Intensity variations of the postnoon auroral bright spots observed at Zhongshan Station, Antarctica on August 8, 1999

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X-Ray Afterglows of GRBs 050318 and 060124 and their External Shock Origin

The observations with Swift X-ray telescope (XRT) challenge the conventional gamma-ray burst model in many aspects. The XRT light curves are generally composed of four consecutive segments, i.e., a steep decay segment, a shallow decay segment, a normal decay segment, a jet-like steep decay segment, and sometimes erratic flares as well. The phys-ical origin of the X-ray emission is highly debatable. We focus here on the physical origin of the X-ray emissions of GRBs 050318 and 060124. We present the XRT light curves and spectra of the two bursts. The light curve decay slopes of the two bursts are normal, and their relations to the spectral indices are consistent with the prediction of the standard forward shock model. The multi-wavelength light curves at 0.5keV, 1.0keV, 2.0keV and 4.0keV can be reproduced by this model with an isotropic kinetic energy Ek = 2.2×1052 erg, e = 0.04, B = 0.01 for GRB 050318 and Ek = 4.2×1053 erg, e = 0.05, B = 0.01 for GRB 060124. These facts suggest that the normal decay phases of the X-rays for the two bursts are of the forward shock origin.     

Transient events in the COBE database simultaneous with gamma ray bursts

We are investigating the COBE DMR data at instances of known -ray bursts (GRBs) when any of the six DMR horn directions was coincident with the direction of a burst. The BATSE instrument on board GRO has detected 207 bursts during the eight-month period of overlap corresponding to the current release of COBE data. The odds of a GRB occurring within the DMR field of view are near one coincidence per year. Here we report on one such serendipitous observation in 1991, GRB 911226, for which a detailed analysis is currently in progress.     

Search for gamma-ray bursts with energies above 1 TEV

Some models of gamma-ray bursts suggest that their spectrum may extend into the energy range above 10 GeV, i.e. above energies accessible with CGRO. Data taken with the HEGRA extensive air shower array are used to search for very high energetic gamma-ray burst counterparts above 1 TeV. First results from the search for BATSE correlated and BATSE independent bursts are presented.     

分频振幅检测“亮点”型浅层气的方法研究及应用

渤中A油田浅层发育大量"亮点"型浅层气,此类气层的识别受调谐厚度的水层影响严重。针对该问题,笔者充分考虑气层、水层产生强振幅的主控因素的差异性,利用正演模拟,分析并总结了不同厚度的气层与调谐厚度的水层在不同分频体上的振幅能量响应规律,提出了利用分频振幅检测浅层"亮点"型气层的方法。将该方法应用于渤中A油田的浅层气预测中,取得了较好的效果,有效地指导了评价井位的部署,对渤海油田类似的气层预测研究具有一定参考价值。     

基于卫星热红外辐射信息的新疆强震震例分析

利用NOAA-14极轨气象卫星红外波段的探测数据,对遥感数据进行多种处理,采用影像目视解释和提取地表辐射亮温值的方法,对新疆的三次强震进行分析,结果发现在地震前都出现了热红外异常,这为地震监测提供了一个重要信息。     

努力实践“硬道理”，勇闯市场天地宽

从解放思想、科学决策、人才培育、谨慎运作等方面,紧紧围绕“发展才是硬道理”的理论,论述了地质勘探企业创市场的新思路、新举措。     

A search for prompt radio emission from GRBs

The Cambridge Low Frequency Synthesis Telescope (CLFST) is being used to search for prompt radio emission from GRBs at 151 MHz. For this search a special observing mode has recently been developed; the antennas of the CLFST are split into seven groups which are spaced about 30° apart. When triggered by the real-time signals from the BACODINE system the antennas are slewed to the GRB position, with data being sampled at 1.5 or 3-s intervals. The antennas slew at about 10° per minute, so that an appreciable fraction of the sky can be accessed on timescales of a few minutes - any prompt radio emission from a GRB might be delayed by this timescale due to propagation effects.     

Deriving the GRB distance scale

We describe a method to address the burster origin problem by determining their distance scale. We show that this can be easily carried out at soft X-ray wavelengths by measuring the effective column densities of a representative sample of burst spectra. We demonstrate the effectiveness of the technique by simulating the performance of a small CATSAT-type mission (Forrestet al., 1995).