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Appendix B: Plots Useful in Paleomagnetism

Scripps Institution of Oceanography, UC San Diego

B.1Equal area projections

B.1.1Calculation of an equal area projection

Cross-section of a sphere showing projection geometry with point P at declination D and inclination I, and the resulting equal area net with point P plotted.

Figure B.1:Construction of an equal area projection for a point P corresponding to a DD of 40° and an II of 35°. [Figure from Tauxe (1998).]

The principles for how to make an equal area projection are shown in Figure B.1. The point P corresponds to a DD of 40° and II of 35°. DD is measured around the perimeter of the equal area net and II is transformed as follows:

L=Lo(1x3),L=L_o\sqrt{(1-|x_3|)},

where Lo=1/x12+x22L_o = 1/\sqrt{x_1^2+x_2^2}.

Schmidt equal area net with intersecting great circles and small circles forming a grid within a circle, oriented with N at top.

Figure B.2:Schmidt (equal area) net.

Four-step sequence on equal area nets showing how to plot a direction: mark declination, rotate net, count inclination inward, and mark the final point.

Figure B.3:How to use an equal area net (see text).

B.1.2Plotting directions

The principles for plotting directions on an equal area net are shown in Figure B.3. Print out the equal area net provided in Figure B.2. Then poke a thumbtack through the center of the diagram and place a piece of tracing paper over the thumbtack. Mark the top of the stereonet as N and the declination of the direction at DirDir in Figure B.3a. Then rotate the mark around the thumbtack such that the declination is at the top of the diagram (Figure B.3b). Count in from the outer ring the number of degrees equal to the inclination - the grid provided is in 2° intervals. Mark the direction (star in Figure B.3d). In paleomagnetism, the convention is for solid symbols to represent downward directions and open symbols to be up.

B.1.3Bedding-tilt corrections

Performing structural corrections can also be done with an equal area net. If samples have been collected from sites where strata have been tilted by tectonic disturbance, a bedding tilt correction is required to determine the NRM direction with respect to paleohorizontal. Structural attitude of beds at the collecting site (strike and dip, or dip angle and direction) must be determined during the course of field work.

The bedding-tilt correction is accomplished by rotating the NRM direction about the local strike axis by the amount of the dip of the beds. Several examples are shown in Figure B.4, and the reader is strongly encouraged to follow through these examples. An intuitive appreciation of these geometrical operations will prove invaluable in understanding many paleomagnetic techniques and applications.

Print out the equal-area grid provided in Figure B.2. Poke a thumb tack through the center and place a piece of tracing paper over it. The graphical procedure for the bedding-tilt correction is as follows:

  1. Bedding attitude is defined by the down-dip direction (the dip direction) and dip angle. In the example of Figure B.4, the dip direction is 40° and dip angle is 20°. The azimuth of bedding strike (orthogonal to down-dip direction) is defined as 90° anti-clockwise from dip direction (310° in the example of Figure B.4).

Equal area projection showing bedding-tilt correction with strike at 310 degrees, dip direction at 40 degrees, and in situ and corrected NRM directions connected by an arrow.

Figure B.4:Example of structural corrections to NRM directions. The bedding attitude is specified by dip and dip direction (squares on the equal-area projections); the azimuth of the strike is 90° anti-clockwise from the dip direction; the rotation required to restore the bedding to horizontal is clockwise (as viewed along the strike line) by the dip angle and is shown by the rotation symbol; the in situ NRM direction is at the tail of the arrow, and the structurally corrected NRM direction is at the head of the arrow.

  1. Put the dip direction/dip angle and the paleomagnetic direction on the equal area net as described in Section B.1.2. These should look like the red square and circle respectively in Figure B.4. Now mark the strike direction as shown in Figure B.4. Rotate the equal-area grid such that the strike is at the top of the grid (you can also put it at the bottom or on either side).

  2. The NRM direction is rotated clockwise about the strike azimuth (along a small circle) by an angle equaling the dip angle. In practice, this means that you count degrees from the circle toward the outer rim along the nearest small circle by the amount of the dip direction. If you reach the outer rim, just “walk back” in toward the center and keep counting. Plot a new circle (the blue one) at that point. If you reached the outer rim and continued back toward the center, this is a negative inclination (upward pointing) and you should use an open symbol.

  3. Following this rotation, the in situ direction can be read from the equal-area projection. Rotate the blue dot to the up-down axis and make a mark on the outer rim. The degrees between this mark and the NN marked is the new declination. The number of degrees between the blue circle and the outer rim is the new inclination. For the example of Figure B.4, the in situ direction is II = 50°, DD = 70° and the direction corrected for bedding tilt is II = 32°; DD = 62°.

