Explosive Volcanism As a Key Driver of the Late Paleozoic Ice Age Gerilyn S

Total Page:16

File Type:pdf, Size:1020Kb

Explosive Volcanism As a Key Driver of the Late Paleozoic Ice Age Gerilyn S https://doi.org/10.1130/G46349.1 Manuscript received 19 January 2019 Revised manuscript received 5 April 2019 Manuscript accepted 9 April 2019 © 2019 The Authors. Gold Open Access: This paper is published under the terms of the CC-BY license. Published online 2 May 2019 Explosive volcanism as a key driver of the late Paleozoic ice age Gerilyn S. Soreghan1, Michael J. Soreghan1, and Nicholas G. Heavens2 1School of Geology and Geophysics, University of Oklahoma, 100 E. Boyd Street, Norman, Oklahoma 73019, USA 2Department of Atmospheric and Planetary Sciences, Hampton University, 154 William R. Harvey Way, Hampton, Virginia 23668, USA ABSTRACT whereas pCO2 reached a nadir at ca. 338–334 Ma, Atmospheric CO2 exerts a robust and well-documented control on Earth’s climate, but the peak glaciation occurred ca. 298–295 Ma (Fig. 1). timing of glaciation during the late Paleozoic Ice Age (LPIA; ca. 360–260 Ma) is inconsistent The highest-resolution reconstructions (Montañez with pCO2 reconstructions, hinting at another factor. Stratospheric volcanic aerosols produce et al., 2016) cover a brief interval of the LPIA (ca. a large but temporary negative radiative forcing under modern conditions. Here we examine 311–298 Ma) and show pCO2 lows ca. 305 Ma explosive volcanism over 200 m.y. of Earth history to show that the LPIA corresponded with and 298 Ma, closer to peak ice conditions, but a sustained increase in volcanism in both tropical and extratropical latitudes. A major peak depict pCO2 rising at the apex of the LPIA (ca. in explosive volcanism at ca. 300 Ma likely corresponded to stratospheric sulfur-injecting 298–295 Ma; Fig. 1). Moreover, climate and cli- eruptions at least three to eight times more frequent than at present. This level of volcanism mate–ice sheet models indicate a CO2 glaciation created a steady, negative radiative forcing potentially sufficient to initiate and, most criti- threshold at ~560 ppmv (Lowry et al., 2014), but cally, sustain icehouse conditions, even under increasing levels of pCO2, and helps resolve high-resolution pCO2 reconstructions for the in- discrepancies between glacial timing and CO2 records. Accounting for the radiative forcing terval near peak icehouse (Montañez et al., 2016) effects of CO2 and sulfate indicates that both are required to explain the LPIA, with sulfate show a high-frequency oscillation both above and producing an especially strong effect at peak icehouse ca. 298–295 Ma. Frequent explosive below this threshold. Finally, climate models can- volcanism would have increased atmospheric acidity, enhancing the reactivity of iron in abun- not account for hypothesized equatorial glaciation dant volcanic ash and glacially generated mineral dust, thus strengthening the climate impact (Soreghan et al., 2014) in moderate-elevation up- of volcanism through a marine biological pump further primed by feedback with glaciation. lands without invoking pCO2 levels (<200 ppmv) that would stress modern vegetation (Pagani et al., INTRODUCTION et al., 2016), although causes for CO2 drawdown 2009), calling into question either the data or the Earth’s climate has fluctuated between ice- are disputed. Long-standing research (Berner, modeling. house and greenhouse states, characterized by 2004; Royer et al., 2004) posits the primacy of Decoupling between glaciation and pCO2 the presence or absence of continental ice and the terrestrial carbon cycle, wherein evolution could reflect a hysteresis effect in which higher strongly correlated with variations in pCO2 of plants sequestered CO2 (e.g., Feulner, 2017) positive radiative forcing from insolation and/or (Berner, 2004; Royer et al., 2004; Jagoutz et al., and accelerated silicate weathering. Plant ex- greenhouse gases is required to ablate an ice 2016; McKenzie et al., 2016). The late