Magnetic Fields & Terrestrial Magnetism
Magnetic flux Φ and flux density B = Φ/A (Tesla), magnetic field line geometry, neutral points between interacting fields, and Earth’s magnetic field elements (declination, inclination/dip, horizontal and vertical components).
Marking a lesson complete represents finishing your study of the topic; it does not denote tested mastery.
Learning Objectives
- Define magnetic flux Φ (Weber) and magnetic flux density B (Tesla), solving problems using Φ = B · A cos θ.
- Map magnetic field lines, locate neutral points where the external and local magnetic fields cancel, and explain why field lines form continuous closed loops.
- Define magnetic meridian, geographic meridian, angle of declination, and angle of dip θ, deriving relations B_H = B cos θ, B_V = B sin θ, and tan θ = B_V / B_H.
Core Theory & Concepts
A magnetic field is a region of space around a magnet, electric current, or moving charge where magnetic forces are exerted. The Earth behaves as a giant magnetic dipole tilted roughly 11° from its rotational axis, providing a crucial terrestrial reference field for navigation and scientific instrumentation.
Magnetic Flux & Flux Density
Magnetic flux Φ measures the total field passing through an area: Φ = B · A = B A cos θ. Flux density B represents flux per unit normal area: B = Φ / A.
Earth’s Field Components & Dip Angle
At any point on Earth, the total field B resolves into horizontal component B_H and vertical component B_V: B_H = B cos θ, B_V = B sin θ, tan θ = B_V / B_H.
Common Misconceptions
A magnetic compass needle points towards True Geographic North.
Syllabus Topic Outline
- 1Concept of magnetic poles, field lines, and flux Φ (Weber)
- 2Magnetic flux density B = Φ / A (Tesla, T = Wb m⁻²)
- 3Bar magnets and neutral points in Earth’s magnetic field
- 4Terrestrial magnetism: Geographic vs Magnetic Meridians
- 5Magnetic elements: Declination, Dip (inclination), and components B_H, B_V