The East Siberian Arctic Shelf: towards further assessment of permafrost-related methane fluxes and role of sea ice

Author:

Shakhova Natalia12,Semiletov Igor123,Sergienko Valentin4,Lobkovsky Leopold5,Yusupov Vladimir6,Salyuk Anatoly3,Salomatin Alexander3,Chernykh Denis3,Kosmach Denis3,Panteleev Gleb1,Nicolsky Dmitry7,Samarkin Vladimir8,Joye Samantha8,Charkin Alexander3,Dudarev Oleg3,Meluzov Alexander5,Gustafsson Orjan9

Affiliation:

1. International Arctic Research Center, University of Alaska Fairbanks, Akasofu Building, Fairbanks, AK 99775-7320, USA

2. Tomsk Polytechnic University, Institute of Natural Resources, Geology and Mineral Exploration, 30 Prospect Lenina, Tomsk, Russia

3. Russian Academy of Sciences, Pacific Oceanological Institute, 43 Baltiiskaya Street, Vladivostok 690041, Russia

4. Russian Academy of Sciences, Institute of Chemistry, 159, 100-Let Vladivostok Prospect, Vladivostok 690022, Russia

5. Russian Academy of Sciences, P.P. Shirshov Oceanological Institute, 36 Nahimovski Prospect, Moscow 117997, Russia

6. Russian Academy of Sciences, Institute on Laser and Information Technologies, 2 Pionerskaya Street, Troitsk 142092, Russia

7. University of Alaska Fairbanks, Geophysical Institute, Snow, Ice and Permafrost, PO Box 757320, Fairbanks, AK 99775-7320, USA

8. Department of Marine Science, University of Georgia Atlanta, 3475 Lenox Road, NE Suite 300, Atlanta, GA 30326-3228, USA

9. Department of Applied Environmental Science and Bolin Centre for Climate Research, Stockholm University, Stockholm 10691, Sweden

Abstract

Sustained release of methane (CH 4 ) to the atmosphere from thawing Arctic permafrost may be a positive and significant feedback to climate warming. Atmospheric venting of CH 4 from the East Siberian Arctic Shelf (ESAS) was recently reported to be on par with flux from the Arctic tundra; however, the future scale of these releases remains unclear. Here, based on results of our latest observations, we show that CH 4 emissions from this shelf are likely to be determined by the state of subsea permafrost degradation. We observed CH 4 emissions from two previously understudied areas of the ESAS: the outer shelf, where subsea permafrost is predicted to be discontinuous or mostly degraded due to long submergence by seawater, and the near shore area, where deep/open taliks presumably form due to combined heating effects of seawater, river run-off, geothermal flux and pre-existing thermokarst. CH 4 emissions from these areas emerge from largely thawed sediments via strong flare-like ebullition, producing fluxes that are orders of magnitude greater than fluxes observed in background areas underlain by largely frozen sediments. We suggest that progression of subsea permafrost thawing and decrease in ice extent could result in a significant increase in CH 4 emissions from the ESAS.

Publisher

The Royal Society

Subject

General Physics and Astronomy,General Engineering,General Mathematics

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