Paleozoic pansion and CO2 drawdown, however, are asyn- sheet than the negative radiative forcing nec- Ice Age (LPIA; ca. 360–260 Ma) archives the chronous, leading others to propose weathering- essary to form it (Zhuang et al., 2014). How- longest Phanerozoic icehouse, and its sedimen- induced drawdown related to Pangean orogeny ever, such a hysteresis creates a “paradox of late tary record preserves evidence for atmospheric ( Goddéris et al., 2017). Paleo zoic glacioeustasy” (Horton and Poulsen, CO2 intermittently as low as that of Quaternary Although pCO2 was relatively low during 2009, p. 715), in which order-of-magnitude glaciations (Montañez et al., 2007, 2016). Gla- the LPIA, it is difficult to ascribe the LPIA to variations in pCO2 in addition to orbital forc- ciation began in the Late Devonian (Isaacson pCO2 alone. Both enhanced silicate weathering ing are required to generate the glacioeustasy et al., 2008; Lakin et al., 2016); after an Early– and organic carbon burial are negative feedbacks of the LPIA. But an analogous paradox for the Middle Mississippian minimum, glaciation (Walker et al., 1981; Berner, 2004; Krissansen- Miocene Antarctic ice sheet is now ascribed to peaked in the earliest Permian (Fig. 1A; Table Totten and Catling, 2017). Lower pCO2 can oversimplification of ice-sheet geophysics (Gas- DR1 in the GSA Data Repository1). At times, weaken the first effect by reducing precipitation son et al., 2016). Indeed, the ice-sheet hysteresis continental ice reached latitudes as low as 32° and temperature, and the second by reducing net effect was reduced for late Paleozoic simulations (Evans, 2003), and alpine glaciation is hypoth- primary productivity through increased plant res- by introduction of dynamic vegetation (Horton esized for equatorial uplands (Soreghan et al., piration (Pagani et al., 2009; Gerhart and Ward, and Poulsen, 2009). In short, such hysteresis ap- 2014). The LPIA ultimately collapsed—Earth’s 2010), particularly at the higher pO2 levels in- pears to be an emergent property of some mod- only example of icehouse termination on a fully ferred for the late Paleozoic (Royer, 2014). Also, els, and thus fails to explain the shortcomings in vegetated planet (Gastaldo et al., 1996). mismatches persist between reconstructed pCO2 correlation of the glaciation and pCO2 records. Diminishing pCO2 along with lower solar and the glacial record. For example, pCO2 (Foster Here we integrate geologic data and radiative luminosity (Crowley and Baum, 1992) is the et al., 2017) exhibits an ambiguous relationship to calculations to explore the hypothesis that the preferred explanation for the LPIA (Montañez the timing of onset, demise, and peak of the LPIA: onset, acme, and, especially, prolonged extent 1GSA Data Repository item 2019219, detailed methods, supplementary figures and data tables, and associated references, is available online at http://www .geosociety .org /datarepository /2019/, or on request from editing@ geosociety .org. CITATION: Soreghan, G.S., Soreghan, M.J., and Heavens, N.G., 2019, Explosive volcanism as a key driver of the late Paleozoic ice age: Geology, v. 47, p. 600–604, https:// doi .org /10 .1130 /G46349.1 600 www.gsapubs.org | Volume 47 | Number 7 | GEOLOGY | Geological Society of America Downloaded from http://pubs.geoscienceworld.org/gsa/geology/article-pdf/47/7/600/4775200/600.pdf by guest on 24 September 2021 Devonian Mississippian Pennsylvanian Permian Triassic Early Mid. Late Early Mid. Late Early Mid. Late Cisuralian Guad.Lopin. r. Fra. Fam. Tou. Visean Ser. Bas. Mos. Gzh. Sak. Art. Kun. Wu. Ch. Ass Kas. Roa. Wo Cap. s A y eposit 10 s ld 20 glacia 30 40 50 of volcanic deposit Documented 60 Radiometric age probabilit 400 380 360 340 320 300 280 260 240 220 200 2 2000 1600 B 1200 800 Montañez et al. (2016) 400 (ppmv) 200 Foster et al. (2017) 100 Atmospheric CO 400 380 360 340 320 300 280 260 240 220 200 150 s C Other volcanics 100 Pyroclastics Ignimbrites 50 Number of deposit 0 400 380 360 340 320 300 280 260 