2014
DOI: 10.1007/s13146-014-0220-7
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Spatial and temporal variations in carbon dioxide (CO2) concentrations in selected soils of the Moravian Karst (Czech Republic)

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Cited by 15 publications
(10 citation statements)
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“…-5 m 2 s -1 ) were applied, in order to cover nonhomogeneous structure of cave overburden. The CO 2 concentrations directly measured in upper parts of the soil profiles in the Moravian Karst range from 1,000 to 10,000 ppmv (4.3 × 10 -2 to 0.43 mol m -3 ) (Faimon & Ličbinská, 2010;Faimon et al, 2012b;Blecha & Faimon, 2014). A narrower range is reported for cave CO 2 concentrations.…”
Section: Discussionmentioning
confidence: 99%
“…-5 m 2 s -1 ) were applied, in order to cover nonhomogeneous structure of cave overburden. The CO 2 concentrations directly measured in upper parts of the soil profiles in the Moravian Karst range from 1,000 to 10,000 ppmv (4.3 × 10 -2 to 0.43 mol m -3 ) (Faimon & Ličbinská, 2010;Faimon et al, 2012b;Blecha & Faimon, 2014). A narrower range is reported for cave CO 2 concentrations.…”
Section: Discussionmentioning
confidence: 99%
“…Other studies indicate similarly high CO 2 concentrations (3-10 vol%) (Peyraube et al 2012(Peyraube et al , 2013Milanolo and Gabrovšek 2015). This is contradictory to low concentrations of soil CO 2 with seasonal character (Faimon and Ličbinská 2010;SanchezCañete et al 2011;Plestenjak et al 2012;Blecha and Faimon 2014a), although supported by some measurements in vadose zone and caves (Otava 1995;Benavente et al 2010). Independence of P CO 2 ðHÞ on surface conditions (temperature variation, rainfall, amount of water in perched collectors etc.)…”
Section: Hypothetical P Co 2 In Epikarstmentioning
confidence: 96%
“…The study was conducted in the Punkva Caves (Moravian Karst, Czech Republic, see, e.g., Absolon 1970;Blecha and Faimon 2014a). Moravian Karst is the largest karst region in the Czech Republic with surface area of 92 km 2 .…”
Section: Site Of Studymentioning
confidence: 99%
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“…() suggest that precipitation has the greatest influence on karst systems only within the first few metres of the epikarst where CO 2 concentrations are more abundant and dissolution generates common surface morphologies, such as dolines, poljes, and cenotes (Veni et al ., ). Capturing these geochemical changes requires both high‐resolution and long‐term data collection, as several studies indicate that epikarst heterogeneity and residence time can greatly influence the point at which dissolution tends to cease and measuring the flux of CO 2 in this part of the system through proxy geochemical data has proven challenging (Hess and White, ; Baldini et al ., ; Blecha and Faimon, , ).…”
Section: Introductionmentioning
confidence: 99%