbooks and is useful for considering hysteresis which we will do in the next section.


Hysteresis We need to put a certain amount of energy into a magnetic material to magnetise it. This is to line up the domains. Once the domains are lined up, no further energy is required to maintain the magnetic field. The coil will get warm because there is an ohmic resistance.
In some materials the domains remain lined up. In this case we have a permanent magnet. To remove the magnetism (i.e. make the domains go random, we have to apply alternating magnetic fields or heat the magnet up to its Curie Temperature. This is the temperature at which the magnet loses its magnetic properties. For cobalt, it is 1400 K.
For other materials, the domains spring back to their randomly oriented state as soon as the current is turned off. The change in the magnetic field induces an EMF, or a reverse voltage spike. However we do not get that energy back that we put in when we release the magnetic field and the domains return to a random state We get slightly less energy back as the field collapses. Some energy is lost and this lost energy is called hysteresis.
Suppose we have a completely demagnetised material that releases its magnetism when the current stops flowing and start to apply a current with a view to lining up all the domains. We get a graph like this:
When the applied magnetic field strength is low, there is a straight line region which shows proportionality between B and H. Above the limit of proportionality, most of the domains are lined up, and the increase in B is no longer linear. Eventually all the domains are lined up and there can be no increase in flux density. This is saturation.
Now let's reduce the current, and then reverse it. The graph looks like this:
As the current (hence the magnetic field strength) starts to fall at A, the flux density does not retrace the red line to O. Instead it follows the line AB. This is because some of the domains remain lined up. This remaining flux density is called remanence.
A reverse magnetic field has to be applied to make domains realign in the opposite direction, so that the overall flux density is zero. This is shown by OC. The graph follows the line BC. The reverse magnetic field OC is called the coercive force or coercivity.
As the reverse field is increased, shown by line CD more and more domains line up in the opposite direction until all are aligned, and we have saturation in the opposite direction at D.
Remanence has the physics code M_{r} and the units are Tesla, T. Typical value for ferrite is 0.35 T. For a neodymium magnet (a typical permanent magnet) the value for remanence is about 1.3 T.
Typical values for coercive force are: Permalloy (another material for making permanent magnets) 79 A m^{1}; neodymium 900 A m^{1}.
A graph like the one above is often called a hysteresis loop.
Describing Hysteresis Losses When the magnetic field is reversed, the domains are reversed and a job of work needs to be done. This takes energy. We can tell that because the material that is being magnetised starts to get warm. Clearly we cannot get rid of hysteresis entirely, but we can try to minimise it as far as we can.
This is a hysteresis graph of a material like hard steel::
For soft steel, the remanence is high, but the coercivity is low:
Soft steel means magnetically soft, so it loses its magnetism rapidly. It is not soft to touch. It is hard and heavy. If you drop some soft steel on your foot, you will know about it.
Ferrite is a magnetic material made from oxides of iron, cobalt, and nickel, along with oxides of magnesium, aluminium, and manganese. The material is a ceramic. You can see ferrite beads on signal cables for computers. One is shown among the tangle of cables behind a PC.
Its hysteresis loop is very small. It is shown on the graph below:
Quantifying Hysteresis Losses Consider a ring made of a magnetic material of which the circumference is l m (so the radius is l/2p) and its crosssectional area is A m^{2}. It has N turns of wire. Experimental work using a magnetometer gives a hysteresis loop like this:
The magnetic field strength, H, is increased by a tiny amount, dH A m^{1} in a time of dt s. The instantaneous current that gives rise to the magnetic field strength OF is i A. We know that:
So we can write an expression for the instantaneous current as:
We also know that the emf due to the change is:
The power = volts × amps, so we can write an expression for instantaneous power:
The little bit of energy, e, supplied in the time period dt seconds is power × time:
The dt terms obligingly cancel out to give us:
We now bring in the expression for the instantaneous current, i:
to give us:
And we can tidy up the expression to give: e= H_{OF}lAdB
Now the term lA is the volume of the ring. The area of the strip = HOF × dB. So we can say:
energy = area of the shaded strip × volume
Therefore the area of the shaded strip is energy ÷ volume.
If we do this from O to A, we have to add up all the little strips. The energy per unit volume is the area of the shape OABF. If we do it for a whole cycle, the energy per unit volume is the area of the whole loop. If the function that describes the loop were simple, calculus integration would give us the area (i.e. energy per unit volume). However this hysteresis loop does not lend itself to that. Instead we need to estimate the area by counting the squares on the graph paper. If more than half the square is occupied by part of the shape, it is counted in. If less than half is occupied, the square is ignored.
Once we have counted the squares (tedious), we need to work out the area, using the scale. If 1 cm vertically is y Tesla, and 1 cm horizontally is x amps per metre, then the total area A cm^{2} gives the hysteresis loss in joules per cubic metre.
Hysteresis loss (J m^{3}) = A cm^{2} × x A m^{1} cm^{1} × y T cm^{1}
Of course we can count millimetre squares (even more tedious), which will reduce the uncertainty.
The Significance of Hysteresis With a pure direct current a certain amount of energy is lost to build up the magnetic field. Once the magnetic field is established, no energy is needed to maintain the magnetic field, so energy losses are from the resistance of the coil. We know this from: P = I^{2} R If the direct current is a rectified AC the loss is slightly more, as shown in the graph:
The real significance of hysteresis is when we use an alternating current. Consider a coil that gives a hysteresis loop that has an area A. We know that the hysteresis loss is given by:
Hysteresis loss (J m^{3}) = A cm^{2} × x A m^{1} cm^{1} × y T cm^{1}
This the loss per cycle. So if we f cycles per second (Hertz), we can say that the hysteresis loss per second is:
Hysteresis loss per second (J m^{3} s^{1}) = A cm^{2} × x A m^{1} cm^{1} × y T cm^{1} × f Hz
Now energy (J) × frequency (Hz) = power (W). This means that the hysteresis loss per second is actually power per unit volume.
To work the actual power loss, we can modify our equation to:
Power loss (W) = A cm^{2} × x A m^{1} cm^{1} × y T cm^{1} × f Hz × V m^{3}
In our study of hysteresis, we have considered the maximum possible hysteresis, which happens when the magnetic material is taken up to saturation. However if we increase the magnetic field strength such that the resulting flux density is half that of saturation, we find that the hysteresis loss is rather less than half.
So far we have relied on counting squares and scaling up to work out the hysteresis loss per unit volume.
Steinmetz Equation The American mathematician and electrical engineer C P Steinmetz (1865  1923) studied hysteresis losses in transformers and quantified them using the Steinmetz equation.
Suppose our hysteresis loss per cycle is given the physics code Q_{h} J m^{3}. If the maximum flux density is B_{max} T, the Steinmetz theory states that:
The hysteresis loss (J m^{3}) per cycle depends on the magnetic material using a constant k_{h}. The constant k_{h} is called the hysteresis coefficient. So we can write:
We can then work out the power loss per cubic metre (W m^{3}), which we will give the physics code P_{h}.
If we know the volume, V m^{3}, we get an expression for the power loss, P_{m }(W):
This relationship works for simple sinusoidal AC waveforms. For a more complex waveform, a modified version is used. The table shows some typical values for the hysteresis coefficient for typical magnetic materials:
Data from http://www.electricalengineeringassignment.com/hysteresisloss Clearly we want to keep hysteresis losses to a minimum, so it makes sense to use materials that have a low hysteresis coefficient in devices like motors and transformers.
In the equation:
the index (power to) is 1.6. It can vary from 1.6 to 3.0. Many sources give it as 2.


