What Drives Glacial Cycles Combined
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Late Pliocene Climate Variability on Milankovitch to Millennial Time Scales: a High-Resolution Study of MIS100 from the Mediterranean
Palaeogeography, Palaeoclimatology, Palaeoecology 228 (2005) 338–360 www.elsevier.com/locate/palaeo Late Pliocene climate variability on Milankovitch to millennial time scales: A high-resolution study of MIS100 from the Mediterranean Julia Becker *, Lucas J. Lourens, Frederik J. Hilgen, Erwin van der Laan, Tanja J. Kouwenhoven, Gert-Jan Reichart Department of Stratigraphy–Paleontology, Faculty of Earth Sciences, Utrecht University, Budapestlaan 4, 3584 CD Utrecht, Netherlands Received 10 November 2004; received in revised form 19 June 2005; accepted 22 June 2005 Abstract Astronomically tuned high-resolution climatic proxy records across marine oxygen isotope stage 100 (MIS100) from the Italian Monte San Nicola section and ODP Leg 160 Hole 967A are presented. These records reveal a complex pattern of climate fluctuations on both Milankovitch and sub-Milankovitch timescales that oppose or reinforce one another. Planktonic and benthic foraminiferal d18O records of San Nicola depict distinct stadial and interstadial phases superimposed on the saw-tooth pattern of this glacial stage. The duration of the stadial–interstadial alterations closely resembles that of the Late Pleistocene Bond cycles. In addition, both isotopic and foraminiferal records of San Nicola reflect rapid changes on timescales comparable to that of the Dansgard–Oeschger (D–O) cycles of the Late Pleistocene. During stadial intervals winter surface cooling and deep convection in the Mediterranean appeared to be more intense, probably as a consequence of very cold winds entering the Mediterranean from the Atlantic or the European continent. The high-frequency climate variability is less clear at Site 967, indicating that the eastern Mediterranean was probably less sensitive to surface water cooling and the influence of the Atlantic climate system. -
Science Journals — AAAS
SCIENCE ADVANCES | RESEARCH ARTICLE CLIMATOLOGY 2017 © The Authors, some rights reserved; Human-induced changes in the distribution of rainfall exclusive licensee American Association 1,2 2 for the Advancement Aaron E. Putnam * and Wallace S. Broecker of Science. Distributed under a Creative ’ A likely consequence of global warming will be the redistribution of Earth s rain belts, affecting water availability Commons Attribution ’ for many of Earth s inhabitants. We consider three ways in which planetary warming might influence the global NonCommercial distribution of precipitation. The first possibility is that rainfall in the tropics will increase and that the subtropics License 4.0 (CC BY-NC). and mid-latitudes will become more arid. A second possibility is that Earth’s thermal equator, around which the planet’s rain belts and dry zones are organized, will migrate northward. This northward shift will be a consequence of the Northern Hemisphere, with its large continental area, warming faster than the Southern Hemisphere, with its large oceanic area. A third possibility is that both of these scenarios will play out simultaneously. We review paleoclimate evidence suggesting that (i) the middle latitudes were wetter during the last glacial maximum, (ii) a northward shift of the thermal equator attended the abrupt Bølling-Allerød climatic transition ~14.6 thousand years ago, and (iii) a southward shift occurred during the more recent Little Ice Age. We also inspect trends in Downloaded from seasonal surface heating between the hemispheres over the past several decades. From these clues, we predict that there will be a seasonally dependent response in rainfall patterns to global warming. -
Milankovitch and Sub-Milankovitch Cycles of the Early Triassic Daye Formation, South China and Their Geochronological and Paleoclimatic Implications
