Monitoring and physical-chemical modeling of conditions of natural surface and underground waters forming in the Kola North

2012 ◽  
Vol 47 (5) ◽  
pp. 657-668 ◽  
Author(s):  
Svetlana I. Mazukhina ◽  
Vladimir A. Masloboev ◽  
Konstantin V. Chudnenko ◽  
Valeriy A. Bychinsky ◽  
Anton V. Svetlov ◽  
...  
2021 ◽  
Vol 13 (1) ◽  
pp. 105-124
Author(s):  
Alexandr Anatolevich Shibkov ◽  
Sergey Sergeevich Kochegarov

2014 ◽  
Vol 402 (1) ◽  
pp. 1.2-1 ◽  
Author(s):  
Gleb S. Pokrovski ◽  
Nikolay N. Akinfiev ◽  
Anastassia Y. Borisova ◽  
Alexandre V. Zotov ◽  
Kalin Kouzmanov

2017 ◽  
Vol 52 (9) ◽  
pp. 890-896
Author(s):  
Victoria V. Maksimova ◽  
Svetlana I. Mazukhina ◽  
Tatiana A. Cherepanova ◽  
Tamara T. Gorbacheva

Metals ◽  
2017 ◽  
Vol 7 (3) ◽  
pp. 83 ◽  
Author(s):  
Venkatesh Vijayaraghavan ◽  
Akhil Garg ◽  
Liang Gao ◽  
Rangarajan Vijayaraghavan

2019 ◽  
Vol 64 (3) ◽  
pp. 282-299
Author(s):  
L. S. Rybnikova ◽  
P. A. Rybnikov

In the Urals region in recent decades, dozens of copper mines, which are the most dangerous in terms of environmental impact, have been closed and flooded. In many of them, acid mine waters continue to form, the concentrations of most components in which exceed the permissible values by several orders of magnitude. The formation of the chemical composition of acidic groundwater has a pronounced unsteady character: a sharp increase in the content of all components in the water after flooding and a gradual decline for many years. On Levikha copper mine (Sverdlovsk region) after filling the depression con in 2007, a site of concentrated discharge of groundwater was formed (technogenic reservoir-a failure in the zone of collapse and displacement). The concentrations of many components 10 years after the completion of flooding are higher than during the development. The analysis of regularities of non-stationary character of hydrogeochemical processes is made on the basis of the data of detailed monitoring and extended definitions of groundwater quality indicators. The main source of acidic water with increased mineralization is the collapse zone, within which the process of drainage for several decades formed technogenic sulfuric acid weathering crust enriched with secondary minerals. According to the data of numerical geofiltration modeling, in the hydrodynamic balance the lateral flow coming from the surrounding areas is 60%, its value is manifested in the dilution of the solution, which is formed in the collapse zone. The time of movement of this flow in the area of collapse is 6–8 years, extremely high values of almost all indicators in the man-made reservoir are observed during this period. According to the inverse physical-chemical modeling (program code Visual MINTEQ ver. 3.0 / 3.1 was used) the composition of rocks, as a result of dissolution-deposition of which underground waters in the area of the flooded mine can be formed, is determined. The duration of the process of formation of acidic groundwater is estimated at tens of years.


2004 ◽  
Vol 418 (3) ◽  
pp. 1021-1034 ◽  
Author(s):  
S. D. Doty ◽  
F. L. Schöier ◽  
E. F. van Dishoeck

2015 ◽  
Vol 10 (S314) ◽  
pp. 139-142
Author(s):  
Nienke van der Marel ◽  
Ewine F. van Dishoeck ◽  
Simon Bruderer ◽  
Paola Pinilla ◽  
Tim van Kempen ◽  
...  

AbstractProtoplanetary disks with cavities in their dust distribution, also named transitional disks, are expected to be in the middle of active evolution and possibly planet formation. In recent years, millimeter-dust rings observed by ALMA have been suggested to have their origin in dust traps, caused by pressure bumps. One of the ways to generate these is by the presence of planets, which lower the gas density along their orbit and create pressure bumps at the edge. We present spatially resolved ALMA Cycle 0 and Cycle 1 observations of CO and CO isotopologues of several famous transitional disks. Gas is found to be present inside the dust cavities, but at a reduced level compared with the gas surface density profile of the outer disk. The dust and gas emission are quantified using the physical-chemical modeling code DALI. In the majority of these disks we find clear evidence for a drop in gas density of at least a factor of 10 inside the cavity, whereas the dust density drops by at least a factor 1000. The CO isotopologue observations reveal that the gas cavities are significantly smaller than the dust cavities. These gas structures suggest clearing by one or more planetary-mass companions.


Sign in / Sign up

Export Citation Format

Share Document