B.1.4Reading ternary diagrams

Ternary diagrams are triangles with the three corners representing a composition (e.g., A, B, C or Fe, FeO, Fe2_2O3_3). In Figure B.5a we show only the A component. To get the percentage of this component, we count up from the base of the triangle and find that the star is 60% of the way toward the apex, indicating that the compound is 60% A in composition. The percentage of composition B is shown in Figure B.5b (15%) and similarly C is shown in Figure B.5c (25%).

Three ternary diagrams with a star plotted at the same position, each highlighting how to read one component: a) 60% A, b) 15% B, c) 25% C.

Figure B.5:How to read a ternary diagram. The three apices are components A, B, C. A composition is plotted as the star. a) Shows the percentage of component A (60%). b) Shows the percentage of component B (15%) and c) shows the percentage of component C (25%).

B.1.5Quantile-Quantile plots

When does a data set conform to a particular distribution? One way to assess this is through the use of Quantile-quantile, or Q-Q, plots (see Fisher et al. (1987) for a more complete discussion). In a Q-Q plot, data are graphed against the value expected from a particular distribution. The data ζi\zeta_i are plotted against a value ziz_i that is expected from the distribution; data compatible with the chosen distribution plot along a line. First, we will develop the Q-Q plot for the uniform and exponential functions required for a Fisher distribution. Then we will explain how to make a Q-Q plot for a normal distribution.

Three panels illustrating Q-Q plot construction: a) density curve divided into areas by sorted data, b) theoretical quantiles dividing the distribution into equal areas, c) resulting Q-Q plot of data versus theoretical quantiles.

Figure B.6:a) Illustration of how the sorted data ζi\zeta_i divide the density curve into areas AiA_i with an average area of 1/(N+1)1/(N+1). b) The values of ziz_i which divide the density function into equal areas ai=1/(N+1)a_i=1/(N+1). c) Q-Q plot of zz and ζ\zeta. [Figure from Tauxe (1998).]

B.1.5.1Q-Q plots for Fisher distributions

In order to make Q-Q plot for Fisher distributions, we proceed as follows (Figure B.6):

  1. Sort the variable of interest ζi\zeta_i into ascending order so that ζ1\zeta_1 is the smallest and ζN\zeta_N is the largest.

  2. If the data are represented by the underlying density function as in Figure B.6a, then the ζi\zeta_i’s divide the curve into (N+1)(N+1) areas, AiA_i, the average value of which is a=1/(N+1)a=1/(N+1). If we assume a form for the density function of ζi\zeta_i, we can calculate numbers ziz_i, that divide the theoretical distribution into areas aia_i each having an area aa (see Figure B.6b).

  3. An approximate test for whether the data ζi\zeta_i are fit by a given distribution is to plot the pairs of points (ζi,zi\zeta_i, z_i), as shown in Figure B.6c. If the assumed distribution is appropriate, the data will plot as a straight line.

  4. The density function PP is the distribution function FF times the area, as mentioned before. The ziz_i are calculated as follows:

F(zi)=(i12)/n, where i=1,,n,F(z_i)=(i-\frac{1}{2})/n, \text{ where } i=1,\dots,n,

so that:

zi=F1((i12)/n), where i=1,,n,z_i=F^{-1}((i-\frac{1}{2})/n), \text{ where } i=1,\dots,n,

and where F1F^{-1} is the inverse function to FF. If the data are uniformly distributed (and constrained to lie between 0 and 1), then both F(x)F(x) and F1(x)=xF^{-1}(x) =x. For an exponential distribution F(x)=1exF(x)=1- e^{-x} and F1(x)=ln(1x)F^{-1}(x)=-\text{ln}(1-x).

  1. Finally, we can calculate parameters MuM_u and MeM_e which, when compared to critical values, allow rejection of the hypotheses of uniform and exponential distributions, respectively. To do this, we first calculate:

DN+=maximum[iNF(x)],D_N^+ = \text{maximum} [{i\over N} - F(x)],

and

DN=maximum[F(x)(i1)N].D_N^- = \text{maximum} [F(x) -{{(i-1)}\over N} ].

