Through analysis of seafloor magnetic anomalies and dating of reversal sequences on land, paleomagnetists have been developing a
Geomagnetic Polarity Time Scale. The current time scale contains 184 polarity intervals in the last 83million years (and therefore 183 reversals). and the Kiaman Superchron. A third candidate, the Moyero Superchron, is more controversial. The Jurassic Quiet Zone in ocean magnetic anomalies was once thought to represent a superchron but is now attributed to other causes. The
Cretaceous Normal Superchron (also called the
Cretaceous Superchron or C34) lasted for 37million years, from about , including stages of the
Cretaceous period from the
Aptian through the
Santonian. The frequency of magnetic reversals steadily decreased prior to the period, reaching its low point (no reversals) during the period. Between the Cretaceous Normal and the present, the frequency has generally increased slowly. The
Kiaman Reverse Superchron lasted from approximately the late
Carboniferous to the late
Permian, or for more than 50million years, from around . The magnetic field had reversed polarity. The name "Kiaman" derives from the Australian town of
Kiama, where some of the first geological evidence of the superchron was found in 1925. The
Ordovician is suspected to have hosted another superchron, called the
Moyero Reverse Superchron, lasting more than 20million years (485 to 463million years ago). Thus far, this possible superchron has only been found in the Moyero river section north of the polar circle in Siberia. Moreover, the best data from elsewhere in the world do not show evidence for this superchron. Certain regions of ocean floor, older than , have low-amplitude magnetic anomalies that are hard to interpret. They are found off the east coast of North America, the northwest coast of Africa, and the western Pacific. They were once thought to represent a superchron called the
Jurassic Quiet Zone, but magnetic anomalies are found on land during this period. The geomagnetic field is known to have low intensity between about and , and these sections of ocean floor are especially deep, causing the geomagnetic signal to be attenuated between the seabed and the surface.
Statistical properties Several studies have analyzed the statistical properties of reversals in the hope of learning something about their underlying mechanism. The discriminating power of statistical tests is limited by the small number of polarity intervals. Nevertheless, some general features are well established. In particular, the pattern of reversals is random. There is no correlation between the lengths of polarity intervals. There is no preference for either normal or reversed polarity, and no statistical difference between the distributions of these polarities. This lack of bias is also a robust prediction of
dynamo theory. There is no
rate of reversals, as they are statistically random. The randomness of the reversals is inconsistent with periodicity, but several authors have claimed to find periodicity. However, these results are probably artifacts of an analysis using sliding windows to attempt to determine reversal rates. Most statistical models of reversals have analyzed them in terms of a
Poisson process or other kinds of
renewal process. A Poisson process would have, on average, a constant reversal rate, so it is common to use a non-stationary Poisson process. However, compared to a Poisson process, there is a reduced probability of reversal for tens of thousands of years after a reversal. This could be due to an inhibition in the underlying mechanism, or it could just mean that some shorter polarity intervals have been missed. A random reversal pattern with inhibition can be represented by a
gamma process. In 2006, a team of physicists at the
University of Calabria found that the reversals also conform to a
Lévy distribution, which describes
stochastic processes with long-ranging correlations between events in time. The data are also consistent with a deterministic, but chaotic, process. ==Character of transitions==