Articles | Volume 13, issue 4
https://doi.org/10.5194/gmd-13-2073-2020
https://doi.org/10.5194/gmd-13-2073-2020
Model description paper
 | 
24 Apr 2020
Model description paper |  | 24 Apr 2020

HR3DHG version 1: modeling the spatiotemporal dynamics of mercury in the Augusta Bay (southern Italy)

Giovanni Denaro, Daniela Salvagio Manta, Alessandro Borri, Maria Bonsignore, Davide Valenti, Enza Quinci, Andrea Cucco, Bernardo Spagnolo, Mario Sprovieri, and Andrea De Gaetano

Viewed

Total article views: 1,931 (including HTML, PDF, and XML)
HTML PDF XML Total Supplement BibTeX EndNote
1,213 652 66 1,931 403 53 52
  • HTML: 1,213
  • PDF: 652
  • XML: 66
  • Total: 1,931
  • Supplement: 403
  • BibTeX: 53
  • EndNote: 52
Views and downloads (calculated since 17 Sep 2019)
Cumulative views and downloads (calculated since 17 Sep 2019)

Viewed (geographical distribution)

Total article views: 1,931 (including HTML, PDF, and XML) Thereof 1,696 with geography defined and 235 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 13 Dec 2024
Download
Short summary
The HR3DHG (high-resolution 3D mercury model) investigates the spatiotemporal behavior, in seawater and marine sediments, of three mercury species (elemental, inorganic, and organic mercury) in a highly polluted marine environment (Augusta Bay, southern Italy). The model shows fair agreement with the experimental data collected during six different oceanographic cruises and can possibly be used for a detailed exploration of the effects of climate change on mercury distribution.