Milankovitch Cycles. Milankovitch Cycles. Milankovitch Cycles. Milankovitch Cycles. Milankovitch Cycles. Milankovitch Cycles.

Similar documents
Glacial Cycles: from Aristotle to Hogg and Back to Budyko

IMA. Celestial Influences on Glacial Cycles. Math and Climate Seminar

Recent Developments in the Theory of Glacial Cycles

Energy Balance Models

Math /29/2014. Richard McGehee, University of Minnesota 1. Math 5490 September 29, Glacial Cycles

Ice Ages and Changes in Earth s Orbit. Topic Outline

Our Geologic Backdrop: Ice Age Cycles

Today s Climate in Perspective: Hendrick Avercamp ( ) ~1608; Rijksmuseum, Amsterdam

lecture 12 Paleoclimate

An Orbital Theory for Glacial Cycles

REVISITING THE ANALOGUE FOR THE COMING ICE AGE

DRAFT. arxiv: v1 [astro-ph.ep] 13 Oct 2015 A SIMPLE METHOD FOR CALCULATING A PLANET S MEAN ANNUAL INSOLATION BY LATITUDE

ENIGMA: something that is mysterious, puzzling, or difficult to understand.

Paleoclimatology ATMS/ESS/OCEAN 589. Abrupt Climate Change During the Last Glacial Period

A brief lesson on oxygen isotopes. more ice less ice

The Ice Age sequence in the Quaternary

ATMS 321: Natural Climate Variability Chapter 11

Solar Insolation and Earth Radiation Budget Measurements

Pleistocene Glaciations

Variations in the Earth's Orbit: Pacemaker of the Ice Ages

Chapter Causes of Climate Change Part I: Milankovitch Cycles

A Paleoclimate Model of Ice-Albedo Feedback Forced by Variations in Earth s Orbit

TOPIC #12 NATURAL CLIMATIC FORCING

Natural Climate Variability: Longer Term

Ice Age research. Milankovitch cycles, Milankovitch curves, Milankovitch insolation, Milankovitch theory, Milankovitch hypothesis.?

Agronomy 406 World Climates

THE TENDENCY OF CLIMATE CHANGE OVER THE PAST SEVERAL MILLIONS OF YEARS AND THE CURRENT INTERGLACIAL DURATION. V.A. Dergachev

Lecture 10: Seasons and Ice Age. Earth s Orbit and Its Variations. Perihelion and Aphelion. Tilt Produces Seasons

The ocean s overall role in climate

Orbital-Scale Interactions in the Climate System. Speaker:

An Introduction to Energy Balance Models

Welcome to ATMS 111 Global Warming.

The Case for Anthropogenic Warming

The Influence of Obliquity on Quaternary Climate

Lab 3. Orbital Configurations and Milankovitch Cycles

Glacial-Interglacial Cycling: Ice, orbital theory, and climate. Dr. Tracy M. Quan IMCS

Climate and Environment

Speleothems and Climate Models

Introduction to Quaternary Geology (MA-Modul 3223) Prof. C. Breitkreuz, SS2012, TU Freiberg

Seasonal & Diurnal Temp Variations. Earth-Sun Distance. Eccentricity 2/2/2010. ATS351 Lecture 3

Milankovitch Theory of the Ice Ages

Dynamics of Energy Balance Models for Planetary Climate

Ice on Earth: An overview and examples on physical properties

November 20, NOTES ES Rotation, Rev, Tilt.notebook. vertically. night. night. counterclockwise. counterclockwise. East. Foucault.

Quarternary Climate Variations

Father of Glacial theory. First investigations of glaciers and mountain geology,

TOPIC #12. Wrap Up on GLOBAL CLIMATE PATTERNS

1. SOLAR GEOMETRY, EXTRATERRESTRIAL IRRADIANCE & INCIDENCE ANGLES

Geos Orogeny-mountain building: existing mountain belts are the result of Cenozoic tectonics. Cenozoic tectonism and climate.

The Budyko Energy Balance Models of the Earth s Climate

Monday, December 4, 2017 The Pleistocene Glaciations (Chapter 14) Week 14 Assessment, closes Wednesday Dec 6

Chapter 14: The Changing Climate

8. Climate changes Short-term regional variations

The Pleistocene Ice Ages

Lecture 0 A very brief introduction

MAR110 LECTURE #28 Climate Change I

SOLAR FORCING. Variations in Solar Emissivity

Questions we would like to learn (scattered through the whole lecture)

NATS 101 Section 13: Lecture 7. The Seasons

"Global Warming Beer" Taps Melted Arctic Ice (UPDATE)

Geol. 656 Isotope Geochemistry

WELCOME TO PERIOD 14:CLIMATE CHANGE. Homework #13 is due today.

