基于加权整体最小二乘的矿区平面坐标转换方法

常用的平面坐标系统转换模型四参数转换法在实际工程应用中,由于公共点一般分布在较小的范围内,点之间的距离较近,因此传统的四参数转换模型中旋转参数和平移参数之间的相关性较大,容易导致法方程病态,进而影响转换参数的精度,文中从重合点坐标重心化的转换模型出发,还原出重心化之前的四参数。通过加权整体最小二乘的转换分析及迭代计算,验证运用加权整体最小二乘(WTLS)方法转换的参数质量比最小二乘(LS)、整体最小二乘(TLS)方法得到的参数质量有显著改善。     

对分量进行联合解算的极移预报方法研究

为了提高极移预报的精度,该文提出结合极移的两个分量进行统一求解的极移联合预报方法:将极移的两个分量组成一个观测方程,并采用LS+AR模型对联合分量的确定项与随机项进行拟合。实验结果表明,文中采用的联合预报方法可以提高极移的预报精度。     

AGNS and MICROQUASARS As High-Energy γ-Ray Sources

The extragalactic analogs of the microquasars, the quasars, are strong γ-ray emitters at GeV energies. It is expected that microquasars are also γ-ray sources, because of the analogy with quasars and because theoretical models predict the high-energy emission. There are two microquasars that appear as the possible counterparts for two unidentified high-energy γ-ray sources.     

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First results of the Central-East-South European Binary Star Study Group (CESEB)

Several eclipsing binary systems have been selected for combined spectral and photometric observations using the Bulgarian NAO 2 m telescope and several smaller telescopes located at various places in the CESE region. Preliminary results, based on a pilot study started in 2001, about radial velocity and light curve variations of the active W UMa system LS Del are presented here.     

响应变量随机缺失下部分线性单指标模型的非参数判别检验

研究了响应变量随机缺失情况下部分线性单指标模型的非参数部分检验问题,检验非参数部分预测变量同响应变量之间是否存在非线性关系.用参数和非参数函数的借补估计对缺失响应变量进行插值,并基于借补估计构造了广义似然比检验统计量,证明了其渐近分布性质.     

重复中位数估计Robust算法在长周期大地电磁中的应用

将基于重复中位数估计的Robust算法应用于长周期大地电磁阻抗张量估算中。与传统Robust估计(M估计)相比,重复中位数估计求解过程不需要重设参量,并且提高了算法对时间域原始资料中噪声干扰的容限,使算法的理论崩溃值从30%提高到50%,也能得到准确的估算结果。龙门山地区实测资料的处理结果表明,基于重复中位数估计的Robust算法应用于阻抗张量的求解具有较强的优越性。     

H.E.S.S. observations of LS 5039

Recent observations of the binary system LS 5039 with the High Energy Stereoscopic System (H.E.S.S.) revealed that its Very High Energy (VHE) γ-ray emission is modulated at the 3.9 days orbital period of the system. The bulk of the emission is largely confined to half of the orbit, peaking around the inferior conjunction epoch of the compact object. The flux modulation provides the first indication of γ-ray absorption by pair production on the intense stellar photon field. This implies that the production region size must be not significantly greater than the gamma-gamma photosphere size (∼1 AU), thus excluding the large scale collimated outflows or jets (extending out to ∼1000 AU). A hardening of the spectrum is also observed at the same epoch between 0.2 and a few TeV which is unexpected under a pure absorption scenario and could rather arise from variation with phase in the maximum electron energy and/or the dominant VHE γ-ray production mechanism. This first-time observation of modulated γ-ray emission allows precise tests of the acceleration and emission models in binary systems. Mathieu de Naurois for the H.E.S.S. Collaboration.     

基于空域最小二乘法求解GOCE卫星重力场的模拟研究

本文论述了最小二乘过程中有色噪声的处理方法,提出使用AR模型对GOCE梯度观测值中的有色噪声进行时域滤波,数值模拟结果验证了该方法的有效性。利用数值模拟验证了直接求逆方法和PCCG法求解大型法方程的有效性,后者的效率远远高于前者。联合加入噪声（有色噪声和白噪声）的卫星重力梯度张量径向分量观测值Vzz和SST观测值,分别使用空域最小二乘法和SA方法恢复了180阶全球重力场模型,前者求解重力场模型的大地水准面和重力异常在180阶次的精度分别为3.01cm和0.75mGal,优于SA方法求解模型的精度。