The potential of using in situ cosmogenic 14CO in ice cores at Dome C to examine the assumption of a constant galactic cosmic ray flux

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dc.contributor.authorPetrenko, VVen_AU
dc.contributor.authorBenZvi, Sen_AU
dc.contributor.authorSmith, AMen_AU
dc.contributor.authorDyonisus, MNen_AU
dc.contributor.authorHmiel, Ben_AU
dc.contributor.authorNeft, PDen_AU
dc.contributor.authorBuizert, Cen_AU
dc.contributor.authorSeveringhaus, JPen_AU
dc.date.accessioned2024-02-28T04:06:16Zen_AU
dc.date.available2024-02-28T04:06:16Zen_AU
dc.date.issued2021-12-17en_AU
dc.date.statistics2023-01-27en_AU
dc.description.abstractCosmogenic nuclides produced in the Earth’s atmosphere and at the surface are powerful proxies for important climate processes and drivers. Records of atmospherically-produced 14C and 10Be have been used to reconstruct past solar activity and solar irradiance. 10Be, 14C, 26Al and other nuclides produced in surface rock are widely used in studies of past ice dynamics and extent. All these studies generally assume that the galactic cosmic ray (GCR) flux at Earth is constant in time. However, the available geochemical evidence for GCR flux constancy is complicated by processes that are not fully constrained. As a result, the assumption of a constant GCR flux may be uncertain by 30% or more. Cosmic rays also produce 14C in situ in glacial ice and firn; this 14C then reacts rapidly to form mainly 14CO and 14CO2. Almost all of the 14C produced in the firn layer is lost to the atmosphere via gas diffusion, and in situ 14C only starts to accumulate in the deepest firn (≈95 m at Dome C) where gas exchange with the atmosphere effectively stops. At this depth, all of the in situ 14C production is via interactions with deep-penetrating muons. Such muons are generated by high-energy primary GCRs that are unaffected by geomagnetic and solar modulation. Further, at sites with low snow accumulation such as Dome C, in situ 14CO strongly dominates over trapped atmospheric 14CO in the ice. As a result, 14CO in ice at Dome C would provide a record of the past GCR flux that is virtually free of confounding factors and should allow to constrain any past flux variations to within ≈ 10%. This presentation will provide a brief overview of results from recent studies of in situ cosmogenic 14CO in Greenland and Antarctica, as well as predictions for Dome C under a range of different GCR flux scenarios.en_AU
dc.identifier.articlenumberC45D-1028en_AU
dc.identifier.booktitleAGU Fall Meeting Abstractsen_AU
dc.identifier.citationPetrenko, V. V., BenZvi, S., Smith, A. M., Dyonisius, M., Hmiel, B., Neff, P. D., Buizert, C., & Severinghaus, J. P. (2021). The potential of using in situ cosmogenic 14CO in ice cores at Dome C to examine the assumption of a constant galactic cosmic ray flux. Paper presented to the AGU Fall Meeting 2021, New Orleans, Louisiana and Online, 13-17 December 2021. In AGU Fall Meeting Abstracts (Vol. 2021, C45D-1028). Retrieved from: https://agu.confex.com/agu/fm21/meetingapp.cgi/Paper/891495en_AU
dc.identifier.conferenceenddate2021-12-17en_AU
dc.identifier.conferencenameAGU Fall Meeting 2021en_AU
dc.identifier.conferenceplaceNew Orleans, Louisiana and Onlineen_AU
dc.identifier.conferencestartdate2021-12-13en_AU
dc.identifier.urihttps://agu.confex.com/agu/fm21/meetingapp.cgi/Paper/891495en_AU
dc.identifier.urihttps://apo.ansto.gov.au/handle/10238/15469en_AU
dc.identifier.volume2021en_AU
dc.language.isoenen_AU
dc.publisherAmerican Geophysical Union (AGU)en_AU
dc.subjectCarbon 14en_AU
dc.subjectIceen_AU
dc.subjectDrill coresen_AU
dc.subjectCosmic ray fluxen_AU
dc.subjectIsotopesen_AU
dc.subjectBeryllium 10en_AU
dc.subjectRocksen_AU
dc.subjectSolar activityen_AU
dc.subjectEarth planeten_AU
dc.subjectClimatesen_AU
dc.titleThe potential of using in situ cosmogenic 14CO in ice cores at Dome C to examine the assumption of a constant galactic cosmic ray fluxen_AU
dc.typeConference Presentationen_AU
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