240 220 200 y 10 D 5 0 vs. last 2.5 m.y. Relative activit 400 380 360 340 320 300 280 260 240 220 200 Age (Ma) Figure 1. Glacial deposits (n = 125), pCO2 (Montañez et al., 2016; Foster et al., 2017), and explosive volcanism (n = 1145) for 400–200 Ma (Cohen et al., 2013; see methods and Tables DR1 and DR2 in the Data Repository [see footnote 1]). A: (Top) Frequency of glacial deposits by stage (sub- stage for stages >10 m.y.). (Base) Relative probability of radioisotopic ages of volcanics. B: Reconstructions of pCO2 (Montañez et al., 2016; Foster et al., 2017). C: Histogram of volcanics by type, binned at 10 m.y. intervals; in key, “Other volcanics” refers to volcanic products other than those coded as pyroclastic or ignimbritic in the original sources. D: Estimated explosive volcanism relative to that of 0–2.5 Ma, inferred from relative number of ignimbrites. Effects of uncertainties indicated with crosses. Empirical (EMP) and saturated (SAT) relate to assumptions about the spreading of ignimbritic material as a function of magnitude (see more details in the Data Repository). Maximum (MAX) and event (EVE) combine the SAT model by counting events by individual eruptions (EVE) versus counting only the largest eruption of a volcano during the Quaternary (MAX). Lower crosses use EVE and EMP models; orange bars use MAX and EMP models; upper crosses use MAX and SAT models. Red line represents value of 1 (average activity of past 2.5 m.y.). Mid.—Middle; Fra.—Frasnian; Fam.—Famennian; Tou.—Tournaisian; Ser.—Serpukhovian; Bas.—Bashkirian; Mos.—Moscovian; Kas.—Kasimovian; Gzh.—Gzhelian; Ass.—Asselian; Sak.—Sakmarian; Art.—Artinskian; Kun.—Kungurian; Guad.—Guadalupian; Rod.—Roadian; Wor.—Wordian; Cap.—Capitanian; Lopin.—Lopingian; Wu.—Wuchiapingian; Ch.—Changhsingian. of the LPIA were driven in part by unusually level binning to reflect the dating resolution of integrates the sub-decadal radiative perturba- intense explosive volcanism prevalent during most deposits. Glacial deposits are reported for tions of multiple, individual eruptions into a sus- Pangean assembly, operating in concert with every stage of the time scale from the Famennian tained forcing on centennial to millennial time pCO2 and indirect forcings related to volcanism.
Recommended publications
  • Cyclicity, Dune Migration, and Wind Velocity in Lower Permian Eolian Strata, Manitou Springs, CO
    Cyclicity, Dune Migration, and Wind Velocity in Lower Permian Eolian Strata, Manitou Springs, CO by James Daniel Pike, B.S. A Thesis In Geology Submitted to the Graduate Faculty of Texas Tech University in Partial Fulfillment of the Requirements for the Degree of MASTER OF SCIENCES Approved Dustin E. Sweet Chair of Committee Tom M. Lehman Jeffery A. Lee Mark Sheridan Dean of the Graduate School August, 2017 Copyright 2017, James D. Pike Texas Tech University, James Daniel Pike, August 2017 ACKNOWLEDGMENTS I would like to extend my greatest thanks to my advisor Dr. Dustin Sweet, who was an excellent advisor during this research. Dr. Sweet was vital throughout the whole process, be it answering questions, giving feedback on figures, and imparting his extensive knowledge of the ancestral Rocky Mountains on me; for this I am extremely grateful. Dr. Sweet allowed me to conduct my own research without looking over my shoulder, but was always available when needed. When I needed a push, Dr. Sweet provided it. I would like to thank my committee memebers, Dr. Lee and Dr. Lehman for providing feedback and for their unique perspectives. I would like to thank Jenna Hessert, Trent Jackson, and Khaled Chowdhury for acting as my field assistants. Their help in taking measurements, collecting samples, recording GPS coordinates, and providing unique perspectives was invaluable. Thank you to Melanie Barnes for allowing me to use her lab, and putting up with the mess I made. This research was made possible by a grant provided by the Colorado Scientific Society, and a scholarship provided by East Texas Geological Society.
