Recent Progress in Paleomagnetic and Rock-Magnetic Studies of the Quaternary in Japan
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Is Earth's Magnetic Field Reversing? ⁎ Catherine Constable A, , Monika Korte B
Earth and Planetary Science Letters 246 (2006) 1–16 www.elsevier.com/locate/epsl Frontiers Is Earth's magnetic field reversing? ⁎ Catherine Constable a, , Monika Korte b a Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California at San Diego, La Jolla, CA 92093-0225, USA b GeoForschungsZentrum Potsdam, Telegrafenberg, 14473 Potsdam, Germany Received 7 October 2005; received in revised form 21 March 2006; accepted 23 March 2006 Editor: A.N. Halliday Abstract Earth's dipole field has been diminishing in strength since the first systematic observations of field intensity were made in the mid nineteenth century. This has led to speculation that the geomagnetic field might now be in the early stages of a reversal. In the longer term context of paleomagnetic observations it is found that for the current reversal rate and expected statistical variability in polarity interval length an interval as long as the ongoing 0.78 Myr Brunhes polarity interval is to be expected with a probability of less than 0.15, and the preferred probability estimates range from 0.06 to 0.08. These rather low odds might be used to infer that the next reversal is overdue, but the assessment is limited by the statistical treatment of reversals as point processes. Recent paleofield observations combined with insights derived from field modeling and numerical geodynamo simulations suggest that a reversal is not imminent. The current value of the dipole moment remains high compared with the average throughout the ongoing 0.78 Myr Brunhes polarity interval; the present rate of change in Earth's dipole strength is not anomalous compared with rates of change for the past 7 kyr; furthermore there is evidence that the field has been stronger on average during the Brunhes than for the past 160 Ma, and that high average field values are associated with longer polarity chrons. -
The Role of Geomagnetic Field Intensity in Late Quaternary Evolution of 2 Humans and Large Mammals 3 4 5 J.E.T
1 1 The role of geomagnetic field intensity in late Quaternary evolution of 2 humans and large mammals 3 4 5 J.E.T. Channell1 and L. Vigliotti2 6 7 1 Department of Geological Sciences, University of Florida, Gainesville, FL 32611, USA 8 9 2 Istituto di Scienze Marine, ISMAR-CNR, Via P. Gobetti 101, 40129 Bologna, Italy 10 11 Corresponding author: James E.T. Channell ([email protected]) 12 13 Key Points: (1) The strength of the geomagnetic field is a proxy for the flux of ultra- 14 violet radiation (UVR). (2) The disappearances of the Neanderthals and many large 15 mammals during the Late Quaternary occur during minima in geomagnetic field 16 strength. (3) Human phylogeny from mitochrondrial DNA and Y-chromosomes can also 17 be linked to minima in field strength, hence UVR flux. 18 19 Abstract 20 21 It has long been speculated that biological evolution was influenced by ultra-violet 22 radiation (UVR) reaching the Earth’s surface, despite imprecise knowledge of the timing 23 of both UVR flux and evolutionary events. The past strength of Earth’s dipole field 24 provides a proxy for UVR flux because of its role in maintaining stratospheric ozone. 25 The timing of Quaternary evolutionary events has become better constrained by fossil 26 finds, improved radiometric dating, use of dung fungi as proxies for herbivore 27 populations, and improved ages for nodes in human phylogeny from human 28 mitochrondrial DNA (mtDNA) and Y-chromosomes. The demise of Neanderthals at ~41 29 ka can now be closely tied to the intensity minimum associated with the Laschamp 30 magnetic excursion, and the survival of anatomically modern humans (AMHs) can be 31 attributed to differences in the aryl hydrocarbon receptor (AhR) that has a key role in 32 the evolutionary response to UVR flux. -
5.10 Geomagnetic Excursions C
