Modelling of the anthropogenic tritium transient and its decay product helium-3 in the Mediterranean Sea using  a  high-resolution regional model

Ayache, M.; Dutay, J.-C.; Jean-Baptiste, P.; Beranger, K.; Arsouze, T.; Beuvier, J.; Palmieri, J.; Le-vu, B.; Roether, W.

doi:https://doi.org/10.5194/os-11-323-2015

Articles | Volume 11, issue 3

Ocean Sci., 11, 323–342, 2015

https://doi.org/10.5194/os-11-323-2015

© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.

Ocean Sci., 11, 323–342, 2015

https://doi.org/10.5194/os-11-323-2015

© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.

Articles | Volume 11, issue 3

Research article 12 May 2015

Research article | 12 May 2015

Modelling of the anthropogenic tritium transient and its decay product helium-3 in the Mediterranean Sea using a high-resolution regional model

M. Ayache et al.

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Final revised paper (published on 12 May 2015)
Preprint (discussion started on 05 Dec 2014)

Interactive discussion

Status: closed

AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment

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RC C1269: 'Re: “Modelling of the anthropogenic tritium transient and its decay product helium-3 in the Mediterranean Sea using a high-resolution regional model” by M. Ayache et al.', Anonymous Referee #1, 19 Jan 2015
- AC C1352: 'Answer to Referee #1', Mohamed AYACHE, 23 Feb 2015
RC C1280: 'Review of “Modelling of the anthropogenic tritium transient and its decay product helium-3 in the Mediterranean Sea using a high-resolution regional model” By M. Ayache et al.', Anonymous Referee #2, 21 Jan 2015
- AC C1353: 'Answer to Referee #2', Mohamed AYACHE, 23 Feb 2015

Short summary

The anthropogenic tritium invasion, and its decay product helium-3, was simulated for the first time in the Mediterranean Sea, using a high-resolution regional model (NEMO-MED12). The simulation covers the entire tritium (3H) transient generated by the atmospheric nuclear weapons tests performed in the 1950s and early 1960s and run until 2011. The model correctly simulates the main features of the thermohaline circulation in the Mediterranean Sea, with a realistic time compared to observations.