    [Show full text]
  • Geologic Map and Upper Paleozoic Stratigraphy of the Marble Canyon Area, Cottonwood Canyon Quadrangle, Death Valley National Park, Inyo County, California
    Geologic Map and Upper Paleozoic Stratigraphy of the Marble Canyon Area, Cottonwood Canyon Quadrangle, Death Valley National Park, Inyo County, California By Paul Stone, Calvin H. Stevens, Paul Belasky, Isabel P. Montañez, Lauren G. Martin, Bruce R. Wardlaw, Charles A. Sandberg, Elmira Wan, Holly A. Olson, and Susan S. Priest Pamphlet to accompany Scientific Investigations Map 3298 2014 U.S. Department of the Interior U.S. Geological Survey Cover View of Marble Canyon area, California, showing dark rocks of Mississippian Indian Springs Formation and Pennsylvanian Bird Spring Formation overlying light rocks of Mississippian Santa Rosa Hills Limestone in middle distance. View is southeast toward Emigrant Wash and Tucki Mountain in distance. U.S. Department of the Interior SALLY JEWELL, Secretary U.S. Geological Survey Suzette M. Kimball, Acting Director U.S. Geological Survey, Reston, Virginia: 2014 For more information on the USGS—the Federal source for science about the Earth, its natural and living resources, natural hazards, and the environment—visit http://www.usgs.gov or call 1–888–ASK–USGS For an overview of USGS information products, including maps, imagery, and publications, visit http://www.usgs.gov/pubprod To order this and other USGS information products, visit http://store.usgs.gov Suggested citation: Stone, P., Stevens, C.H., Belasky, P., Montanez, I.P., Martin, L.G., Wardlaw, B.R., Sandberg, C.A., Wan, E., Olson, H.A., and Priest, S.S., 2014, Geologic map and upper Paleozoic stratigraphy of the Marble Canyon area, Cottonwood Canyon quadrangle, Death Valley National Park, Inyo County, California: U.S. Geological Survey Scientific Investigations Map 3298, scale 1:24,000, 59 p., http://dx.doi.org/10.3133/sim3298.
    [Show full text]
  • Curriculum Vitae
    Carl Simpson 1 CU Museum of Natural History Phone (USA): +1 303-735-5323 University of Colorado, 265 UCB [email protected] Boulder, CO, 8039-0265 http://simpson-carl.github.io @simpson carl Position Assistant Professor, Department of Geological Sciences, University of Colorado, Boulder. Curator of Invertebrate Paleontology, CU Museum, University of Colorado, Boulder. Education Ph.D. Department of Geophysical Sciences, 2006 University of Chicago, Chicago, IL, USA B.A. College of Creative Studies (Biology), June 2000 University of California, Santa Barbara, CA, USA Professional Experience 2015 - 2016 Springer Fellow, Department of Paleobiology, National Museum of Natural History, Smithsonian Institution 2012-2015 Abbott Fellow, Department of Paleobiology, National Museum of Natural His- tory, Smithsonian Institution. 2012 Visiting Scholar, Cooperation and Evolution of Multicellularity program. Kavli In- stitute for Theoretical Physics. 2011 Visiting Scholar Fellowship, National Evolutionary Synthesis Center. 2008-2012 Postdoctoral Researcher, Museum f¨ur Naturkunde, Leibniz Institute for Evo- lution and Biodiversity at the Humbolt University, Berlin. 2006-2008 Research Associate, Department of Biology, Duke University. 2004 Research assistant for John Alroy, the Paleobiology Database, National Center for Ecological Analysis and Synthesis. 2001 Santa Fe Institute Complex Systems Summer School; Budapest, Hungary. 2001 Comparative Invertebrate Embryology. Friday Harbor Marine Laboratories. Fellowships & Grants • Springer Fellowship, \Quantifying the stochastic and deterministic aspects of macroevo- lution" Smithsonian Institution, National Museum of Natural History 2015-2016. • NSF ELT Collaborative Research: \Investigating the Biotic and Paleoclimatic Con- sequences of Dust in the Late Paleozoic." 2013-2017. with Gerilyn Soreghan, Linda Hinnov, Sarah Aciego, and Nicholas Heavens. • Abbott Postdoctoral Fellowship, \The Macroevolution of Bryozoan Polymorphism" Smithsonian Institution, National Museum of Natural History.