Chp Spectral analysis a. Requires that the climate record must be at least 4 times longer than the cycled analyzed

What s up with Earth s Climate? David Archer Department of the Geophysical Sciences University of Chicago

How long will the precession epoch last in terms of Pleistocene glacial cycles?

Fundamental Principles and Results of a New Astronomic Theory of Climate Change

ASD4: Orbital Perturbations

Climate Change: Past and Future ERTH 303, 3 December, 2009

Second-Order Draft Chapter 6 IPCC WG1 Fourth Assessment Report

Extent of Periglacial = Global Permafrost Permafrost: Soil and/or rock where temperatures remain below 0 degrees C for 2 or more years.

MAR110 LECTURE #22 Climate Change

Simulation of Long-Term Future Climate Changes with the Green McGill Paleoclimate Model: The Next Glacial Inception

Meteorology Practice Test

In the summer of 1836, Agassiz stayed with a well known geologist (Chapentier) who had been convinced by a collegue (Venetz) of extensive Alpine

Lecture 7: Natural Climate Change. Instructor: Prof. Johnny Luo.

Pacific Northwest Quaternary Climate History: Very Short Version 2:00

The following terms are some of the vocabulary that students should be familiar with in order to fully master this lesson.

Let s make a simple climate model for Earth.

Extremes of Weather and the Latest Climate Change Science. Prof. Richard Allan, Department of Meteorology University of Reading

Lecture 7: The Monash Simple Climate

Paleoceanography II Telluric Effects on Oceanography

Lessons from the past: interpreting the paleorecord & modelling

Solar variability and Climate Change

Topic 6: Insolation and the Seasons

Physics 115/242 The Kepler Problem

Climate Change. April 21, 2009

Chapter 6: Global Climate Change

The Role of Mathematics in Understanding the Earth s Climate. Andrew Roberts

A User s Guide to the Sky

Earth-Sun Relationships. The Reasons for the Seasons

Package palinsol. August 29, 2016

Development of the Global Environment

Lecture 3: Global Energy Cycle

Today we will discuss global climate: how it has changed in the past, and how the current status and possible future look.

The Tswaing Impact Crater, South Africa: derivation of a long terrestrial rainfall record for the southern mid-latitudes

We re living in the Ice Age!

Modeling the Climatic Response to Orbital Variations

Lecture 21: Glaciers and Paleoclimate Read: Chapter 15 Homework due Thursday Nov. 12. What we ll learn today:! Learning Objectives (LO)

PALEOCEANOGRAPHY, VOL. 3, NO. 5, PAGES , OCTOBER College of Oceanography Oregon State University, Corvallis

Lecture #03. January 20, 2010, Wednesday

Transcription:

Richard McGehee Temperatures in the Cenozoic ra Seminar on the Mathematics of Climate Change School of Mathematics March 4, 9 http://www.tqnyc.org/nyc5141/beginningpage.html Hansen, et al, 8, p. 7 Recent Temperature Cycles What Causes Glacial Cycles? 45 4 35 3 kiloyear bp 5 15 1 5 Widely Accepted Hypothesis 4 - -4-6 -8-1 tem perature The glacial cycles are driven by the variations in the arth s orbit (), causing a variation in incoming solar radiation (insolation). This hypothesis is widely accepted, but also widely regarded as insufficient to explain the observations. Note the period of about 1 kyr. The additional hypothesis is that there are feedback mechanisms that amplify the Milankovitch cycles. What these feedbacks are and how they work is not fully understood. Heat Balance ccentricity Historical Overview of Climate Change Science, IPCC AR4, p.96 http://ipcc-wg1.ucar.edu/wg1/report/ar4wg1_print_ch1.pdf http://www.crrel.usace.army.mil/permafrosttunnel/ice_age_arth_orbit.jpg 1

Obliquity Precession http://upload.wikimedia.org/wikipedia/commons/6/61/axialtiltobliquity.png http://earthobservatory.nasa.gov/library/giants/milankovitch/milankovitch_.html Perihelion: 91.5x1 6 mi Aphelion: 94.5x1 6 mi Semimajor axis: 93x1 6 mi ccentricity: 1.5/93 =.16 ccentricity Solar output: K Watts Solar intensity at distance r from the sun: K () () Wm Q t = 4π r t Cross section of arth: π r m Kr Global solar input: 4r() t W Total annual solar input ( P = one year (in seconds)): P Kr Kr dt dt = 4r() t 4 r() t P Joules Specific angular momentum (angular momentum per unit mass): Total annual solar input: Ω= r θ m s 1 Kr Kr Kr Kr 4 () 4 4 P P dt θ dt π π = d = θ = r t Ω Ω Ω Mean annual solar input: π Kr Watts PΩ Mean annual solar intensity on the arth s surface: Joules Kepler s Third Law: Derived from Kepler: Mean annual solar intensity: P a 3 1 e aω 3 1 K Ka ˆ a Ka ˆ = = Wm 8PΩ 1 e 1 e a = semimajor axis e = eccentricity π Kr 1 = K Wm P r PΩ Ω 4π 8

