3.4 Earth’s Magnetic Field

Heat transferred from the solid inner core to the liquid outer core leads to convection of the liquid iron of the outer core. Because iron is a metal and conducts electricity (even when molten), its motion generates a magnetic field.

Earth’s magnetic field is defined by the north and south poles that align generally with the axis of rotation (Figure 3.15). The lines of magnetic force flow into Earth in the northern hemisphere and out of Earth in the southern hemisphere. Because of the shape of the field lines, the magnetic force trends at different angles to the surface in different locations (red arrows of Figure 3.15). At the north and south poles, the force is vertical. Anywhere on the equator the force is horizontal, and everywhere in between, the magnetic force is at some intermediate angle to the surface. As we’ll see in Chapter 4, the variations in these orientations provide a critical piece of evidence to the understanding of continental drift as an aspect of plate tectonics.

Depiction of Earth’s magnetic field as a bar magnet coinciding with the core. The south pole of such a magnet points to Earth’s North Pole. The red arrows represent the orientation of the magnetic field at various locations on Earth’s surface. [SE after TStein CC-BY-SA http://bit.ly/1PPSov7]

Figure 3.15 Depiction of Earth’s magnetic field as a bar magnet coinciding with the core. The south pole of such a magnet points to Earth’s North Pole. The red arrows represent the orientation of the magnetic field at various locations on Earth’s surface. [Steven Earle after TStein CC-BY-SA http://bit.ly/1PPSov7]

Earth’s magnetic field is generated within the outer core by the convective movement of liquid iron, but the magnetic field is not stable over geological time. For reasons that are not completely understood, the magnetic field decays periodically and then becomes re-established. When it does re-establish, the polarity may have reversed (i.e., your compass would point south rather than north). Over the past 250 Ma, there have a few hundred magnetic field reversals, and their timing has been anything but regular. The shortest ones that geologists have been able to define lasted only a few thousand years, and the longest one was more than 30 million years, during the Cretaceous (Figure 3.16).

Magnetic field reversal chronology for the past 170 Ma. Black stripes mark times when the magnetic field was oriented the same as today. [SE after AnomieX, Public Domain http://bit.ly/1mENqWY]

Figure 3.16 Magnetic field reversal chronology for the past 170 Ma. Black stripes mark times when the magnetic field was oriented the same as today. [Steven Earle after AnomieX, Public Domain http://bit.ly/1mENqWY]

 

Exercise 3.3 What Does Your Magnetic Dip Meter Tell You?

Regular compasses point only to the north magnetic pole, but if you have a magnetic dip meter (or an iPhone with the appropriate app*), you could also measure the angle of the magnetic field at your location in the up-and-down sense. You don’t need to get the app (or an iPhone) to do this exercise!

Using Figure 3.15 as a guide, describe where you’d be on Earth if the vertical angles are as follows:

Vertical orientation General location Vertical orientation General location
Straight down Up at a shallow angle
Down at a steep angle Parallel to the ground

*See the magnetic inclination app at: http://www.hotto.de/mobileapps/iphonemagneticinclinationmeter.html

Changes in Earth’s magnetic field have been studied using a mathematical model which simulates convection in the outer core.  Reversals happened when the model was run to simulate a period of several hundred thousand years.  According to the lead author of the study, Gary Glatzmaier, of University of California Santa Cruz: “Our solution shows how convection in the fluid outer core is continually trying to reverse the field but that the solid inner core inhibits magnetic reversals because the field in the inner core can only change on the much longer time scale of diffusion. Only once in many attempts is a reversal successful, which is probably the reason why the times between reversals of the Earth’s field are long and randomly distributed.” A depiction of Earth’s magnetic field lines during a stable period and during a reversal is shown in Figure 3.17. To read more about these phenomena see Glatzmaier’s Geodynamo website at: http://es.ucsc.edu/~glatz/geodynamo.html.

Earth’s magnetic field between reversals (left) and during a reversal (right). The lines represent magnetic field lines: blue where the field points toward Earth’s centre and yellow where it points away. The rotation axis of Earth is vertical, and the outline of the core is shown as a dashed white circle. [NASA, Public Domain http://bit.ly/1kOQrC9]

Figure 3.17 Earth’s magnetic field between reversals (left) and during a reversal (right). The lines represent magnetic field lines: blue where the field points toward Earth’s centre and yellow where it points away. The rotation axis of Earth is vertical, and the outline of the core is shown as a dashed white circle. [NASA, Public Domain http://bit.ly/1kOQrC9]