    [Show full text]
  • Atmospheric Dust Stimulated Marine Primary Productivity During Earth's
    https://doi.org/10.1130/G46977.1 Manuscript received 14 April 2019 Revised manuscript received 8 November 2019 Manuscript accepted 12 November 2019 © 2019 Geological Society of America. For permission to copy, contact [email protected]. Published online 17 December 2019 Atmospheric dust stimulated marine primary productivity during Earth’s penultimate icehouse Mehrdad Sardar Abadi1, Jeremy D. Owens2, Xiaolei Liu1, Theodore R. Them II2,3, Xingqian Cui4, Nicholas G. Heavens5,6 and Gerilyn S. Soreghan1 1 School of Geosciences, University of Oklahoma, Norman, Oklahoma 73019, USA 2 Department of Earth, Ocean, and Atmospheric Science, Florida State University, and National High Magnetic Field Laboratory, Tallahassee, Florida 32306, USA 3 Department of Geology and Environmental Geosciences, College of Charleston, Charleston, South Carolina 29424, USA 4 Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA 5 Department of Atmospheric and Planetary Sciences, Hampton University, 21 E. Tyler Street, Hampton, Virginia 23668, USA 6 Space Science Institute, 4750 Walnut Street, Suite 205, Boulder, Colorado 80301, USA ABSTRACT BACKGROUND AND METHODS The importance of dust as a source of iron (Fe) for primary production in modern oceans Pennsylvanian–Permian carbonate strata is well studied but remains poorly explored for deep time. Vast dust deposits are well recog- of the study area were located at ∼30°S at the nized from the late Paleozoic and provisionally implicated in primary production through Fe time of deposition, adjacent to the northeastern fertilization. Here, we document dust impacts on marine primary productivity in Moscovian Arabian margin of Gondwana, in relative prox- (Pennsylvanian, ca.
    [Show full text]
  • Download File
    Contents lists available at ScienceDirect Palaeogeography, Palaeoclimatology, Palaeoecology journal homepage: www.elsevier.com/locate/palaeo Pangea B and the Late Paleozoic Ice Age ⁎ D.V. Kenta,b, ,G.Muttonic a Earth and Planetary Sciences, Rutgers University, Piscataway, NJ 08854, USA b Lamont-Doherty Earth Observatory of Columbia University, Palisades, NY 10964, USA c Dipartimento di Scienze della Terra 'Ardito Desio', Università degli Studi di Milano, via Mangiagalli 34, I-20133 Milan, Italy ARTICLE INFO ABSTRACT Editor: Thomas Algeo The Late Paleozoic Ice Age (LPIA) was the penultimate major glaciation of the Phanerozoic. Published compi- Keywords: lations indicate it occurred in two main phases, one centered in the Late Carboniferous (~315 Ma) and the other Late Paleozoic Ice Age in the Early Permian (~295 Ma), before waning over the rest of the Early Permian and into the Middle Permian Pangea A (~290 Ma to 275 Ma), and culminating with the final demise of Alpine-style ice sheets in eastern Australia in the Pangea B Late Permian (~260 to 255 Ma). Recent global climate modeling has drawn attention to silicate weathering CO2 Greater Variscan orogen consumption of an initially high Greater Variscan edifice residing within a static Pangea A configuration as the Equatorial humid belt leading cause of reduction of atmospheric CO2 concentrations below glaciation thresholds. Here we show that Silicate weathering CO2 consumption the best available and least-biased paleomagnetic reference poles place the collision between Laurasia and Organic carbon burial Gondwana that produced the Greater Variscan orogen in a more dynamic position within a Pangea B config- uration that had about 30% more continental area in the prime equatorial humid belt for weathering and which drifted northward into the tropical arid belt as it transformed to Pangea A by the Late Permian.
