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Cryogenian Glaciation and the Onset of Carbon-Isotope Decoupling” by N
CORRECTED 21 MAY 2010; SEE LAST PAGE REPORTS 13. J. Helbert, A. Maturilli, N. Mueller, in Venus Eds. (U.S. Geological Society Open-File Report 2005- M. F. Coffin, Eds. (Monograph 100, American Geophysical Geochemistry: Progress, Prospects, and New Missions 1271, Abstracts of the Annual Meeting of Planetary Union, Washington, DC, 1997), pp. 1–28. (Lunar and Planetary Institute, Houston, TX, 2009), abstr. Geologic Mappers, Washington, DC, 2005), pp. 20–21. 44. M. A. Bullock, D. H. Grinspoon, Icarus 150, 19 (2001). 2010. 25. E. R. Stofan, S. E. Smrekar, J. Helbert, P. Martin, 45. R. G. Strom, G. G. Schaber, D. D. Dawson, J. Geophys. 14. J. Helbert, A. Maturilli, Earth Planet. Sci. Lett. 285, 347 N. Mueller, Lunar Planet. Sci. XXXIX, abstr. 1033 Res. 99, 10,899 (1994). (2009). (2009). 46. K. M. Roberts, J. E. Guest, J. W. Head, M. G. Lancaster, 15. Coronae are circular volcano-tectonic features that are 26. B. D. Campbell et al., J. Geophys. Res. 97, 16,249 J. Geophys. Res. 97, 15,991 (1992). unique to Venus and have an average diameter of (1992). 47. C. R. K. Kilburn, in Encyclopedia of Volcanoes, ~250 km (5). They are defined by their circular and often 27. R. J. Phillips, N. R. Izenberg, Geophys. Res. Lett. 22, 1617 H. Sigurdsson, Ed. (Academic Press, San Diego, CA, radial fractures and always produce some form of volcanism. (1995). 2000), pp. 291–306. 16. G. E. McGill, S. J. Steenstrup, C. Barton, P. G. Ford, 28. C. M. Pieters et al., Science 234, 1379 (1986). 48. -
The Last Maximum Ice Extent and Subsequent Deglaciation of the Pyrenees: an Overview of Recent Research
Cuadernos de Investigación Geográfica 2015 Nº 41 (2) pp. 359-387 ISSN 0211-6820 DOI: 10.18172/cig.2708 © Universidad de La Rioja THE LAST MAXIMUM ICE EXTENT AND SUBSEQUENT DEGLACIATION OF THE PYRENEES: AN OVERVIEW OF RECENT RESEARCH M. DELMAS Université de Perpignan-Via Domitia, UMR 7194 CNRS, Histoire Naturelle de l’Homme Préhistorique, 52 avenue Paul Alduy 66860 Perpignan, France. ABSTRACT. This paper reviews data currently available on the glacial fluctuations that occurred in the Pyrenees between the Würmian Maximum Ice Extent (MIE) and the beginning of the Holocene. It puts the studies published since the end of the 19th century in a historical perspective and focuses on how the methods of investigation used by successive generations of authors led them to paleogeographic and chronologic conclusions that for a time were antagonistic and later became complementary. The inventory and mapping of the ice-marginal deposits has allowed several glacial stades to be identified, and the successive ice boundaries to be outlined. Meanwhile, the weathering grade of moraines and glaciofluvial deposits has allowed Würmian glacial deposits to be distinguished from pre-Würmian ones, and has thus allowed the Würmian Maximum Ice Extent (MIE) –i.e. the starting point of the last deglaciation– to be clearly located. During the 1980s, 14C dating of glaciolacustrine sequences began to indirectly document the timing of the glacial stades responsible for the adjacent frontal or lateral moraines. Over the last decade, in situ-produced cosmogenic nuclides (10Be and 36Cl) have been documenting the deglaciation process more directly because the data are obtained from glacial landforms or deposits such as boulders embedded in frontal or lateral moraines, or ice- polished rock surfaces. -
Chapter 30. Latest Oligocene Through Early Miocene Isotopic Stratigraphy
Shackleton, N.J., Curry, W.B., Richter, C., and Bralower, T.J. (Eds.), 1997 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 154 30. LATEST OLIGOCENE THROUGH EARLY MIOCENE ISOTOPIC STRATIGRAPHY AND DEEP-WATER PALEOCEANOGRAPHY OF THE WESTERN EQUATORIAL ATLANTIC: SITES 926 AND 9291 B.P. Flower,2 J.C. Zachos,2 and E. Martin3 ABSTRACT Stable isotopic (d18O and d13C) and strontium isotopic (87Sr/86Sr) data generated from Ocean Drilling Program (ODP) Sites 926 and 929 on Ceara Rise provide a detailed chemostratigraphy for the latest Oligocene through early Miocene of the western Equatorial Atlantic. Oxygen isotopic data based on the benthic foraminifer Cibicidoides mundulus exhibit four distinct