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Physics · Ch 12 — Magnetism

Earth's Magnetism

12.5

Earth's Magnetism

It is common everyday experience that a bar magnet or magnetic needle, suspended freely in air, always aligns itself along the geographic North-South direction; and if it additionally has the freedom to rotate about a horizontal axis, it settles at some fixed angle to the horizontal rather than lying perfectly flat. This behaviour is direct evidence that a magnetic field is present everywhere on (and around) the Earth -- called Terrestrial Magnetism -- and it is precisely this field that makes navigation by compass possible. The Earth's magnetic field lines enter the Earth's surface near its (north) magnetic pole and emerge near its (south) magnetic pole, exactly matching the external field pattern of a bar magnet. Unless stated otherwise, every direction mentioned below (North, South, etc.) is the GEOGRAPHIC direction, not the magnetic one.

The Earth is treated, to a good approximation, as one huge bar magnet. Its magnetic north pole (N) -- the pole where field lines converge, matching a bar magnet's own south-type behaviour -- is located below Antarctica, while its magnetic south pole (S) is located below northern Canada; the straight line NS joining these two poles is called the Earth's magnetic axis, labelled MM'. A great circle lying in the plane perpendicular to this magnetic axis is called the magnetic equatorial circle, labelled AA'; it happens to pass through India close to Thiruvananthapuram (Fig. 12.5).

Two reference planes are needed to describe how the Earth's field is oriented at any particular place. The geographic meridian is the vertical plane, perpendicular to the Earth's surface, that passes through the geographic (rotation) axis -- it defines true geographic north. The magnetic meridian is the vertical plane, also perpendicular to the surface, that instead passes through the Earth's magnetic axis; the direction of the Earth's resultant magnetic field at a place always lies along, or parallel to, this magnetic meridian plane (Fig. 12.6). The angle between the geographic meridian and the magnetic meridian at a place is called the magnetic declination, α\alpha. This declination is small in India: about 0∘58′0^\circ58' west at Mumbai and about 0∘41′0^\circ41' east at Delhi, so a compass at either city already shows very close to true north.

Within the magnetic meridian plane at a place, the Earth's resultant field B⃗\vec B generally makes some angle with the horizontal, called the magnetic inclination or angle of dip, ϕ\phi (Fig. 12.7). Resolving B⃗\vec B into a horizontal component BHB_H and a vertical component BVB_V gives BH=Bcos⁡ϕB_H=B\cos\phi and BV=Bsin⁡ϕB_V=B\sin\phi; the vertical component is comparatively easy to measure directly. From these, tan⁡ϕ=BVBH\tan\phi=\dfrac{B_V}{B_H} (Eq. 12.10) and B=BH2+BV2B=\sqrt{B_H^2+B_V^2} (Eq. 12.11). Three special cases follow directly: (1) at the magnetic north pole, B=BVB=B_V (directed straight upward), BH=0B_H=0, and ϕ=90∘\phi=90^\circ; (2) at the magnetic south pole, B=BVB=B_V (directed straight downward), BH=0B_H=0, and ϕ=270∘\phi=270^\circ; (3) anywhere on the magnetic (great-circle) equator, B=BHB=B_H (directed from geographic South to North), BV=0B_V=0, and ϕ=0∘\phi=0^\circ.

Because the horizontal component BHB_H, the declination α\alpha, and the dip ϕ\phi all vary from place to place (and slowly with time, as the Earth's own magnetic poles drift), magnetic maps -- drawn by joining places that share the same value of a given magnetic element -- are essential for accurate navigation. These are called iso-magnetic charts: lines joining places of equal horizontal component BHB_H are Isodynamic lines; lines joining places of equal declination α\alpha are Isogonic lines; and lines joining places of equal inclination (dip) ϕ\phi are Aclinic lines. …

Figure 12.5Fig. 12.5: Earth's magnetism

What this figure shows. The Earth is drawn as a sphere behaving like a giant embedded bar magnet. Its magnetic north pole (N) is marked below Antarctica and its magnetic south pole (S) is marked below northern Canada, with the straight line NS joining them labelled as the magnetic axis MM'. A great circle around the Earth, perpendicular to this magnetic axis, is drawn and labelled AA', the magnetic equator, shown passing through India near Thiruvananthapuram. Field lines are shown emerging from the Earth's magnetic south pole region and curving around to enter at the magne …

Figure 12.6Fig. 12.6: Magnetic declination

What this figure shows. At a point on the Earth's surface, two vertical planes are drawn intersecting along the local vertical: the geographic meridian plane (containing the geographic/rotation axis, defining true north) and the magnetic meridian plane (containing the Earth's magnetic axis, along which the local resultant magnetic field lies). The angle between these two planes, measured at the point, is marked as the declination α\alpha. A compass needle aligned along the magnetic meridian is shown offset from the true-north direction …

Figure 12.7Fig. 12.7: Magnetic inclination (angle of dip)

What this figure shows. Within the vertical magnetic-meridian plane at a place, the Earth's resultant magnetic field vector B⃗\vec B is drawn tilted below (or above) the horizontal. The horizontal line is marked, and the field vector B⃗\vec B makes an angle ϕ\phi with it -- the angle of dip. The field is resolved into a horizontal component BH=Bcos⁡ϕB_H=B\cos\phi, drawn along the horizontal line, and a vertical component BV=Bsin⁡ϕB_V=B\sin\phi, drawn perpendicular to it, with the two components and the resultant BB forming a right triangle …

Misc Ex.2Example 12.2: Earth's magnetic dipole moment from its equatorial field

Worked out. Earth's magnetic field at the equator is given as Beq=4×10−5B_{eq}=4\times10^{-5} T at radius r=6.4×106r=6.4\times10^6 m, modelling Earth as a bar magnet. Using the equatorial-field formula Beq=μ04πmr3B_{eq}=\dfrac{\mu_0}{4\pi}\dfrac{m}{r^3}, solved for mm: m=Beqr3μ0/4π=(4×10−5)×(6.4×106)310−7≈1.05×1023m=\dfrac{B_{eq}r^3}{\mu_0/4\pi}=\dfrac{(4\times10^{-5})\times(6.4\times10^6)^3}{10^{-7}}\approx1.05\times10^{23} A m2^2, matching the accepted order of magnitude of the Earth's real magnetic dipole moment. …

Misc Ex.3Example 12.3: Neutral points of a bar magnet placed against Earth's horizontal field

Worked out. A bar magnet of magnetic moment mm is placed horizontally, with two neutral points P and Q (where the magnet's own field exactly cancels the horizontal component BHB_H of the Earth's field) located on its equatorial line -- i.e. their position vectors make angles of 90∘90^\circ and 270∘270^\circ with the direction of mm. Since the equatorial field is anti-parallel to mm, equating its magnitude to BHB_H at r=1r=1 m with BH=3.5×10−5B_H=3.5\times10^{-5} T gives m=BHr3μ0/4π=3.5×10−5×1310−7=350m=\dfrac{B_Hr^3}{\mu_0/4\pi}=\dfrac{3.5\times10^{-5}\times1^3}{10^{-7}}=350 A m$^ …