    [Show full text]
  • Demystifying Climate Change Session 6
    Demystifying Climate Change Session 6 CO2 and Other Greenhouse Gases: Where do they come from? Where do they go? How are they regulated? Burp… OLLI at Illinois Spring 2021 D. H. Tracy [email protected] 418.53 ppm Mar 6, 2021 3/9/21 Climate Change 6 2 Course Outline 1. Building Blocks: Some important concepts 2. Our Goldilocks Earth: a Radiative Balancing Act 3. The Role of the Atmosphere: Greenhouse Gases & Clouds 4. Global Circulation and Dynamics of the Earth System: Oceans, Atmosphere, Biosphere, Cryosphere, People, Lithosphere 5. Natural Variability of the Climate, short and long term. Ice Ages 6. Carbon Dioxide and other Greenhouse Gases: Where do they come from, where do they go, how are they regulated? 7. Impacts and Future Projections for Global Warming -- Uncertainties 8. Amelioration Strategies. The Climate Debate. Policy Options. 3/9/21 Climate Change 6 3 Remember CO2 Saturation? 400ppm CO2 T260K P0.5 L6.4m 100%100% Lesson: Blue: 800 ppm 80% Greenhouse Gases 4 ppm are much more Red: potent, per ppm, 400 ppm 60% when at low 1 ppm concentrations: 40% Not saturated. Absorption of Full Atmosphere Full of Absorption 20% Absorption of Full Atmosphere ofFull Absorption 0% 8.5 9 10 11 12 13 14 15 16 17 18 19 20 Wavelength (mm) Wavelength (m) 3/9/21 Climate Change 6 4 Actual Surface Temperature vs. GH Gas Concentration Doublings Behavior Expected for Linear Increase Minor/Trace Gases ∆T2X TSURF 2x Log Increase Saturation TSKIN setting in 254 K (-2F) Doublings T 0 1 1 1 1 1 /128 x /64 x /32 x /16 x /8 x ¼ x ½x 1x 2x 4x 8x 3/9/21
    [Show full text]
  • Fjord Network in Namibia: a Snapshot Into the Dynamics of the Late Paleozoic Glaciation Pierre Dietrich1,2, Neil P
    https://doi.org/10.1130/G49067.1 Manuscript received 20 October 2020 Revised manuscript received 19 March 2021 Manuscript accepted 21 June 2021 © 2021 The Authors. Gold Open Access: This paper is published under the terms of the CC-BY license. Fjord network in Namibia: A snapshot into the dynamics of the late Paleozoic glaciation Pierre Dietrich1,2, Neil P. Griffis3,4, Daniel P. Le Heron5, Isabel P. Montañez3, Christoph Kettler5, Cécile Robin1 and François Guillocheau1 1 Géosciences Rennes, Université de Rennes, CNRS, UMR 6118, 35000 Rennes, France 2 Department of Geology, University of Johannesburg, Johannesburg 2006, South Africa 3 Department of Earth and Planetary Sciences, University of California, Davis, California 95616, USA 4 Berkeley Geochronology Center, Berkeley, California 94709, USA 5 Department für Geologie, Universität Wien, Althanstraße 14, 1190 Wien, Austria ABSTRACT infer the pace of ice-margin fluctuations and Fjords are glacially carved estuaries that profoundly influence ice-sheet stability by the paleo-ice thickness that once occupied draining and ablating ice. Although abundant on modern high-latitude continental shelves, these fjords. Furthermore, we estimate glacio- fjord-network morphologies have never been identified in Earth’s pre-Cenozoic glacial epochs, isostatic adjustment following deglaciation. hindering our ability to constrain ancient ice-sheet dynamics. We show that U-shaped valleys This work highlights the dynamic nature of in northwestern Namibia cut during the late Paleozoic ice age (LPIA, ca. 300 Ma), Earth’s the LPIA in southwestern Gondwana and the penultimate icehouse, represent intact fjord-network morphologies. This preserved glacial potential for an under-appreciated deep-time morphology and its sedimentary fill permit a reconstruction of paleo-ice thicknesses, glacial carbon and sediment sink that, if valid, would dynamics, and resulting glacio-isostatic adjustment.