Gondwana Research 22 (2012) 748–759 Contents lists available at SciVerse ScienceDirect Gondwana Research journal homepage: www.elsevier.com/locate/gr Milankovitch and sub-Milankovitch cycles of the early Triassic Daye Formation, South China and their geochronological and paleoclimatic implications Huaichun Wu a,b,⁎, Shihong Zhang a, Qinglai Feng c, Ganqing Jiang d, Haiyan Li a, Tianshui Yang a a State Key Laboratory of Geobiology and Environmental Geology, China University of Geosciences, Beijing 100083, China b School of Ocean Sciences, China University of Geosciences (Beijing), Beijing 100083 , China c State Key Laboratory of Geological Processes and Mineral Resources, China University of Geosciences, Wuhan 430074, China d Department of Geoscience, University of Nevada, Las Vegas, NV 89154, USA article info abstract Article history: The mass extinction at the end of Permian was followed by a prolonged recovery process with multiple Received 16 June 2011 phases of devastation–restoration of marine ecosystems in Early Triassic. The time framework for the Early Received in revised form 25 November 2011 Triassic geological, biological and geochemical events is traditionally established by conodont biostratigra- Accepted 2 December 2011 phy, but the absolute duration of conodont biozones are not well constrained. In this study, a rock magnetic Available online 16 December 2011 cyclostratigraphy, based on high-resolution analysis (2440 samples) of magnetic susceptibility (MS) and Handling Editor: J.G. Meert anhysteretic remanent magnetization (ARM) intensity variations, was developed for the 55.1-m-thick, Early Triassic Lower Daye Formation at the Daxiakou section, Hubei province in South China. The Lower Keywords: Daye Formation shows exceptionally well-preserved lithological cycles with alternating thinly-bedded mud- Early Triassic stone, marls and limestone, which are closely tracked by the MS and ARM variations. -
Plio-Pleistocene Imprint of Natural Climate Cycles in Marine Sediments
Lebreiro, S. M. 2013. Plio-Pleistocene imprint of natural climate cycles in marine sediments. Boletín Geológico y Minero, 124 (2): 283-305 ISSN: 0366-0176 Plio-Pleistocene imprint of natural climate cycles in marine sediments S. M. Lebreiro Instituto Geológico y Minero de España, OPI. Dept. de Investigación y Prospectiva Geocientífica. Calle Ríos Rosas, 23, 28003-Madrid, España [email protected] ABSTracT The response of Earth to natural climate cyclicity is written in marine sediments. The Earth is a complex system, as is climate change determined by various modes, frequency of cycles, forcings, boundary conditions, thresholds, and tipping elements. Oceans act as climate change buffers, and marine sediments provide archives of climate conditions in the Earth´s history. To read climate records they must be well-dated, well-calibrated and analysed at high-resolution. Reconstructions of past climates are based on climate variables such as atmospheric composi- tion, temperature, salinity, ocean productivity and wind, the nature and quality which are of the utmost impor- tance. Once the palaeoclimate and palaeoceanographic proxy-variables of past events are well documented, the best results of modelling and validation, and future predictions can be obtained from climate models. Neither the mechanisms for abrupt climate changes at orbital, millennial and multi-decadal time scales nor the origin, rhythms and stability of cyclicity are as yet fully understood. Possible sources of cyclicity are either natural in the form of internal ocean-atmosphere-land interactions or external radioactive forcing such as solar irradiance and volcanic activity, or else anthropogenic. Coupling with stochastic resonance is also very probable. -
An Observational Study of the Tropical Tropospheric Circulation
An Observational Study of the Tropical Tropospheric Circulation Ioana M. Dima A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy University of Washington 2005 Program Authorized to Offer Degree: Department of Atmospheric Sciences University of Washington Graduate School This is to certify that I have examined this copy of a doctoral dissertation by Ioana M. Dima and have found that it is complete and satisfactory in all respects, and that any and all revisions by the final examining committee have been made. Chair of the Supervisory Committee: ______________________________________________________________________ John M. Wallace Reading Committee: ______________________________________________________________________ John M. Wallace ______________________________________________________________________ Dennis L. Hartmann ______________________________________________________________________ Edward S. Sarachik Date: ______________________ In presenting this dissertation in partial fulfillment of the requirements for the doctoral degree at the University of Washington, I agree that the Library shall make its copies freely available for inspection. I further agree that extensive copying of the dissertation is allowable only for scholarly purposes, consistent with “fair use” as prescribed in the U.S. Copyright Law. Requests for copying or reproduction of this dissertation may be referred to Proquest Information and Learning, 300 North Zeeb Road, Ann Arbor, MI 48106-1346, to whom the -
The Global Monsoon Across Time Scales Mechanisms And
Earth-Science Reviews 174 (2017) 84–121 Contents lists available at ScienceDirect Earth-Science Reviews journal homepage: www.elsevier.com/locate/earscirev The global monsoon across time scales: Mechanisms and outstanding issues MARK ⁎ ⁎ Pin Xian Wanga, , Bin Wangb,c, , Hai Chengd,e, John Fasullof, ZhengTang Guog, Thorsten Kieferh, ZhengYu Liui,j a State Key Laboratory of Mar. Geol., Tongji University, Shanghai 200092, China b Department of Atmospheric Sciences, School of Ocean and Earth Science and Technology, University of Hawaii at Manoa, Honolulu, HI 96825, USA c Earth System Modeling Center, Nanjing University of Information Science and Technology, Nanjing 210044, China d Institute of Global Environmental Change, Xi'an Jiaotong University, Xi'an 710049, China e Department of Earth Sciences, University of Minnesota, Minneapolis, MN 55455, USA f CAS/NCAR, National Center for Atmospheric Research, 3090 Center Green Dr., Boulder, CO 80301, USA g Key Laboratory of Cenozoic Geology and Environment, Institute of Geology and Geophysics, Chinese Academy of Sciences, P.O. Box 9825, Beijing 100029, China h Future Earth, Global Hub Paris, 4 Place Jussieu, UPMC-CNRS, 75005 Paris, France i Laboratory Climate, Ocean and Atmospheric Studies, School of Physics, Peking University, Beijing 100871, China j Center for Climatic Research, University of Wisconsin Madison, Madison, WI 53706, USA ARTICLE INFO ABSTRACT Keywords: The present paper addresses driving mechanisms of global monsoon (GM) variability and outstanding issues in Monsoon GM science. This is the second synthesis of the PAGES GM Working Group following the first synthesis “The Climate variability Global Monsoon across Time Scales: coherent variability of regional monsoons” published in 2014 (Climate of Monsoon mechanism the Past, 10, 2007–2052). -
Bjerknes, 1966: a Possible Response of the Atmospheric Hadley
A possible response of the atmospheric Hadley circulation to equatorial anomalies of ocean temperature By J. BJERKNES, University of California, Los Angeles (Manuscript received January 18, 1966) ABSTRACT Weakness and temporary elimination of the equatorial easterly winds over the eastern and central Pacific in late 1957 and early 1958 brought about a brief cessation of equatorial upwelling which in turn caused the occurrence of above-normal surface water temperatures in the tropical Pacific from the American coast westward to the dateline. This sudden introduction of a large anomalous heat source for the atmosphere intensified its thermodynamic circulation, especially in the wintertime (northern) hemisphere. Record intensity of the westerlies resulted in the eastern North Pacific. The anomalous depth of the Low in the Gulf of Alaska had the downwind effect of weakening the Iceland Low and setting the stage for a cold winter in northern Europe. Introduction tion run faster than normal in the affected longitude sector and transport absolute angular The concept of the Hadley circulation as used momentum to the subtropical jet stream at a in this article refers to the rising motion at the faster rate than normal. The continued pole- thermal equator and simultaneous sinking mo- ward flux of absolute angular momentum and tion in the belt of subtropical highs mutually the downward flux of the same in the belt of connected by the equatorward component of surface westerlies can then also be assumed to the tradewinds in the lower troposphere and by maintain stronger than normal westerlies in the compensating flow away from the equator in middle latitudes of t,he longitude sector under the upper troposphere. -