d18O excursions of more than 0.5ä, including event Mi1 near the Oligocene/Miocene boundary from 23.9 to 22.9 Ma and increases at about 21.5, 18 and 16.5 Ma, probably reßecting episodes of early Miocene Antarctic glaciation events (Mi1a, Mi1b, and Mi2). Carbon isotopic data exhibit well-known d13C increases near the Oligocene/Miocene boundary (~23.8 to 22.6 Ma) and near the early/middle Miocene boundary (~17.5 to 16 Ma). Strontium isotopic data reveal an unconformity in the Hole 926A sequence at about 304 meters below sea ßoor (mbsf); no such unconformity is observed at Site 929. The age of the unconfor- mity is estimated as 17.9 to 16.3 Ma based on a magnetostratigraphic calibration of the 87Sr/86Sr seawater curve, and as 17.4 to 15.8 Ma based on a biostratigraphic calibration. Shipboard biostratigraphic data are more consistent with the biostratigraphic calibration. -
Sam White the Real Little Ice Age Between C.1300 and C.1850 A.D
Journal of Interdisciplinary History, xliv:3 (Winter, 2014), 327–352. THE REAL LITTLE ICE AGE Sam White The Real Little Ice Age Between c.1300 and c.1850 a.d. the world became, on average, slightly but signiªcantly colder. The change varied over time and space, and its causes remain un- certain. Nevertheless, this cooling constitutes a meaningful climate event, with signiªcant historical consequences. Both the cooling trend and its effects on humans appear to have been particularly Downloaded from http://direct.mit.edu/jinh/article-pdf/44/3/327/1706251/jinh_a_00574.pdf by guest on 28 September 2021 acute from the late sixteenth to the late seventeenth century in much of the Northern Hemisphere. This article explains why climatologists and historians are conªdent that these changes occurred. On close examination, the objections raised in this issue of the journal by Kelly and Ó Gráda turn out to be entirely unfounded. The proxy data for early mod- ern global cooling (such as tree rings and ice cores) are robust, and written weather descriptions and observations of physical phenom- ena (such as glacial movements and river freezings) by and large of- fer independent conªrmation. Kelly and Ó Gráda’s proposed alter- native measures of climate and climate change suffer from serious ºaws. As we review the evidence and refute their criticisms, it will become clear just how solid the case for the Little Ice Age (lia) has become. the case for the little ice age The evidence for early modern global cooling comes, ªrst and foremost, from extensive research into physical proxies, including ice cores, tree rings, corals, and speleothems (stalagmites and stalactites). -
Sea Level and Global Ice Volumes from the Last Glacial Maximum to the Holocene
Sea level and global ice volumes from the Last Glacial Maximum to the Holocene Kurt Lambecka,b,1, Hélène Roubya,b, Anthony Purcella, Yiying Sunc, and Malcolm Sambridgea aResearch School of Earth Sciences, The Australian National University, Canberra, ACT 0200, Australia; bLaboratoire de Géologie de l’École Normale Supérieure, UMR 8538 du CNRS, 75231 Paris, France; and cDepartment of Earth Sciences, University of Hong Kong, Hong Kong, China This contribution is part of the special series of Inaugural Articles by members of the National Academy of Sciences elected in 2009. Contributed by Kurt Lambeck, September 12, 2014 (sent for review July 1, 2014; reviewed by Edouard Bard, Jerry X. Mitrovica, and Peter U. Clark) The major cause of sea-level change during ice ages is the exchange for the Holocene for which the direct measures of past sea level are of water between ice and ocean and the planet’s dynamic response relatively abundant, for example, exhibit differences both in phase to the changing surface load. Inversion of ∼1,000 observations for and in noise characteristics between the two data [compare, for the past 35,000 y from localities far from former ice margins has example, the Holocene parts of oxygen isotope records from the provided new constraints on the fluctuation of ice volume in this Pacific (9) and from two Red Sea cores (10)]. interval. Key results are: (i) a rapid final fall in global sea level of Past sea level is measured with respect to its present position ∼40 m in <2,000 y at the onset of the glacial maximum ∼30,000 y and contains information on both land movement and changes in before present (30 ka BP); (ii) a slow fall to −134 m from 29 to 21 ka ocean volume. -
