“…Using the statistical method of Johnson and McGee (1983), the amount of time, Δt, represented by a sampled section can be approximated using the formula Δt (m.y.) = SтN, where S = -ln (1 -2p)/2 (т = mean time span of polarity intervals; N = the number of paleomagnetic sites; and p = R/ [N -l], where R is the number of reversals encountered).…”