Nonlinear Reluctance
Nonlinear reluctance with magnetic hysteresis
Libraries:
Simscape /
Electrical /
Passive
Description
The Nonlinear Reluctance block models linear or nonlinear reluctance with magnetic hysteresis. Use this block to build custom inductances and transformers that exhibit magnetic hysteresis.
The length and area parameters in the Geometry settings let you define the geometry for the part of the magnetic circuit that you are modeling. The block uses the geometry information to map the magnetic domain Through and Across variables to flux density and field strength.
Equations for Linear Reluctance Parameterization
The equations for the linear reluctance parameterization are:
where:
B is the flux density.
μ0 is the permeability in a vacuum.
μr is the relative magnetic permeability.
H is the field strength.
mmf is the magnetomotive force (mmf) across the component.
leff is the effective length of the section being modeled.
φ is magnetic flux.
seff is the effective cross-sectional area of the section being modeled.
Equations for Reluctance with Single Saturation Point Parameterization
This parameterization models a switch-linear reluctance. In the unsaturated state, the material has a specified relative magnetic permeability. In the saturated state, the relative permeability is 𝜇0.
The equations for reluctance with single saturation point are
If .
Otherwise,
where:
mmf is the magnetomotive force (mmf) across the component.
leff is the effective length of the section being modeled.
H is the field strength.
φ is magnetic flux.
seff is the effective cross-sectional area of the section being modeled.
B is the flux density.
Bsat is the flux density at saturation.
Rsat is the magnetic reluctance at saturation.
μ0 is the permeability in a vacuum.
μr is the relative magnetic permeability.
μr_unsat is the unstaurated relative magnetic permeability.
Reluctance (B-H Curve)
For the reluctance (B-H Curve) parameterization, specify the material property by B-H curve.
Equations for Reluctance with Hysteresis Parameterization
The flux density and magnetomotive force equations are:
where:
B is flux density.
φ is magnetic flux.
seff is the effective cross-sectional area of the section being modeled.
mmf is magnetomotive force (mmf) across the component.
leff is the effective length of the section being modeled.
H is field strength.
The block then implements the relationship between B and H according to the Jiles-Atherton [1, 2] equations. The equation that relates B and H to the magnetization of the core is:
where:
μ0 is the magnetic permeability constant.
M is magnetization of the core.
The magnetization acts to increase the magnetic flux density, and its value depends on both the current value and the history of the field strength H. The block uses the Jiles-Atherton equations to determine M at any given time.
The figure below shows a typical plot of the resulting relationship between B and H.
In this case, the magnetization starts as zero, and hence the plot starts at B = H = 0. As the field strength increases, the plot tends to the positive-going hysteresis curve; then on reversal the rate of change of H, it follows the negative-going hysteresis curve. The difference between positive-going and negative-going curves is due to the dependence of M on the trajectory history. Physically the behavior corresponds to magnetic dipoles in the core aligning as the field strength increases, but not then fully recovering to their original position as field strength decreases.
The starting point for the Jiles-Atherton equation is to split the magnetization effect into two parts, one that is purely a function of effective field strength (Heff) and the other an irreversible part that depends on history:
The Man term is called the anhysteretic magnetization because it exhibits no hysteresis. It is described by the following function of the current value of the effective field strength, Heff:
This function defines a saturation curve with limiting values ±Ms and point of saturation determined by the value of a, the anhysteretic shape factor. It can be approximately thought of as describing the average of the two hysteretic curves. In the block interface, you provide values for when Heff = 0 and a point [H1, B1] on the anhysteretic B-H curve, and these are used to determine values for α and Ms.
The parameter c is the coefficient for reversible magnetization, and dictates how much of the behavior is defined by Man and how much by the irreversible term Mirr. The Jiles-Atherton model defines the irreversible term by a partial derivative with respect to field strength:
For , .
For , .
Comparison of this equation with a standard first order differential equation reveals that as increments in field strength, H, are made, the irreversible term Mirr attempts to track the reversible term Man, but with a variable tracking gain of . The tracking error acts to create the hysteresis at the points where δ changes sign. The main parameter that shapes the irreversible characteristic is K, which is called the bulk coupling coefficient. The parameter α is called the inter-domain coupling factor, and is also used to define the effective field strength used when defining the anhysteretic curve:
The value of α affects the shape of the hysteresis curve, larger values acting to increase the B-axis intercepts. However, notice that for stability the term must be positive for δ > 0 and negative for δ < 0. Therefore not all values of α are permissible, a typical maximum value being of the order 1e-3.
You can determine representative parameters for the equation coefficients by using the following procedure:
Provide a value for the Anhysteretic B-H gradient when H is zero parameter (when Heff = 0) plus a data point [H1, B1] on the anhysteretic B-H curve. From these values, the block initialization determines values for α and Ms.
Set the Coefficient for reversible magnetization, c parameter to achieve correct initial B-H gradient when starting a simulation from [H B] = [0 0]. The value of c is approximately the ratio of this initial gradient to the Anhysteretic B-H gradient when H is zero. The value of c must be greater than 0 and less than 1.
Set the Bulk coupling coefficient, K parameter to the approximate magnitude of H when B = 0 on the positive-going hysteresis curve.
Start with α very small, and gradually increase to tune the value of B when crossing H = 0 line. A typical value is in the range of 1e-4 to 1e-3. Values that are too large cause the gradient of the B-H curve to tend to infinity, which is nonphysical and generates a run-time assertion error.
To get a good match against a predefined B-H curve, you may have to iterate on these four steps
Variables
To set the priority and initial target values for the block variables prior to simulation, use the Initial Targets section in the block dialog box or Property Inspector. For more information, see Set Priority and Initial Target for Block Variables.
Nominal values provide a way to specify the expected magnitude of a variable in a model. Using system scaling based on nominal values increases the simulation robustness. Nominal values can come from different sources, one of which is the Nominal Values section in the block dialog box or Property Inspector. For more information, see System Scaling by Nominal Values.
Examples
Ports
Conserving
Parameters
References
[1] Jiles, D. C. and D. L. Atherton. “Theory of ferromagnetic hysteresis.” Journal of Magnetism and Magnetic Materials. Vol. 61, 1986, pp. 48–60.
[2] Jiles, D. C. and D. L. Atherton. “Ferromagnetic hysteresis.” IEEE® Transactions on Magnetics. Vol. 19, No. 5, 1983, pp. 2183–2184.
Extended Capabilities
Version History
Introduced in R2017b