Deciphering the cosmogenic code to learn Earth’s surface history
dc.contributor.author | Stroeven, AP | en_AU |
dc.contributor.author | Fink, D | en_AU |
dc.contributor.author | Caffee, M | en_AU |
dc.date.accessioned | 2021-12-21T03:29:11Z | en_AU |
dc.date.available | 2021-12-21T03:29:11Z | en_AU |
dc.date.issued | 2016-11-28 | en_AU |
dc.date.statistics | 2021-11-14 | en_AU |
dc.description | Citation from webpage - Stroeven, A. P.,Fink, D., and Caffee, M. (2016), Deciphering the cosmogenic code to learn Earth’s surface history, Eos, 97, https://doi.org/10.1029/2016EO062975. Published on 28 November 2016. | en_AU |
dc.description.abstract | Galactic cosmic rays continually bombard Earth’s upper atmosphere, causing a cascade of secondary particle fluxes. The more energetic components of this particle cascade penetrate the atmosphere and interact with the nuclear building blocks within the minerals that compose the rocks on Earth’s surface, producing a wide variety of secondary nuclides.Text © 2016. The authors. CC BY-NC-ND 3.0 | en_AU |
dc.identifier.booktitle | EOS 97 | en_AU |
dc.identifier.citation | Stroeven, A. P., Fink, D., & Caffee, M. (2016). Deciphering the cosmogenic code to learn Earth’s surface history. Paper presented at Third Nordic Workshop on Cosmogenic Nuclide Techniques; Stockholm, Sweden, 8–10 June 2016. In Eos, 97. doi:10.1029/2016EO062975 | en_AU |
dc.identifier.conferenceenddate | 10 July 2016 | en_AU |
dc.identifier.conferencename | Third Nordic Workshop on Cosmogenic Nuclide Techniques | en_AU |
dc.identifier.conferenceplace | Stockholm, Sweden | en_AU |
dc.identifier.conferencestartdate | 8 July 2016 | en_AU |
dc.identifier.issn | 2324-9250 | en_AU |
dc.identifier.uri | https://doi.org/10.1029/2016EO062975 | en_AU |
dc.identifier.uri | https://apo.ansto.gov.au/dspace/handle/10238/12623 | en_AU |
dc.language.iso | en | en_AU |
dc.publisher | American Geophysical Union | en_AU |
dc.subject | Cosmic radiation | en_AU |
dc.subject | Particle influx | en_AU |
dc.subject | Earth atmosphere | en_AU |
dc.subject | Isotopes | en_AU |
dc.subject | Chlorine 36 | en_AU |
dc.subject | Beryllium 10 | en_AU |
dc.subject | Aluminium 26 | en_AU |
dc.subject | Mass spectroscopy | en_AU |
dc.title | Deciphering the cosmogenic code to learn Earth’s surface history | en_AU |
dc.type | Conference Paper | en_AU |
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