SIBERIAN TRAPS SULFUR AND CARBON DEGASSING AND END-PERMIAN CLIMATE FEEDBACKS

2016 ◽  
Author(s):  
Benjamin Alexander Black ◽  
◽  
Ryan Neely ◽  
Jean-Francois Lamarque ◽  
Jeffrey Kiehl ◽  
...  
Author(s):  
David J Beerling ◽  
Michael Harfoot ◽  
Barry Lomax ◽  
John A Pyle

The discovery of mutated palynomorphs in end-Permian rocks led to the hypothesis that the eruption of the Siberian Traps through older organic-rich sediments synthesized and released massive quantities of organohalogens, which caused widespread O 3 depletion and allowed increased terrestrial incidence of harmful ultraviolet-B radiation (UV-B, 280–315 nm; Visscher et al . 2004 Proc. Natl Acad. Sci. USA 101 , 12 952–12 956). Here, we use an extended version of the Cambridge two-dimensional chemistry–transport model to evaluate quantitatively this possibility along with two other potential causes of O 3 loss at this time: (i) direct effects of HCl release by the Siberian Traps and (ii) the indirect release of organohalogens from dispersed organic matter. According to our simulations, CH 3 Cl released from the heating of coals alone caused comparatively minor O 3 depletion (5–20% maximum) because this mechanism fails to deliver sufficiently large amounts of Cl into the stratosphere. The unusual explosive nature of the Siberian Traps, combined with the direct release of large quantities of HCl, depleted the model O 3 layer in the high northern latitudes by 33–55%, given a main eruptive phase of less than or equal to 200 kyr. Nevertheless, O 3 depletion was most extensive when HCl release from the Siberian Traps was combined with massive CH 3 Cl release synthesized from a large reservoir of dispersed organic matter in Siberian rocks. This suite of model experiments produced column O 3 depletion of 70–85% and 55–80% in the high northern and southern latitudes, respectively, given eruption durations of 100–200 kyr. On longer eruption time scales of 400–600 kyr, corresponding O 3 depletion was 30–40% and 20–30%, respectively. Calculated year-round increases in total near-surface biologically effective (BE) UV-B radiation following these reductions in O 3 layer range from 30–60 (kJ m −2  d −1 ) BE up to 50–100 (kJ m −2  d −1 ) BE . These ranges of daily UV-B doses appear sufficient to exert mutagenic effects on plants, especially if sustained over tens of thousands of years, unlike either rising temperatures or SO 2 concentrations.


2021 ◽  
Author(s):  
Linda Elkins-Tanton ◽  
Steven Grasby ◽  
Benjamin Black ◽  
Roman Veselovskiy ◽  
Omid Ardakani ◽  
...  

<p>The Permo-Triassic Extinction was the most severe in Earth history. The Siberian Traps eruptions are strongly implicated in the global atmospheric changes that likely drove the extinction. A sharp negative carbon isotope excursion coincides within geochronological uncertainty with the oldest dated rocks from the Norilsk section of the Siberian flood basalts. The source of this light carbon has been debated for decades.</p><p>We focused on the voluminous volcaniclastic rocks of the Siberian Traps, relatively unstudied as potential carriers of carbon-bearing gases. Over six field seasons we collected rocks from across the Siberian platform and show the first direct evidence that the earliest eruptions particularly in the southern part of the province burned large volumes of a combination of vegetation and coal. Samples from the Maymecha-Kotuy region, from the Nizhnyaya Tunguska, Podkamennaya Tunguska, and Angara Rivers all show evidence of high-temperature organic matter carbonization and combustion.</p><p>Field evidence indicates a process in which ascending magmas entrain xenoliths of coal and carbonaceous sediments that are carbonized in the subsurface and also combusted either through reduction of magmas or when exposed to the atmosphere. We demonstrate that the volume and composition of organic matter interactions with magmas may explain the global carbon isotope signal, and have significantly driven the extinction.</p>


2021 ◽  
Author(s):  
E. Dietze ◽  
A. Andreev ◽  
K. Mangelsdorf ◽  
M. Theuerkauf ◽  
C. Kraamwinkel ◽  
...  

2018 ◽  
Vol 11 (12) ◽  
pp. 949-954 ◽  
Author(s):  
Benjamin A. Black ◽  
Ryan R. Neely ◽  
Jean-François Lamarque ◽  
Linda T. Elkins-Tanton ◽  
Jeffrey T. Kiehl ◽  
...  
Keyword(s):  

Lithos ◽  
2005 ◽  
Vol 79 (3-4) ◽  
pp. 407-424 ◽  
Author(s):  
Andrew D. Saunders ◽  
Richard W. England ◽  
Marc K. Reichow ◽  
Rosalind V. White

2011 ◽  
Vol 4 (3) ◽  
pp. 723-757 ◽  
Author(s):  
◽  
N. Bellouin ◽  
W. J. Collins ◽  
I. D. Culverwell ◽  
P. R. Halloran ◽  
...  

Abstract. We describe the HadGEM2 family of climate configurations of the Met Office Unified Model, MetUM. The concept of a model "family" comprises a range of specific model configurations incorporating different levels of complexity but with a common physical framework. The HadGEM2 family of configurations includes atmosphere and ocean components, with and without a vertical extension to include a well-resolved stratosphere, and an Earth-System (ES) component which includes dynamic vegetation, ocean biology and atmospheric chemistry. The HadGEM2 physical model includes improvements designed to address specific systematic errors encountered in the previous climate configuration, HadGEM1, namely Northern Hemisphere continental temperature biases and tropical sea surface temperature biases and poor variability. Targeting these biases was crucial in order that the ES configuration could represent important biogeochemical climate feedbacks. Detailed descriptions and evaluations of particular HadGEM2 family members are included in a number of other publications, and the discussion here is limited to a summary of the overall performance using a set of model metrics which compare the way in which the various configurations simulate present-day climate and its variability.


Science ◽  
1992 ◽  
Vol 258 (5089) ◽  
pp. 1760-1763 ◽  
Author(s):  
I. H. Campbell ◽  
G. K. Czamanske ◽  
V. A. Fedorenko ◽  
R. I. Hill ◽  
V. Stepanov

2008 ◽  
Vol 44 (2) ◽  
pp. 158-174 ◽  
Author(s):  
Yu. S. Genshaft ◽  
L. V. Tikhonov ◽  
V. M. Ladygin ◽  
E. M. Spiridonov ◽  
A. Ya. Saltykovskii
Keyword(s):  

Sign in / Sign up

Export Citation Format

Share Document