对童氏"7.5B"计算及乙型水驱法的改进

研究了童宪章院士"7.5B"的准确性和适应性,指出了"7.5B"方法只适用于多个油田的统计计算,而不完全适应于单一油藏.从理论上推导了"7.5B"的数学表达式,给出了一条准确计算该值的有效途径.对童氏水油比与采出程度关系乙型水驱法及采出程度与含水关系图版作了改进

Measurement of separate electron and positron spectra from 10 to 20 GeV with the geomagnetic field on DAMPE*

The cosmic-ray (CR) electrons and positrons in space are of considerable significance for studying the origin and propagation of CRs. The satellite-borne detector Dark Matter Particle Explorer (DAMPE) has been used to measure the separate electron and positron spectra, as well as the positron fraction. In this study, the Earth's magnetic field is used to distinguish CR electrons and positrons, as the DAMPE detector does not carry an onboard magnet. The energy for the measurements ranges from 10 to 20 GeV, which is currently limited at high energy by the zenith-pointing orientation of DAMPE. The results are consistent with previous measurements based on the magnetic spectrometer by AMS-02 and PAMELA, whereas the results of Fermi-LAT appear to be systematically shifted to larger values