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The AAPG/Datapages Combined Publications Database
West Texas Geological Society
Abstract
Shale Core Analyses Required for
Gas
Reserve Estimates
Abstract
Gas
-in-Place (GIP) analysis is generally performed for
gas
resource assessment (evaluation of exploration prospects), reservoir production modeling (development optimization and production forecasting), or geologic hazard evaluation (
gas
emissions during tunneling/mining). Four primary reservoir parameters are needed to calculate the GIP: reservoir or well drainage area; reservoir thickness; bulk density; and in-situ
gas
content. These variables are usually determined using
data
obtained
from geophysical logs, well site testing, and laboratory analysis of drill cuttings or core.
Generally speaking, GIP assessment of conventional reservoir is a relatively straightforward volumetric calculation since the
gas
molecules are stored by compression within available free
gas
porosity and there is no significant
gas
molecule-reservoir rock interaction. On the other hand, unconventional reservoirs have three storage mechanisms; compression of
gas
within rock pores; absorption of
gas
by mobile hydrocarbons or brine; and adsorption of
gas
within micropores. These complex
gas
storage mechanisms are exacerbated further, due to the fact actual
gas
content is a function of geological factors which affect the retention of adsorbed phase
gas
within the reservoir. Thus, accurate in-situ
gas
content often cannot be calculated solely from knowledge of physical rock properties but instead must be directly measured from freshly cut rock samples. In addition to the complexities surrounding unconventional
gas
storage mechanisms and
gas
content determination, there are unique and difficult challenges when trying to ascertain deliverability and the design of stimulation and production strategies.
Critical
data
requirements, methodology, and analytical techniques used to assess unconventional reservoirs will be discussed. Additionally, recent advances in unconventional reservoir assessment technology and remaining exploration, production, and development challenges will be presented.
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