Wednesday, December 22, 2010

Fractal Plate Reconstruction Table 2



Age
(Ma)


2.581


6.033


11.040


19.722


26.154


28.715


31.116


33.738


37.771


Latitude


12.395


11.906


11.049


12.850


13.126


13.039


13.032


13.303


14.622


Longitude


41.738


40.366


37.655


32.877


34.052


34.616


34.722


34.352


32.585


Angle


1.001


4.057


6.781


12.168


15.947


17.272


18.670


20.360


22.499


SAF


I


0.4982


0.5018


0.5242


0.5100


0.4970


0.4840


0.4851


0.4983


0.4887


II


0.4664


0.4408


0.5585


0.5320


0.5254


0.5416


0.5398


0.5177


0.5025


III


0.4652


0.5000


0.5601


0.5414


0.5302


0.5109


0.5007


0.4965


0.4749


IV


0.5002


0.5078


0.5083


0.5279


0.5468


0.5502


0.5437


0.5303


0.5000


V


0.5000


0.5242


0.5000


0.5038


0.5000


0.5000


0.5000


0.5000


0.5000


VI


0.4890


0.4751


0.4907


0.5039


0.5336


0.5030


0.4863


0.4904


0.5000


VII


0.5000


0.4730


0.5000


0.5000


0.5000


0.5000


0.5519


0.5000


0.4654


VIII


0.5000


0.5000


0.5000


0.5000


0.5000


0.5515


0.5343


0.5186


0.5000


IX


0.5000


0.5000


0.5000


0.5000


0.5000


0.5000


0.5109


0.5576


0.5285


X


0.5311


0.5343


0.4991


0.5248


0.5449


0.5526


0.5495


0.5370


0.5000


FZs


0.5000


0.5000


0.5000


0.5000


0.5000


0.5000


0.5000


0.5000


0.5000

Table 2. Final segment rotation parameters and asymmetry factors for magnetic isochron crossing ages, Australian and Antarctic oceanic plates. Partial rotation angle for Antarctic plate to the ridge is the asymmetry factor multiplied by the total rotation angle. For the Australian plate the partial rotation angle to the ridge is (1.0 – the asymmetry factor) multiplied by the total rotation angle. In the absence of data points, asymmetry factor is assumed to be 0.500. 
© 2010 Rex H. Pilger, Jr.
Return to article.

Fractal Plate Reconstruction Table 1




Age
(Ma)


Initial


Final


Longitude


Latitude


Angle


Longitude


Latitude


Angle


0.000*


41.800


11.300


0.633


--


--


--


2.581


40.300


11.164


1.655


41.738


12.395


1.001


5.000


40.638


11.446


3.192


40.972


12.123


3.151


6.033


40.770


11.591


3.830


40.366


11.906


4.057


10.000


38.728


11.830


6.184


37.759


11.025


6.314


11.040


37.942


11.896


6.790


37.655


11.049


6.781


15.000


35.773


12.481


9.140


37.796


12.082


8.980


19.722


34.370


13.393


12.051


32.877


12.850


12.168


20.000


34.304


13.437


12.225


32.695


12.874


12.356


25.000


33.520


13.840


15.275


33.610


13.141


15.345


26.154


33.556


13.805


15.919


34.052


13.126


15.947


28.715


33.984


13.580


17.319


34.616


13.039


17.272


30.000


34.234


13.466


18.148


34.718


13.015


17.989


31.116


34.377


13.396


18.890


34.722


13.032


18.670


33.738


34.377


13.451


20.495


34.352


13.303


20.360


35.000


34.326


13.666


21.324


33.934


13.599


21.122


37.771


33.475


14.650


22.882


32.585


14.622


22.499


39.464


32.000


15.600


23.300


31.845


15.459


23.506


40.000


31.465


15.924


23.398


33.419


16.267


26.186

Table 1. Initial and final total finite rotation parameters, degrees, Antarctic and Australian plates. Initial parameters are converted to normalized pseudovectors assigned magnitudes equal to total rotation rate for each age and then interpolated in each of the three dimensions via cubic splines at 5 m.y. intervals.
Sources: Cande and Stock (2004, in italics), Müller et al. (2008; 39.424 Ma). Timescale: Gradstein et al. (2004)
Return to article.

Monday, December 20, 2010

Fractal Plate Reconstruction?