Laskar: Ka ˆ 1 e ccentricity The effect due to eccentricity is more significant. Note periods of about 1 Kyr and 4 Kyr. Semi major axis does not change much. Zachos, et al, "Trends, Rhythms, and Aberrations in Global Climate 65 Ma to Present". Science 9 (1), 687. Obliquity Precession Note period of about 41 Kyr. Note period of about 3 Kyr. Zachos, et al, "Trends, Rhythms, and Aberrations in Global Climate 65 Ma to Present". Science 9 (1), 687. Zachos, et al, "Trends, Rhythms, and Aberrations in Global Climate 65 Ma to Present". Science 9 (1), 687. Solar Forcing Solar Forcing (Hays, et al) http://en.wikipedia.org/wiki/milankovitch_cycles Hays, et al, Science 194 (1976), p. 115 3

Hays, et al, Summary Climate Response, Hays, et al 1) Three indices of global climate have been monitored in the record of the past 45, years in Southern Hemisphere ocean-floor sediments. )... climatic variance of these records is concentrated in three discrete spectral peaks at periods of 3,, 4,, and approximately 1, years. These peaks correspond to the dominant periods of the earth's solar orbit, and contain respectively about 1, 5, and 5 percent of the climatic variance. Three different temperature proxies from sea sediment data. Hays, et al, Science 194 (1976), p. 117 Hays, et al, Science 194 (1976), p. 1131 Hays, et al, Summary 3) The 4,-year climatic component has the same period as variations in the obliquity of the earth's axis and retains a constant phase relationship with it. 4) The 3,-year portion of the variance displays the same periods (about 3, and 19, years) as the quasiperiodic precession index. 5) The dominant, 1,-year climatic component has an average period close to, and is in phase with, orbital eccentricity. Unlike the correlations between climate and the higher-frequency orbital variations (which can be explained on the assumption that the climate system responds linearly to orbital forcing), an explanation of the correlation between climate and eccentricity probably requires an assumption of nonlinearity. Hays, et al, Science 194 (1976), p. 1131 Hays, et al, Summary 6) It is concluded that changes in the earth's orbital geometry are the fundamental cause of the succession of Quaternary ice ages. 7) A model of future climate based on the observed orbital-climate relationships, but ignoring i anthropogenic effects, predicts that t the long-term trend over the next seven thousand years is toward extensive Northern Hemisphere glaciation*. *Quoted by George Will, Washington Post, February 5, 9 Hays, et al, Science 194 (1976), p. 1131 Solar Forcing Climate Response (Zachos, et al) A. Power spectrum of climate for the last 4.5 Myr. Note the peaks at 41Kyr and 1 Kyr. B. Power spectrum of climate for the period 5 Myr bp to.5 Myr bp. Note the new peak at 4 Kyr and the split peaks at 16Kyr and 95 Kyr. http://en.wikipedia.org/wiki/milankovitch_cycles Zachos, et al, Science 9 (1), p. 689 4

Temperatures in the Cenozoic ra The cycles have not changed much. ccentricity.7.6.5 eccentricity.4.3..1-5 -45-4 -35-3 -5 - -15-1 -5 megayear Hansen, et al, 8, p. 7 Laskar The cycles have not changed much. Obliquity obliquity 4.5 4 3.5 3.5 The Milankovitch cycles have not changed much, but the climate response has changed a lot. Not just a nonlinear response. But that s a different story. -5-45 -4-35 -3-5 - -15-1 -5 megayear Laskar Hansen, et al, 8, p. 7 Summary Budyko s Ice Line Model The solar forcing, defined as the maximum insolation at latitude 65 N, is dominated by precession, followed by obliquity, followed by eccentricity. The climate response is dominated by eccentricity, followed by obliquity, followed by precession (Hays) OR obliquity, followed by eccentricity, with negligible precession (Zachos). The explanation is that there are nonlinear feedbacks. The total annual solar input depends mainly on eccentricity, and a little bit on semimajor axis, but not at all on obliquity or precession. Is there another explanation? dt R = Qs y T y I T y + H T y dt ( ) ( 1 α ( )( )) ( )( ) ( )( ) The annual global average insolation is Q. The annual average insolation as a function of latitude θ, where y = sinθ, is Qs(y). Q is largely determined by the eccentricity, but s(y) is determined from a combination of the other orbital elements. What is s(y) as a function of obliquity and precession? Stay tuned. 5

Climate Response (Zachos, et al) A. Power spectrum of climate for the last 4.5 Myr. Note the peaks at 41Kyr and 1 Kyr. B. Power spectrum of climate for the period 5 Myr bp to.5 Myr bp. Note the new peak at 4 Kyr and the split peaks at 16Kyr and 95 Kyr. Zachos, et al, Science 9 (1), p. 689 6