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Autor:
Lattanzi P.[1], Rimodia V.[1], Chiarantini L.[1], Colica A.[2], Benvenuti M.[2], Costagliola P.[2], Ruggieri G.[1]
Publikováno v:
Procedia earth and planetary science 17 (2017): 468–471.
info:cnr-pdr/source/autori:Lattanzi P.[1], Rimodia V.[1], Chiarantini L.[1], Colica A.[2], Benvenuti M.[2], Costagliola P.[2], Ruggieri G.[1]/titolo:Mercury dispersion through streams draining the Mt. Amiata district, southern Tuscany, Italy/doi:/rivista:Procedia earth and planetary science/anno:2017/pagina_da:468/pagina_a:471/intervallo_pagine:468–471/volume:17
info:cnr-pdr/source/autori:Lattanzi P.[1], Rimodia V.[1], Chiarantini L.[1], Colica A.[2], Benvenuti M.[2], Costagliola P.[2], Ruggieri G.[1]/titolo:Mercury dispersion through streams draining the Mt. Amiata district, southern Tuscany, Italy/doi:/rivista:Procedia earth and planetary science/anno:2017/pagina_da:468/pagina_a:471/intervallo_pagine:468–471/volume:17
The Mt. Amiata area hosts the 3rd largest Hg district in the world, overlapping with a present-day geothermal system that is exploited for energy production. Mining activity ceased in 1980; remediation of mining areas was only partial, and is still u
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=cnr_________::63eef257a591f1db297ee6c9ff7eeaa8
https://www.journals.elsevier.com/procedia-earth-and-planetary-science/
https://www.journals.elsevier.com/procedia-earth-and-planetary-science/