Fractal Plate Reconstructions, Seafloor Spreading Asymmetry, and Kinematics utilizing Fractal Criteria
Summary
Information theory and fractal analysis provide a basis for a new approach to plate reconstructions of magnetic isochrons and fracture zone crossings. The new approach models accretionary boundaries as fractals (via variable binning sizes) and seeks parameter sets that produce a minimum sum of logarithms of bin numbers. Spline interpolation of a trial reconstruction parameter set, including spreading asymmetry along ridge segments, and Monte Carlo modifications to the parameters provide iterative calculation of the full fractal set. Such a method allows for incorporation of all isochron identifications from the plates of interest in a single, iterative calculation set rather than just a few separate, selected individual reconstruction calculations. The splined parameter sets also provide a means for calculating instantaneous rotation rates and asymmetries. More detailed analysis of the fractal results for a number of the “best” solutions also provides alternative approaches to characterization of the uncertainty in the derived reconstruction parameters; more work will be required in this area.

Paleostress maps - updated

The Western United States paleostress maps in a previous post are largely based on a compilation used in Pilger (2003).


The merged data set, including Bird's (2002) data set, mentioned in the immediately previous post, has been used for updating the earlier maps. The sH1 measurements are in light blue for the first 5 m.y. of each 10 m.y. interval and dark blue for the last 5 m.y. Tangents to calculated instantaneous kinematic small circles (see Pilger, 2003, for a description of methodology) are calculated each 5 m.y. as labeled. (Click graphic to enlarge. Click Back button or icon to return to post.)


0-10 Ma

Sunday, December 19, 2010

Merged Paleostress Data Sets

Paleostress data from Peter Bird's (2001) and Rex Pilger's (2003) compilations have been merged: link. References are also included.

It is my intention to continue adding to this data set and maintain its public availability. Please send comments and additional contributions/corrections to rexpilger (at) gmail (period) com.

Saturday, December 18, 2010

Paleostress data - asking for more

Most of the paleostress data presented in maps by Pilger (2003) and in earlier webposts (here and here) are available at this link.

The World Stress Map project largely consists of contemporary or at most Recent data, and not paleostress measurements. Peter Bird has compiled a separate, partially overlapping data set with different constraints. Yet, together, the compilations are woefully inadequate, especially outside the US Cordillera. In light of the growing importance of fracture reservoirs for petroleum and gas, knowledge of paleostresses and paleofractures is valuable for exploration and development of such resources.

If you have additional paleostress data, I would welcome the opportunity to add them to the data store. Please email rexpilger (at) gmail (dot) com.

Wednesday, December 15, 2010

Intracontinental Tectonics, Stresses, and Fracture Reservoirs - Clues from Plate Kinematics

Introduction

Now in its sixth decade, plate tectonics has reshaped the understanding of the evolution of the Earth, especially the origin of major earthquakes, ocean basins, mountain belts, and magmatism. Elaboration of the theory relative to hydrocarbon exploration and development has provided insight into the nature of continental margin sedimentary basins, especially in concert with improved understanding of stratigraphic sequencing, fluid pressures and migration, diagenesis, and compaction. Plate tectonics has also provided a framework for understanding compressional thrust belts associated with convergent plate boundaries, both continental to continental and continental to oceanic plate.

Monday, December 13, 2010

Wednesday, September 29, 2010

Alien Science

Bloggers are afire with the "news" of a United Nations designated representative for future encounters of humanity with intelligent alien life. So the Sunday Times tell us via the Aussies (link via First Things). Try a Bing search for a hint of the excitement. Alas, Trekkies, it's apparently not so. No, the all-knowing UN hasn't overreached this far, yet.
I recall an episode of Johnny Carson's Tonight Show, years ago, in which the clever host asked his audience the rhetorical question (paraphrased from aging memory): "Why do the UFO's always land in places like Roswell? Why not Central Park?"
I'm a geologist/geophysicist by training and profession. Is the public aware, and have my fellow geoscientists realized, that in the earth's four billion year rock record there have been found no, none, nada, zip, zero... traces of evidence of any extraterrestrial intelligence: fossilized tricorders, abandoned transporter chambers or obsolete stargate molds, detached Enterprise engine imprints?

Thursday, August 19, 2010

Organized Science and Its Dirty Little Secret

If there is a recognized deity in the world of organized science, one of its names is “Peer Review”. Before results of any serious scientific investigation are published in a reputable journal, an associate editor farms out the submitted paper to “peers” of the hopeful author(s) (in a few cases the editor may reject a submission without review). Much of the time this process works fairly well; the reviewers provide an evaluation of the would-be contribution: its novelty (has somebody else has produced the same result?), evidence (and further testability), coherence (do the data support the interpretation), and citation of appropriate sources, and makes a recommendation: accept as is (rare), accept with modifications (more common), or go back to the salt mines and here’s why (most common). The editor may solicit numerous reviewers and from the typically one or two returned reviews makes his or her decision on the submission.