Cliff-Hanger - Blasting Near the Edge

The Australasian Institute of Mining and Metallurgy
N Elith
Organization:
The Australasian Institute of Mining and Metallurgy
Pages:
13
File Size:
789 KB
Publication Date:
Jan 1, 2003

Abstract

Coal is a valuable energy source in New Zealand and has been mined from the West Coast for over 100 years. Stockton Mine is New Zealand's largest opencast coal producer supplying around 1.5 Mt of hard coking and thermal coal to international markets annually. The Stockton Plateau forms an extensive, gently inclined dip slope on erosion resistant Lower Eocene Brunner Coal Measures unconformably overlying basement rocks. The dip slope rises 600 - 1000 masl, locally dissected by fault scarps and present-day fluvial systems, some of which are deeply incised. Within the Mt Augustus Mining Block overburden comprises of a 30 - 40 m thick sequence of fluviatile, coarse to granular coal measure sandstones. High quality coking coal is preserved as a gently dipping, 10 - 12 m thick seam. High and sometimes very steep cliffs of jointed overburden shape the skyline escarpment, above steep forested slopes and gullies. As mining has progressed at Mt Augustus individual coal blocks are progressively becoming more technically challenging. This paper outlines the scientific approach taken by Solid Energy International and mining contractors to carefully unlock many thousands of tons of coal whilst protecting nearby flora and fauna from the impacts of dislodged rock and other blasting side-effects. The strategy involved: an expert-driven onsite risk assessment,formulation of a management plan to manage impacts,conducting an in situ vibration research program, andanalysis of results and operational designs to eliminate potential environmental problems.
Citation

APA: N Elith  (2003)  Cliff-Hanger - Blasting Near the Edge

MLA: N Elith Cliff-Hanger - Blasting Near the Edge. The Australasian Institute of Mining and Metallurgy, 2003.

Export
Purchase this Article for $25.00

Create a Guest account to purchase this file
- or -
Log in to your existing Guest account