Reduced El Niño–Southern Oscillation During the Last Glacial
RESEARCH | REPORTS PALEOCEANOGRAPHY vergent results and our newly generated data by considering geographic location, choice of fora- minifera species, and changes in thermocline – depth (see supplementary materials). Reduced El Niño Southern Oscillation ENSO variability is asymmetric (the El Niño warm phase is more extreme than the La Niña during the Last Glacial Maximum cold phase) (14), so temperature variations in the equatorial Pacific are not normally distrib- Heather L. Ford,1,2* A. Christina Ravelo,1 Pratigya J. Polissar2 uted (7, 15), and statistical tests that assume normality (e.g., standard deviation) can lead to El Niño–Southern Oscillation (ENSO) is a major source of global interannual variability, but erroneous conclusions with respect to changes its response to climate change is uncertain. Paleoclimate records from the Last Glacial in variance. Therefore, we use quantile-quantile Maximum (LGM) provide insight into ENSO behavior when global boundary conditions (Q-Q) plots—a simple, yet powerful way to vi- — (ice sheet extent, atmospheric partial pressure of CO2) were different from those today. sualize distribution data to compare the tem- In this work, we reconstruct LGM temperature variability at equatorial Pacific sites perature range and distribution recorded by two using measurements of individual planktonic foraminifera shells. A deep equatorial populations of individual foraminifera shells to thermocline altered the dynamics in the eastern equatorial cold tongue, resulting in interpret possible climate forcing mechanisms. reduced ENSO variability during the LGM compared to the Late Holocene. These results Sensitivity studies using modern hydrographic suggest that ENSO was not tied directly to the east-west temperature gradient, as data show how changes in ENSO and seasonality previously suggested. -
UC Riverside UC Riverside Electronic Theses and Dissertations
UC Riverside UC Riverside Electronic Theses and Dissertations Title Exploring the Texture of Ocean-Atmosphere Redox Evolution on the Early Earth Permalink https://escholarship.org/uc/item/9v96g1j5 Author Reinhard, Christopher Thomas Publication Date 2012 Peer reviewed|Thesis/dissertation eScholarship.org Powered by the California Digital Library University of California UNIVERSITY OF CALIFORNIA RIVERSIDE Exploring the Texture of Ocean-Atmosphere Redox Evolution on the Early Earth A Dissertation submitted in partial satisfaction of the requirements for the degree of Doctor of Philosophy in Geological Sciences by Christopher Thomas Reinhard September 2012 Dissertation Committee: Dr. Timothy W. Lyons, Chairperson Dr. Gordon D. Love Dr. Nigel C. Hughes ! Copyright by Christopher Thomas Reinhard 2012 ! ! The Dissertation of Christopher Thomas Reinhard is approved: ________________________________________________ ________________________________________________ ________________________________________________ Committee Chairperson University of California, Riverside ! ! ACKNOWLEDGEMENTS It goes without saying (but I’ll say it anyway…) that things like this are never done in a vacuum. Not that I’ve invented cold fusion here, but it was quite a bit of work nonetheless and to say that my zest for the enterprise waned at times would be to put it euphemistically. As it happens, though, I’ve been fortunate enough to be surrounded these last years by an incredible group of people. To those that I consider scientific and professional mentors that have kept me interested, grounded, and challenged – most notably Tim Lyons, Rob Raiswell, Gordon Love, and Nigel Hughes – thank you for all that you do. I also owe Nigel and Mary Droser a particular debt of graditude for letting me flounder a bit my first year at UCR, being understanding and supportive, and encouraging me to start down the road to where I’ve ended up (for better or worse). -
Exhibit Specimen List FLORIDA SUBMERGED the Cretaceous, Paleocene, and Eocene (145 to 34 Million Years Ago) PARADISE ISLAND
