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By the end of this topic, you should be able to:
Imagine a magnetic field made up of invisible lines flowing through space — we call these magnetic field lines. Now imagine holding a flat loop of wire in that field. Some of those field lines will pass through the area of the loop.
Magnetic flux (symbol: Φ, the Greek letter "phi") is a measure of how many magnetic field lines pass through a given area. More precisely:
Magnetic flux is defined as the product of the magnetic flux density and the cross-sectional area that is perpendicular (at right angles) to the direction of the magnetic field.
Φ=BA
| Symbol | Quantity | Unit |
|---|---|---|
| Φ | Magnetic flux | Weber (Wb) |
| B | Magnetic flux density | Tesla (T) |
| A | Cross-sectional area | m² |
The amount of flux through an area depends on the angle between the field lines and the surface:
Think of it like rain falling on an umbrella. If you hold the umbrella flat (horizontal), all the rain hits it — maximum. If you tilt it completely sideways (vertical), no rain hits it — zero.
If the magnetic field lines are not perfectly perpendicular to the area, you must take the component of B that is perpendicular. The formula becomes:
Φ=BAcosθ
where θ is the angle between the magnetic field lines and the normal to the area (the normal is an imaginary line drawn at right angles to the surface).
Examiner Tip: Be careful — θ is measured from the normal line (perpendicular to the surface), NOT from the surface itself. If a question tells you the angle between the field and the surface, subtract it from 90° to get θ.
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