5.10 Geomagnetic Excursions C. Laj, Laboratoire des Sciences du Climat et de l’Environment, Unite´ Mixte CEA-CNRS-UVSQ, Gif-sur-Yvette, France J. E. T. Channell, University of Florida, Gainesville, FL, USA ª 2007 Elsevier B.V. All rights reserved. 5.10.1 Introduction 373 5.10.1.1 History of the Polarity Timescale and Excursions 373 5.10.1.2 Nomenclature for Excursions and Polarity Intervals 375 5.10.2 Geomagnetic Excursions in the Brunhes Chron 376 5.10.2.1 Introduction 376 5.10.2.2 The Laschamp Excursion 379 5.10.2.3 The Mono Lake Excursion 383 5.10.2.4 The Blake Excursion 385 5.10.2.5 The Iceland Basin Excursion 387 5.10.2.6 The Pringle Falls Excursion 389 5.10.2.7 Excursions in the Early Brunhes Chron 391 5.10.3 Geomagnetic Excursions in the Matuyama Chron 393 5.10.3.1 Background 393 5.10.3.2 Excursions between the Gauss–Matuyama Boundary and the Re´ union Subchron 396 5.10.3.3 Huckleberry Ridge 396 5.10.3.4 Gilsa 396 5.10.3.5 Gardar and Bjorn 397 5.10.3.6 Cobb Mountain 397 5.10.3.7 Punaruu 397 5.10.3.8 Intra-Jaramillo Excursion (1r.1n.1r) 397 5.10.3.9 Santa Rosa 397 5.10.3.10 Kamikatsura 398 5.10.4 Geomagnetic Excursions in Pre-Matuyama Time 398 5.10.4.1 C5n.2n (Late Miocene) 400 5.10.4.2 Other Miocene Excursions/Subchrons 401 5.10.4.3 Oligocene and Eocene 401 5.10.4.4 Middle Cretaceous 402 5.10.5 Duration of Geomagnetic Excursions 402 5.10.6 Excursional Field Geometry 404 5.10.7 Concluding Remarks 405 References 407 5.10.1 Introduction Miocene lavas from central France (Puy de Dome). -
Possible Holocene Excursion of the Earth's Magnetic Field In
Earth Planets Space, 51, 175–191, 1999 Possible Holocene excursion of the Earth’s magnetic field in southern South America: New records from archaeological sites in Argentina Hugo G. Nami1,2 1Laboratorio de Paleomagnetismo “Daniel A. Valencio”, Departamento de Ciencias Geologicas,´ Facultad de Ciencias Exactas, F´ısicas y Naturales, Universidad de Buenos Aires, Ciudad Universitaria (Pabellon´ II), (1428) Buenos Aires, Argentina 2Programa de Estudios Prehistoricos´ (CONICET), B. Mitre 1970 Piso 5 “A”, Buenos Aires (1039), Republica´ Argentina (Received August 3, 1998; Revised November 18, 1998; Accepted December 17, 1998) Palaeomagnetic studies were carried out in several archaeological and palaeontological sites across Argentina and Chile. Remanence directions far removed from the present magnetic field, probably corresponding to a field excursion were recorded in several stratigraphic sections spaning ∼11 to 2 ky bp. Detailed palaeomagnetic data from 235 cores obtained in six sections from archaeological sites in Argentina are reported. Stability of the NRM was analyzed by progressive thermal and alternating field demagnetization and ChRM directions determined in most cases. Computed VGPs from those directions tend to be concentrated over North America, Europe, Eastern Asia and Africa. Using 275 VGPs a palaeomagnetic pole that is ∼20◦ apart from the Earth’s rotation’s axis was obtained. 1. Introduction ported. Additionally, a summary of the evidence of a proba- Sedimentary deposits from archaeological sites, caves and ble GF excursion occurred in southern South America during rockshelters have been the subject of paleomagnetic research the latest Pleistocene and Holocene is reported. for many years. These investigations were useful in examin- ing paleomagnetic secular variation (PSV) at different locali- 2. -
The 13 Million Year Cenozoic Pulse of the Earth ∗ Jiasheng Chen A,B,C, Vadim A
Earth and Planetary Science Letters 431 (2015) 256–263 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl The 13 million year Cenozoic pulse of the Earth ∗ Jiasheng Chen a,b,c, Vadim A. Kravchinsky b, , Xiuming Liu a,c a School of Geographical Sciences, Fujian Normal University, Fuzhou 350007, China b Department of Physics, University of Alberta, Edmonton, Alberta T6G 2E1, Canada c Key Laboratory of Western China’s Environmental Systems, Research School of Arid Environment & Climate Change, Lanzhou University, Lanzhou 730000, China a r t i c l e i n f o a b s t r a c t Article history: The geomagnetic polarity reversal rate changes radically from very low to extremely high. Such process Received 12 January 2015 indicates fundamental changes in the Earth’s core reorganization and core–mantle boundary heat flow Received in revised