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Airborne Shortwave Infrared Spectral Remote Sensing as a Direct Prospecting Method for Oil and Gas Resources
作者姓名:杨柏林
作者单位:InstituteofGeochemistry,ChineseAcademyofSciences,Guiyang550002
摘    要:The spectral characters of hydrocarbons in some oil-bearing strata and soil layers ouer oil and gas reservoirs in the Junggar Basin and northern Tarim Basin in Xinjng are compared with those of chemically pure hydrocarbons.The hydrocarbons are characterized by the bi-absorption at 2310nm and 2350nm.Hydrocarbon and radioactive anomalies in oil and gas terrains are found much more widespread than carbonate alterations.Based on the spectra of heavy hydrocarbons related to oil between 2270nm and 2460nm and refined data treatme nt, remote sensing may hold encouraging promise as a directly prospecting technique for oil and gas resources.

关 键 词:地震勘察  新疆  地物  油气勘探  遥感  短波红外线光谱

Airborne shortwave infrared spectral remote sensing as a direct prospecting method for oil and gas resources
Yang Bailin.Airborne Shortwave Infrared Spectral Remote Sensing as a Direct Prospecting Method for Oil and Gas Resources[J].Chinese Journal of Geochemistry,1994,13(2):156-164.
Authors:Yang Bailin
Institution:(1) Chinese Academy of Sciences, Institute of Geochemistry, 550002 Guiyang
Abstract:The spectral characters of hydrocarbons in some oil-bearing strata and soil layers over oil and gas reservoirs in the Junggar Basin and northern Tarira Basin in Xinjiang are compared with those of chemically pure hydrocarbons. The hydrocarbons are characterized by the bi-absorption at 2310nm and 2350nm. Hydrocarbon and radioactive anomalies in oil and gas terrains are found much more widespread than carbonate alterations. Based on the spectra of heavy hydrocarbons related to oil between 2270nm and 2460nm and refined data treatme nt, remote sensing may hold encouraging promise as a directly prospecting technique for oil and gas resources.
Keywords:remote sensing of oil and gas  airborne remote sensing  shortwave infrared spectrum  spectra of ground objects  Xinjiang
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