Exhibit Specimen List FLORIDA SUBMERGED The Cretaceous, Paleocene, and Eocene (145 to 34 million years ago) FLORIDA FORMATIONS Avon Park Formation, Dolostone from Eocene time; Citrus County, Florida; with echinoid sand dollar fossil (Periarchus lyelli); specimen from Florida Geological Survey Avon Park Formation, Limestone from Eocene time; Citrus County, Florida; with organic layers containing seagrass remains from formation in shallow marine environment; specimen from Florida Geological Survey Ocala Limestone (Upper), Limestone from Eocene time; Jackson County, Florida; with foraminifera; specimen from Florida Geological Survey Ocala Limestone (Lower), Limestone from Eocene time; Citrus County, Florida; specimens from Tanner Collection OTHER Anhydrite, Evaporite from early Cenozoic time; Unknown location, Florida; from subsurface core, showing evaporite sequence, older than Avon Park Formation; specimen from Florida Geological Survey FOSSILS Tethyan Gastropod Fossil, (Velates floridanus); In Ocala Limestone from Eocene time; Barge Canal spoil island, Levy County, Florida; specimen from Tanner Collection Echinoid Sea Biscuit Fossils, (Eupatagus antillarum); In Ocala Limestone from Eocene time; Barge Canal spoil island, Levy County, Florida; specimens from Tanner Collection Echinoid Sea Biscuit Fossils, (Eupatagus antillarum); In Ocala Limestone from Eocene time; Mouth of Withlacoochee River, Levy County, Florida; specimens from John Sacha Collection PARADISE ISLAND The Oligocene (34 to 23 million years ago) FLORIDA FORMATIONS Suwannee -
Reforestation in a High-CO2 World—Higher Mitigation Potential Than
Geophysical Research Letters RESEARCH LETTER Reforestation in a high-CO2 world—Higher mitigation 10.1002/2016GL068824 potential than expected, lower adaptation Key Points: potential than hoped for • We isolate effects of land use changes and fossil-fuel emissions in RCPs 1 1 1 1 •ClimateandCO2 feedbacks strongly Sebastian Sonntag , Julia Pongratz , Christian H. Reick , and Hauke Schmidt affect mitigation potential of reforestation 1Max Planck Institute for Meteorology, Hamburg, Germany • Adaptation to mean temperature changes is still needed, but extremes might be reduced Abstract We assess the potential and possible consequences for the global climate of a strong reforestation scenario for this century. We perform model experiments using the Max Planck Institute Supporting Information: Earth System Model (MPI-ESM), forced by fossil-fuel CO2 emissions according to the high-emission scenario • Supporting Information S1 Representative Concentration Pathway (RCP) 8.5, but using land use transitions according to RCP4.5, which assumes strong reforestation. Thereby, we isolate the land use change effects of the RCPs from those Correspondence to: of other anthropogenic forcings. We find that by 2100 atmospheric CO2 is reduced by 85 ppm in the S. Sonntag, reforestation model experiment compared to the reference RCP8.5 model experiment. This reduction is [email protected] higher than previous estimates and is due to increased forest cover in combination with climate and CO2 feedbacks. We find that reforestation leads to global annual mean temperatures being lower by 0.27 K in Citation: 2100. We find large annual mean warming reductions in sparsely populated areas, whereas reductions in Sonntag, S., J. -
The Climate of the Last Glacial Maximum: Results from a Coupled Atmosphere-Ocean General Circulation Model Andrew B
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 104, NO. D20, PAGES 24,509–24,525, OCTOBER 27, 1999 The climate of the Last Glacial Maximum: Results from a coupled atmosphere-ocean general circulation model Andrew B. G. Bush Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, Canada S. George H. Philander Program in Atmospheric and Oceanic Sciences, Department of Geosciences, Princeton University Princeton, New Jersey Abstract. Results from a coupled atmosphere-ocean general circulation model simulation of the Last Glacial Maximum reveal annual mean continental cooling between 4Њ and 7ЊC over tropical landmasses, up to 26Њ of cooling over the Laurentide ice sheet, and a global mean temperature depression of 4.3ЊC. The simulation incorporates glacial ice sheets, glacial land surface, reduced sea level, 21 ka orbital parameters, and decreased atmospheric CO2. Glacial winds, in addition to exhibiting