form 18 September fluctuations. However, we still do not know how critical such changes are to surface geology and climate 2015 processes. Our analysis of the geomagnetic reversal frequency, oxygen isotope record, and tectonic plate Accepted 21 September 2015 subduction rate, which are indicators of the changes in the heat flux at the core mantle boundary, Available online 13 October 2015 Editor: M. Frank climate and plate tectonic activity, shows that all these changes indicate similar rhythms on million years’ timescale in the Cenozoic Era occurring with the common fundamental periodicity of ∼13 Myr Keywords: during most of the time. The periodicity is disrupted only during the last 20 Myr. Such periodic behavior Cenozoic suggests that large scale climate and tectonic changes at the Earth’s surface are closely connected with Cenozoic climate change the million year timescale cyclical reorganization of the Earth’s interior. -
Paleoclimatic Context of Geomagnetic Dipole Lows and Excursions in the Brunhes, Clue for an Orbital Influence on the Geodynamo?
Earth and Planetary Science Letters 275 (2008) 269–284 Contents lists available at ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl Paleoclimatic context of geomagnetic dipole lows and excursions in the Brunhes, clue for an orbital influence on the geodynamo? Nicolas Thouveny a,⁎, Didier L. Bourlès a, Ginette Saracco a, Julien T. Carcaillet a,b, F. Bassinot c a CEREGE, Aix-Marseille Université et CNRS, Europôle Méditerranéen de l'Arbois, BP 80, 13545, Aix en Provence, cedex 4, France b Laboratoire de Géodynamique des Chaînes Alpines (LGCA), Université Joseph Fourier et CNRS, BP53, 38041 Grenoble cedex 09, France c Laboratoire des Sciences du Climat et de l'Environnement, CNRS-CEA, Avenue de la Terrasse, 91198, Gif/Yvette, France article info abstract Article history: The hypothesis of an influence of the astronomical precession on the geodynamo energy budget was recently Received 8 July 2008 reappraised by theoreticians. Paleomagnetic indications of such an influence remain controversial because Accepted 15 August 2008 reconstructions of paleointensity variations from sediments are suspected to be contaminated by lithological, Available online 2 October 2008 paleoclimatically induced influences. Three sets of complementary indicators are however available: Editor: R.D. van der Hilst 1) records of the direction of magnetization in sediments, 2) records of magnetic anomalies of the deep sea floor basalts and 3) records of production variations of cosmogenic isotopes from sediment and ice cores. Keywords: These records confirm the genuine geomagnetic origin of paleointensity lows and their narrow link with geomagnetic dipole lows excursions or short reversals recorded in various materials and often dated by radiometric methods. -
Solis Glaciation Ang Core Reversal
Relations and Implications of Aperiodic Earth Core / Geomagnetic Field Reversals with Earth Glaciations José L. Fernández-Solís, PhD [email protected] (979) 458-1058 3137 TAMU College Station, TX 77845 Swedish Academy of Science 22 June 2015 NASA 26 May 2017 Current version 13 August 2018 Executive Summary This research answers the critical question: What happens when earth loses its magnetic field (“temporarily in geological times– i.e. several thousand years”)? How does earth loses its magnetic field? What are the consequences of galactic-cosmic and solar space radiation flux and a weakened, chaotic or disappearing geomagnetic field? What are the relationships among earth’s core reversal, magnetic field reversal, magma displacement, accelerated tectonic activity, supervolcanic eruptions, and climatic consequences? The current, and considerable, scientific body of knowledge does not take fully into consideration earth’s aperiodic and irregular but real and in human time scale, long-lasting geomagnetic field reversals. A total geomagnetic reversal is a change in a planet’s magnetic field such that the positions of magnetic north and magnetic south interchange. We are 200+ years into the midst of geomagnetic field reversal phenomena, within an extended earth glacial period. The current reversal’s consequences will last thousands of years, but no research links existing body of knowledge to this phenomenon. Reversals can have relatively mild consequences such as the last Little Ice Age, or Snowball Earth or even more critical, icehouse Earth. The Little Ice Age occurred 1300 – 1870 CE. The last snowball earth was 21,000 years ago and ended 11,500 years ago, lasting approximately 10,000 years! This event is calculated to have covered New York City in glacial ice, three Empire State Buildings or higher. -
