A brief description of magnetic circuits with symmetrical, or asymmetrical, parallel parts

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Magnetic Circuits with Symmetrical Parallel Parts

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Consider the symmetrical magnetic circuit diagramed in Figure 1, where the path AB is of length l_1 and area A_1, the path BC is of length l_2 and area A_2, the path CD is of length l_3 and area A_3, and so on.

Figure 1
Figure 1

In this case, we can write that the magnetic flux density for the path AB is:

B_{AB} = \frac{\Phi}{A_1}
(4)

We also consider the number of ampere-turns/meter for the path AB as being AT_{AB}.

Following a similar reasoning, we can write that the magnetic flux density for the path BC is:

B_{BC} = \frac{\Phi}{2A_2}
(5)

while the number of ampere-turns/meter is AT_{BC}.

We can apply the same rationale for the other segments as well. We can thus write that the total number of ampere-turns/meter is:

AT_{AB} l_1 + AT_{BC} l_2 + AT_{CD} l_3 + ...
(6)

As the circuit is symmetrical, it is easy to find out how the magnetic flux divides. For example, in Figure 1 the magnetic flux in the center is twice that in each side.

Magnetic Circuits with Asymmetrical Parallel Parts

Consider the asymmetrical circuit diagramed in Figure 2.

Figure 2
Figure 2

In this case, due to the lack of symmetry, \Phi_1 \neq \Phi_2. There are two methods which allow you to calculate the magnetic flux on each parallel part.

The first method assumes that there is no magnetic saturation. The problem is then worked out by using magnetic permeabilities. For a magnetic circuit as the one diagramed in Figure 3, we obtain that:

\Phi = \frac{NI}{R_1 + \frac{R_2 R_3}{R_2 + R_3}}
(7)

where R is the magnetic reluctance (for a more detailed discussion on the magnetic reluctance see Magnetic Reluctance ).

Figure 3
Figure 3

The second method is more of a trial-and-error method. It first implies dividing up the magnetic flux by hinting the right values, and then calculating \int{H dl} for all paths. These should be equal, and if they are not, then you have to re-adjust the initial division of the magnetic fluxes.