anticyclonic circulations over the ice sheets themselves, show a strong cyclonic circulation over the northwest Atlantic basin, enhanced easterly flow over the tropical Pacific, and enhanced westerly flow over the Indian Ocean. Changes in equatorial winds are congruous with a westward shift in tropical convection, which leaves the western Pacific much drier than today but the Indonesian archipelago much wetter. Global mean specific humidity in the glacial climate is 10% less than today. Stronger Pacific easterlies increase the tilt of the tropical thermocline, increase the speed of the Equatorial Undercurrent, and increase the westward extent of the cold tongue, thereby depressing glacial sea surface temperatures in the western tropical Pacific by ϳ5Њ–6ЊC. 1. Introduction and Broccoli, 1985a, b; Broccoli and Manabe, 1987; Broccoli and Marciniak, 1996]. -
The History of Ice on Earth by Michael Marshall
The history of ice on Earth By Michael Marshall Primitive humans, clad in animal skins, trekking across vast expanses of ice in a desperate search to find food. That’s the image that comes to mind when most of us think about an ice age. But in fact there have been many ice ages, most of them long before humans made their first appearance. And the familiar picture of an ice age is of a comparatively mild one: others were so severe that the entire Earth froze over, for tens or even hundreds of millions of years. In fact, the planet seems to have three main settings: “greenhouse”, when tropical temperatures extend to the polesand there are no ice sheets at all; “icehouse”, when there is some permanent ice, although its extent varies greatly; and “snowball”, in which the planet’s entire surface is frozen over. Why the ice periodically advances – and why it retreats again – is a mystery that glaciologists have only just started to unravel. Here’s our recap of all the back and forth they’re trying to explain. Snowball Earth 2.4 to 2.1 billion years ago The Huronian glaciation is the oldest ice age we know about. The Earth was just over 2 billion years old, and home only to unicellular life-forms. The early stages of the Huronian, from 2.4 to 2.3 billion years ago, seem to have been particularly severe, with the entire planet frozen over in the first “snowball Earth”. This may have been triggered by a 250-million-year lull in volcanic activity, which would have meant less carbon dioxide being pumped into the atmosphere, and a reduced greenhouse effect. -
The Petroleum Potential of the Riphean–Vendian Succession of Southern East Siberia
See discussions, stats, and author profiles for this publication at: https://www.researchgate.net/publication/253369249 The petroleum potential of the Riphean–Vendian succession of southern East Siberia CHAPTER in GEOLOGICAL SOCIETY LONDON SPECIAL PUBLICATIONS · MAY 2012 Impact Factor: 2.58 · DOI: 10.1144/SP366.1 CITATIONS READS 2 95 4 AUTHORS, INCLUDING: Olga K. Bogolepova Uppsala University 51 PUBLICATIONS 271 CITATIONS SEE PROFILE Alexander P. Gubanov Scandiz Research 55 PUBLICATIONS 485 CITATIONS SEE PROFILE Available from: Olga K. Bogolepova Retrieved on: 08 March 2016 Downloaded from http://sp.lyellcollection.org/ by guest on March 25, 2013 Geological Society, London, Special Publications The petroleum potential of the Riphean-Vendian succession of southern East Siberia James P. Howard, Olga K. Bogolepova, Alexander P. Gubanov and Marcela G?mez-Pérez Geological Society, London, Special Publications 2012, v.366; p177-198. doi: 10.1144/SP366.1 Email alerting click here to receive free e-mail alerts when service new articles cite this article Permission click here to seek permission to re-use all or request part of this article Subscribe click here to subscribe to Geological Society, London, Special Publications or the Lyell Collection Notes © The Geological Society of London 2013 Downloaded from http://sp.lyellcollection.org/ by guest on March 25, 2013 The petroleum potential of the Riphean–Vendian succession of southern East Siberia JAMES P. HOWARD*, OLGA K. BOGOLEPOVA, ALEXANDER P. GUBANOV & MARCELA GO´ MEZ-PE´ REZ CASP, West Building, 181a Huntingdon Road, Cambridge CB3 0DH, UK *Corresponding author (e-mail: [email protected]) Abstract: The Siberian Platform covers an area of c.