What the Geological Record Tells Us About Our Present and Future Climate
Downloaded from http://jgs.lyellcollection.org/ by guest on October 2, 2021 Perspective Journal of the Geological Society https://doi.org/10.1144/jgs2020-239 | Vol. 178 | 2020 | jgs2020-239 Geological Society of London Scientific Statement: what the geological record tells us about our present and future climate Caroline H. Lear1*, Pallavi Anand2, Tom Blenkinsop1, Gavin L. Foster3, Mary Gagen4, Babette Hoogakker5, Robert D. Larter6, Daniel J. Lunt7, I. Nicholas McCave8, Erin McClymont9, Richard D. Pancost10, Rosalind E.M. Rickaby11, David M. Schultz12, Colin Summerhayes13, Charles J.R. Williams7 and Jan Zalasiewicz14 1 School of Earth and Environmental Sciences, Cardiff University, Main Building, Park Place, CF10 3AT, UK 2 School of Environment Earth and Ecosystem Sciences, Open University, Walton Hall, Milton Keynes MK7 6AA, UK 3 National Oceanography Centre Southampton, University of Southampton, European Way, Southampton, SO14 3ZH, UK 4 Geography Department, Swansea University, Swansea, SA2 8PP, UK 5 Lyell Centre, Heriot Watt University, Research Avenue South, Edinburgh, EH14 4AP, UK 6 British Antarctic Survey, British Antarctic Survey, High Cross, Madingley Road, Cambridge CB3 0ET, UK 7 School of Geographical Sciences, University of Bristol, University Road, Bristol, BS8 1SS, UK 8 Department of Earth Sciences, University of Cambridge, Downing Street, Cambridge, CB2 3EQ, UK 9 Department of Geography, Durham University, Lower Mountjoy, South Road, Durham, DH1 3LE, UK 10 School of Earth Sciences, University of Bristol, Wills Memorial -
The Intertropical Convergence Zone (ITCZ)
9/19/2018 Dr. Hoch RGPL 103 Global Cities: Planning and Development Dr. Hoch Email: [email protected] 1 9/19/2018 2 9/19/2018 Earth’s Orbit Around Sun Aphelion Perihelion July 6 (12:00) Jan 3 (00:00) 152.5 Million Km 147.5 Mil. Km EARTH SUN Dates for 2010 Earth Rotation Earth’s axis N Pole Ecliptic Plane (Plane of earth revolution around sun) 23 1/2° 3 9/19/2018 Northern Hemisphere Seasons • Summer • North pole tilted toward Sun • Days are longer than the nights • Get more energy - higher temperatures •Fall • Neither pole tilted toward the Sun • Days about equal with nights • Less energy than in the summer • Cooler temperatures Northern Hemisphere Seasons cont. •Winter • North pole tilted away from the Sun • Days shorter than the nights • Get less energy-Cold temperatures • Spring • Neither pole tilted toward the Sun • Days about equal to nights • More energy than winter- Warmer temperatures 4 9/19/2018 Global regions • Tropics (23 ½°N ‐ 23 ½°S) • Low latitudes (30°N ‐ 30°S) • Mid latitudes (30°N ‐ 60°N and 30°S ‐ 60°S ) • High latitudes (60°N ‐ 90°N and 60°S ‐ 90°S ) 5 9/19/2018 Key positional relationships •Tropic of Cancer - 23 1/2° N •Highest latitude in the Northern Hemisphere that the suns vertical rays ever reach •Tropic of Capricorn- 23 1/2° S •Highest latitude in the Southern Hemisphere that the suns vertical rays ever reach •Arctic circle- 66 1/2° N •24 hrs of daylight-summer solstice •24 hrs of darkness at winter solstice •Antarctic circle- 66 1/2° S •24 hrs of daylight-winter solstice •24 hrs of darkness at summer solstice Circle -
Milankovitch Cycles and the Earth's Climate
MILANKOVITCH CYCLES AND THE EARTH'S CLIMATE John Baez Climate Science Seminar California State University Northridge April 26, 2013 Understanding the Earth's climate poses different challenges at different time scales. The Earth has been cooling for at least 15 million years, with glaciers in the Northern Hemisphere for at least 5 million years. Irregular climate cycles have been getting stronger during this time, becoming full-fledged glacial cycles roughly 2.5 million years ago. These cycles lasted roughly 40,000 years at first, and more recently about 100,000 years. Let's zoom out and look at the climate over longer and longer periods of time! NASA Goddard Institute of Space Science Reconstruction of temperature from 