    [Show full text]
  • Earth's Outgassing and Climatic Transitions
    Earth’s Outgassing and Climatic Transitions: The Slow Burn Towards Environmental “Catastrophes”? N. Ryan McKenzie1 and Hehe Jiang2 1811-5209/19/0015-0325$2.50 DOI: 10.2138/gselements.15.5.325 n multimillion-year timescales, outgassing from the Earth’s interior Solid Earth carbon degassing occurs at mid-ocean ridges, rifts, provides the principal source of CO2 to the ocean–atmosphere system, volcanic arcs in subduction zones, Owhich plays a fundamental role in shaping the Earth’s baseline climate. orogenic belts, and large igneous Fluctuations in global outgassing have been linked to icehouse–greenhouse provinces (FIG. 1). The global transitions, although uncertainties surround paleo-outgassing fluxes. Here, we volcanic flux of CO2 probably varied significantly throughout discuss how volcanic outgassing and the carbon cycle have evolved in concert geologic time. Changes in subduc- with changes in plate tectonics and biotic evolution. We describe hypotheses tion zone length, in the volume of driving mechanisms for the Paleozoic icehouse–greenhouse climates and of a mantle plume, and/or in the explore how climatic transitions may have influenced past biotic crises and, global oceanic crust production rate can result in at least a two-fold in particular, how variable outgassing rates established the backdrop for increase in volcanic CO2 inputs carbon cycle perturbations to instigate prominent mass extinction events. (Lee et al. 2013). Variation in the CO2 input would, therefore, play KEYWORDS: carbon cycle, outgassing, weathering, climate,
    [Show full text]
  • Newsletter 5.19
    The NJAIChE Newsletter Volume 26 Issue 2 New Jersey’s Oldest Section Greetings from the 2019 Section Officers Arizona Side of the NJ Chairperson: Howard Stamato Section! Chair-Elect: Mike Kolber We have the normal meetings planned on the second Tuesday of each month (Stage House in Scotch Plains or Rolf’s in Warren, NJ) with our executive Treasurer: committee meeting on the first Tuesday at Paisanos at Yasha Zelmanovich Watchung Square Mall. As usual we are always l ooking for volunteers to help Secretary: run the section. Please contact any officer or just Jacqueline Sibbles show up at Paisanos. Important Links Directors: Webpage: https://njaiche.org/ Andrew Soos Laura Turci Facebook: Ken Carlson https://www.facebook.com/njaiche.engineers/ David Greene Director Emeritus: Phil Messina 2 AIChE Newsletter ANNUAL RUTGERS STUDENT AWARDS NJAIChE honored on April 24th the Leader Scholars and Research Scholars from the Rutgers Chemical and Biomolecular Engineering Department. Junior Leader Scholar- Tiffany Yang Junior Research Scholar - Sarah Sonbati Senior Leader Scholar - Carimer Andujar Senior Research Scholar - Ana Nachtigal AIChE Newsletter 3 The Interglacial Period We Are In ICE AGES An ice age is a long period of lower temperatures on the Earth's surface and atmosphere, resulting in the presence of continental and polar ice sheets and alpine glaciers. Earth is currently in the Quaternary glaciation. Although geologists describe the entire time period as an "ice age", in popular culture the term "ice age" is usually associated with just the most recent glacial period or glacials (when the ice sheets were at their maximum extent). Since earth still has ice sheets, geologists consider the Quaternary glaciation to be ongoing, with earth now experiencing an interglacial period.
    [Show full text]
  • CESM Journal Publications
    Abalos, M., W. J. Randel, D. E. Kinnison, and E. Serrano, 2013: Quantifying tracer transport in the tropical lower stratosphere using WACCM. Atmos. Chem. Phys., 13, 10591-10607, doi:10.5194/acp-13-10591-2013. Abe-Ouchi, A., et al., 2015: Ice-sheet configuration in the CMIP5/PMIP3 Last Glacial Maximum experiments. Geosci. Model Dev., 8, 3621-3637. Abbot, D. S., M. Huber, G. Bousquet, and C. C. Walker, 2009: High-CO2 cloud radiative forcing feedback over both land and ocean. Geophys. Res. Lett., L05702, doi:10.1029/2008GL036703. Abiodun, B. J., J. M. Prusa, and W. J. Gutowski, 2008: Implementation of a non-hydrostatic, adaptive-grid dynamics core in CAM3. Part I: Comparison of dynamics cores in aqua-planet simulations. Clim. Dynamics, 31, 795-810 doi:10.1007/s00382-008-0381-y. Abiodun, B. J., W. J. Gutowski, and J. M. Prusa, 2008: Implementation of a non-hydrostatic, adaptive-grid dynamics core in CAM3. Part II: Dynamical Influences on ITCZ behavior and tropical precipitation. Clim. Dynamics, 31, 811-822, doi:10.1007/s00382-008-0382-x. Abiodun, B. J., W. J. Gutowski, A. A. Abatan, and J. M. Prusa, 2011: CAM-EULAG: A non-hydrostatic atmospheric climate model with grid stretching. Acta Geophysica, 59, 1158-1167, doi:10.2478/s1160-011- 0032-2. Acosta Navarro, J. C., V. Varma, I. Riipinen, O. Seland, A. Kirkevag, H. Struthers, T. Iversen, H. -C. Hansson, and A. M. L. Ekman, 2016: Amplification of Arctic warming by past air pollution reductions in Europe. Nature Geoscience, 9, doi:10.1038/ngeo2673. Acosta, R. P., and M.