661 the 'Sterno-Etrussia' Geomagnetic Excursion
RADIOCARBON, Vol 46, Nr 2, 2004, p 661–681 © 2004 by the Arizona Board of Regents on behalf of the University of Arizona THE ‘STERNO-ETRUSSIA’ GEOMAGNETIC EXCURSION AROUND 2700 BP AND CHANGES OF SOLAR ACTIVITY, COSMIC RAY INTENSITY, AND CLIMATE V A Dergachev1 • O M Raspopov2 • B van Geel3 • G I Zaitseva4 ABSTRACT. The analysis of both paleo- and archeomagnetic data and magnetic properties of continental and marine sedi- ments has shown that around 2700 BP, the geomagnetic Sterno-Etrussia excursion took place in 15 regions of the Northern Hemisphere. The study of magnetic properties of sediments of the Barents, Baltic, and White Seas demonstrates that the dura- tion of this excursion was not more than 200–300 yr. Paleoclimatic data provide extensive evidence for a sharp global cooling around 2700 BP. The causes of natural climate vari- ation are discussed. Changes of the galactic cosmic ray intensity may play a key role as the causal mechanism of climate change. Since the cosmic ray intensity (reflected by the cosmogenic isotope level in the earth’s atmosphere) is modulated by the solar wind and by the terrestrial magnetic field, this may be an important mechanism for long-term solar climate variabil- ity. The Sterno-Etrussia excursion may have amplified the climate shift, which, in the first place, was the effect of a decline of solar activity. During excursions and inversions, the magnetic moment decreases, which leads to an increased intensity of cosmic rays penetrating the upper atmosphere. Global changes in the electromagnetic field of the earth result in sharp changes in the climate-determining factors in the atmosphere, such as temperatures, total pressure field, moisture circulation, intensity of air flows, and thunderstorm activity. -
UPL12778 Bard98gca___Copie.Pdf
Geochimica et Cosmochimica Acta, Vol. 62, No. 12, pp. 2025–2038, 1998 Copyright © 1998 Elsevier Science Ltd Pergamon Printed in the USA. All rights reserved 0016-7037/98 $19.00 1 .00 PII S0016-7037(98)00130-6 PAUL GAST LECTURE Geochemical and geophysical implications of the radiocarbon calibration EDOUARD BARD* CEREGE, Universite´ Aix-Marseille III and CNRS, Institut Universitaire de France, Europoˆle de l’Arbois, 13545, Aix-en-Provence cedex 4, France (Received March 10, 1998; accepted in revised form March 10, 1998) Abstract—A precise and accurate chronological framework is crucial to study the dynamics of a variety of phenomena which occurred during the last 45,000 years. Although the 14C dating method has been widely applied since the 1950s, it is recognized that the atmospheric 14C/12C ratio has not been stable during the past. In order to calculate accurate ages, these fluctuations have to be corrected by means of a calibration curve obtained by comparing raw 14C measurements with true calendar ages provided by independent dating methods. The calibration curve obtained so far is characterized by a long-term trend with raw 14C ages being significantly younger than calendar ages during most of the last 45,000 years. Abrupt 14C shifts, which occurred over centuries to millennia, are superimposed on this long-term trend of decreasing atmospheric 14C/12C ratio. To a certain extent, it is possible to outline the different causes of atmospheric 14C variations by considering complementary information obtained from other cosmogenic nuclides studied at different latitudes: (1) Most high-frequency changes in the atmospheric 14C/12C ratio are linked to magnetic fluctuations of solar origin as revealed by studying the last three centuries for which direct observations of the Sun are available.