73 different records | Marcott et al. 8 temperature reconstructions | Global Warming Art Recent glacial cycles | Global Warming Art Oxygen isotope measurements of benthic forams, Lisiecki and Raymo The Pliocene began 5.3 million years ago; the Pleistocene 2.6 million years ago. Oxygen isotope measurements of benthic forams, Zachos et al. I Why did it suddenly get colder, with the Antarctic becoming covered with ice, 34 million years ago? I Why did the Antarctic thaw 25 million years ago, then reglaciate 15 million years ago? I Why are glacial cycles becoming more intense, starting around 5 million years ago? I Why did they have an average `period' of roughly 41,000 years at first, and then switch to a period of roughly 100,000 years about 1 million years ago? I Why does the Earth tend to slowly cool and then suddenly warm within -
Late Quaternary Changes in Climate
SE9900016 Tecnmcai neport TR-98-13 Late Quaternary changes in climate Karin Holmgren and Wibjorn Karien Department of Physical Geography Stockholm University December 1998 Svensk Kambranslehantering AB Swedish Nuclear Fuel and Waste Management Co Box 5864 SE-102 40 Stockholm Sweden Tel 08-459 84 00 +46 8 459 84 00 Fax 08-661 57 19 +46 8 661 57 19 30- 07 Late Quaternary changes in climate Karin Holmgren and Wibjorn Karlen Department of Physical Geography, Stockholm University December 1998 Keywords: Pleistocene, Holocene, climate change, glaciation, inter-glacial, rapid fluctuations, synchrony, forcing factor, feed-back. This report concerns a study which was conducted for SKB. The conclusions and viewpoints presented in the report are those of the author(s) and do not necessarily coincide with those of the client. Information on SKB technical reports fromi 977-1978 {TR 121), 1979 (TR 79-28), 1980 (TR 80-26), 1981 (TR81-17), 1982 (TR 82-28), 1983 (TR 83-77), 1984 (TR 85-01), 1985 (TR 85-20), 1986 (TR 86-31), 1987 (TR 87-33), 1988 (TR 88-32), 1989 (TR 89-40), 1990 (TR 90-46), 1991 (TR 91-64), 1992 (TR 92-46), 1993 (TR 93-34), 1994 (TR 94-33), 1995 (TR 95-37) and 1996 (TR 96-25) is available through SKB. Abstract This review concerns the Quaternary climate (last two million years) with an emphasis on the last 200 000 years. The present state of art in this field is described and evaluated. The review builds on a thorough examination of classic and recent literature (up to October 1998) comprising more than 200 scientific papers. -
From Isotopes to Temperature, & Influences of Orbital Forcing on Ice
ATM 211 UWHS Climate Science UW Program on Climate change Unit 3: Natural Climate Variability B. Paleoclimate on Millennial Timescales (Ch. 12 & 14) a. Recent Ice Ages b. Milankovitch Cycles Grade Level 9-12 Overview Time Required This module provides a hands-on learning experience where students Preparation 4-6 hours to become familiar with will review ice core isotope records to determine the isotope-temperature scaling Excel data, Online Orbital Applet, and their relationship to orbital variations. The objective of this module is for and PowerPoint students to learn how water isotopes are used to infer temperature changes back 3-5 hours Class Time (All three labs) in time, and how orbital variations (Milankovitch forcing) control the multi- 5 minute pre survey 25 min PowerPoint topic millennial scale climate variability. In addition, students will learn about how background & Lab 1 introduction climate feedbacks (CO2, sea ice, iron-fertilization) can amplify/moderate 25 min Lapse Rate exercise temperature changes that cannot be explained solely by orbital forcing. 40 min Compile class data and apply to Dome C ice core 30 min Lab 2 (Excel calculations for The module is divided into three independent parts, allowing teachers to Rayleigh Distillation) OPTIONAL pick and choose the sections they wish to cover when. An overview of the three 50 min Lab 3 Worksheets on Orbital changes and Milankovitch labs is described below. 30 min Lab 4 (Excel calculations for CO2 and Orbital temp changes) Lab 1: From Isotopes to Temperature: The students will begin by finding 5 minute post survey ice core/snow pit locations in Antarctica and making predictions about how temperature might change with elevation and distance from the ocean.