    [Show full text]
  • Abalos, M., WJ Randel, DE Kinnison, and E. Serrano, 2013
    Abalos, M., W. J. Randel, D. E. Kinnison, and E. Serrano, 2013: Quantifying tracer transport in the tropical lower stratosphere using WACCM. Atmos. Chem. Phys., 13, 10591-10607, doi:10.5194/acp-13-10591-2013. Abe-Ouchi, A., et al., 2015: Ice-sheet configuration in the CMIP5/PMIP3 Last Glacial Maximum experiments. Geosci. Model Dev., 8, 3621-3637. Abbot, D. S., M. Huber, G. Bousquet, and C. C. Walker, 2009: High-CO2 cloud radiative forcing feedback over both land and ocean. Geophys. Res. Lett., L05702, doi:10.1029/2008GL036703. Abiodun, B. J., J. M. Prusa, and W. J. Gutowski, 2008: Implementation of a non-hydrostatic, adaptive-grid dynamics core in CAM3. Part I: Comparison of dynamics cores in aqua-planet simulations. Clim. Dynamics, 31, 795-810 doi:10.1007/s00382-008-0381-y. Abiodun, B. J., W. J. Gutowski, and J. M. Prusa, 2008: Implementation of a non-hydrostatic, adaptive-grid dynamics core in CAM3. Part II: Dynamical Influences on ITCZ behavior and tropical precipitation. Clim. Dynamics, 31, 811-822, doi:10.1007/s00382-008-0382-x. Abiodun, B. J., W. J. Gutowski, A. A. Abatan, and J. M. Prusa, 2011: CAM-EULAG: A non-hydrostatic atmospheric climate model with grid stretching. Acta Geophysica, 59, 1158-1167, doi:10.2478/s1160-011- 0032-2. Acosta Navarro, J. C., V. Varma, I. Riipinen, O. Seland, A. Kirkevag, H. Struthers, T. Iversen, H. -C. Hansson, and A. M. L. Ekman, 2016: Amplification of Arctic warming by past air pollution reductions in Europe. Nature Geoscience, 9, doi:10.1038/ngeo2673. Aghedo, A. M., K.
    [Show full text]
  • Injecting Climate Modeling Into Deep Time Studies
    INSIDE: INJECTING CLIMATE MODELING INTO DEEP TIME STUDIES: IDEAS FOR NEARLY EVERY PROJECT PLUS: PRESIDENT’S COMMENTS, REFLECTIONS ON MAJOR THEMES IN CURRENT STRATIGRAPHY..., UPCOMING SEPM CONFERENCES The Sedimentary Record Special Publication #105 Deposits, Architecture, and Controls of Carbonate Margin, Slope, and Basinal Settings Edited by: Klaas Verwer, Ted E. Playton, and Paul M. (Mitch) Harris Carbonate margin, slope and basinal depositional environments, and their transitions, are highly dynamic and heterogeneous components of carbonate platform systems. Carbonate slopes are of particular interest because they form repositories for volumetrically significant amounts of sediment produced from nearly all carbonate environments, and form the links between shallow-water carbonate platform settings where prevailing in situ factories reside and their equivalent deeper-water settings dominated by resedimentation processes. Slope environments also provide an extensive stratigraphic record that, although is preserved differently than platform-top or basinal strata, can be utilized to unravel the growth evolution, sediment factories, and intrinsic to extrinsic parameters that control carbonate platform systems. In addition to many stimulating academic aspects of carbonate margin, slope, and basinal settings, they are increasingly recognized as significant conventional hydrocarbon reservoirs as well. The papers in this volume, which are drawn from the presentations made at the AAPG Annual Meeting in Long Beach, California (USA), in May 2012,
    [Show full text]