For a uniform distribution F(x)=xF(x)=x, so MuM_u is calculated by first calculating DN+D_N^+ as the maximum of [i/Nζi][i/N-\zeta_i] and DND_N^- as the maximum of [ζi(i1)/N][\zeta_i-(i-1)/N]. The Kuiper’s statistic VnV_n is DN++DND_N^++D_N^- and MuM_u is given by:

Mu=Vn(N0.567+1.623N),M_u = V_n (\sqrt{N} - 0.567 + {1.623\over{\sqrt{N}}}),

(see Fisher et al. (1987)). A value of Mu>1.207M_u > 1.207 can be grounds for rejecting the hypothesis of uniformity at the 95% level of certainty. Similarly, DN+D_N^+ and DND_N^- can be calculated for the inclination data (using ζi=90Ii\zeta_i=90-I_i) as [i/N(1eζi)][i/N-(1-e^{-\zeta_i})] and maximum of [(1eζi)(i1)/N][(1-e^{-\zeta_i})-(i-1)/N] respectively. The Kolmogorov-Smirnov statistic DnD_n is the largest of the two. The test statistic for exponentially distributed data MeM_e is given by:

Me=(Dn0.2N)(N+0.26+12N).M_e = {(D_n - {0.2 \over{N}})} {( \sqrt N + 0.26 + {1\over {2\sqrt N} } )}.

Values of MeM_e larger than 1.094 allow rejection of the exponential hypothesis at the 95% level of confidence. If either MuM_u or MeM_e exceed the critical values, the hypothesis of a Fisher distribution can be rejected.

B.1.5.2Q-Q plots for normal distributions

In order to calculate the appropriate values for ziz_i assuming a normal distribution (see Abramowitz & Stegun (1970)):

  1. For i=1Ni=1\rightarrow N, calculate p=iN+1p = {i\over {N+1}}.

  2. If p>0.5p>0.5, then q=1pq=1-p; if p<0.5p<0.5, then q=pq=p.

  3. Calculate the following for all p0.5p\ne 0.5:

t=2ln(q),t=\sqrt{-2\ln(q)},

and

u=t(a1+a2t+a3t2)(1+a4t+a5t2+a6t3),u=t-{ {(a_1+a_2t+a_3t^2)}\over { (1 +a_4t+a_5t^2+a_6t^3)}},

where a1=2.515517,a2=0.802853,a3=0.010328,a4=1.432788,a5=0.189269,a6=0.001388a_1=2.515517, a_2=0.802853, a_3=0.010328, a_4=1.432788, a_5=0.189269, a_6=0.001388.

  1. If p>0.5p>0.5, then zi=uz_i=u; if p<0.5p<0.5, then zi=uz_i=-u.

  2. If p=0.5p=0.5, then zi=0z_i=0.

The values of ziz_i calculated in this way for a simulated Gaussian distribution are plotted as the “normal quantile” data and will plot along a line if the data are in fact normally distributed. To test this in a more quantitative way, we can calculate DN+D_N^+ and DND_N^- as follows:

  1. Calculate the mean xˉ\bar x and standard deviation σ\sigma for the data.

  2. Then calculate:

p=xixˉ2σ,p = {{x_i - \bar x}\over {\sqrt 2 \sigma}},

and

q=11+0.3275911x.q = {1\over {1+{0.3275911|x|}}}.
  1. Substitute qq into the following expression (function 7.1.26 from Abramowitz & Stegun (1970)):

erf(q)=1ep2[a1q+a2q2+a3q3+a4q4+a5q5],\text{erf}(q) = 1-e^{-p^2} [ a_1q +a_2q^2 + a_3 q^3 + a_4 q^4+a_5q^5],

where a1=0.254829592,a2=0.284496736,a3=1.421413741a_1=0.254829592, a_2=-0.284496736, a_3=1.421413741, and a5=1.061405429a_5= 1.061405429.

  1. Change the sign of erf(q)\text{erf}(q) such that it has the same sign as qq.

  2. Substitute F(x)=0.5(1+erf(q))F(x)=0.5(1+\text{erf}(q)) into Equation B.4 and Equation B.5 in Section B.1.5 for DN+D_N^+ and DND_N^- respectively. The Kolmogorov-Smirnov parameter DD (e.g., Fisher et al. (1987)) is the larger of DN+D_N^+ or DND_N^-.

  3. The null hypothesis that a given data set is normally distributed can be rejected at the 95% level of confidence if DD exceeds a critical value DcD_c given by 0.886/N0.886/\sqrt{N}.

References
  1. Tauxe, L. (1998). Paleomagnetic Principles and Practice. Kluwer Academic Publishers.
  2. Fisher, N. I., Lewis, T., & Embleton, B. J. J. (1987). Statistical Analysis of Spherical Data. Cambridge University Press. 10.1017/CBO9780511623059
  3. Abramowitz, M., & Stegun, I. A. (Eds.). (1970). Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables (Vol. 55). National Bureau of Standards.