Transport of Chemical Contaminants in Karst Terranes: Outline and Summary

Notice - This site contains archived material(s)

Archive disclaimer
Archive disclaimer
Archived files are provided for reference purposes only. These files are no longer maintained by the Agency and may be outdated. For current EPA information, go to www.epa.gov. It is EPA's policy to support reasonable accommodation to persons with disabilities, pursuant to the Rehabilitation Act of 1973, 29 U.S.C. 791. If you need assistance with accessing archived files, contact EPA's Reasonable Accommodations or submit a request using the Contact Us form.


Abstract

Chemical spills that reach an aquifer in karst terranes do not behave like those in granular or highly fractured aquifers. pills reaching diffuse-flow aquifers display relatively slow transport, are radially dispersive, and can be tracked through the use of monitoring wells. pills in most karst terranes, however, are stored and transported in both the vadose and phreatic zones and do not exhibit radial dispersion. ctual contaminant transport in the phreatic zone of a karst aquifer may be extremely rapid to and highly concentrated at eventual discharge points, but the pollutant(s) cannot be tracked by any methods currently known. Contaminant attenuation is greatly limited in karst terranes. he unusual storage and transport characteristics responsible for the rapid transport and poor attenuation of contaminants in karst aquifers are a consequence of the unique properties of their flow system. inkhole development, the absence of surface water drainage, solutional enlargement of vertical fractures in the unsaturated zone, and the development of subsurface conduits (caves) are some of the properties of karst terranes that have substantial effects on the storage and transport of chemical contaminants.

Citation

Field, M. Transport of Chemical Contaminants in Karst Terranes: Outline and Summary. U.S. Environmental Protection Agency, Washington, D.C., EPA/600/D-90/001 (NTIS PB90200270).

Additional Information

Presented at the International Geological Congress, Washington, DC, 7/9-19/89