A L Peratt and W F Yao 2008 Phys. Scr. 2008 014048 doi:10.1088/0031-8949/2008/T131/014048
A L Peratt1,2 and W F Yao3
Show affiliationsA past intense solar outburst and its effect on Earth was proposed by Gold (1962 Pontificiae Acad. Sci. Scr. Varia 25 159) who, along with others, based his hypotheses on strong astronomical and geophysical evidence. The discovery that objects from the Neolithic or Early Bronze Age carry patterns associated with high-current Z-pinches, as would result from an intense plasma impinging Earth, provides a possible insight into the origin and meaning of these ancient symbols produced by humans. Peratt (2003 Trans. Plasma Sci. 31 1192) dealt with the comparison of graphical and radiation data from high-current Z-pinches to petroglyphs, geoglyphs and megaliths. Peratt (2007 Trans. Plasma Sci. 35 778) focused primarily, but not exclusively, on petroglyphs of some 84 different morphologies; pictures found in laboratory experiments and carved on rock. These corresponded to mankind's visual observations of ancient aurora as might be produced if the solar wind had increased at times between one and two orders of magnitude, millennia ago (Gold 1962 Pontificiae Acad. Sci. Scr. Varia 25 159). In Peratt (2007 Trans. Plasma Sci. 35 778), the data were given on the source of light and its temporal change from a current-increasing Z-pinch or dense plasma focus aurora. Orientation and field-of-view data are given as surveyed and contributed from 139 countries, from sites and fields containing several millions of these objects, the latest data coming from a 300 km survey along the Orinoco river basin in Venezuela. In this paper, we include additional petroglyph figures derivable from experiment and computer. This information allows a reconstruction of the auroral form presumably associated with extreme geomagnetic storms and shows, based on existent geophysical evidence, relativistic electron flow inward at Earth's south polar axis and hypervelocity proton impacts around the north polar axis.
94.30.Va Magnetosheath; interaction with interplanetary space (including solar wind)
94.30.Aa Auroral phenomena in magnetospher
96.60.Vg Particle emission, solar wind
91.65.Ti Sedimentary petrology
95.80.+p Astronomical catalogs, atlases, sky surveys, databases, retrieval systems, archives, etc.
Issue T131 (October 2008)
Received 10 June 2008, accepted for publication 17 June 2008
Published 5 December 2008
A L Peratt and W F Yao 2008 Phys. Scr. 2008 014048
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