Intracontinental basins and strong earthquakes

Introduction A M=8 earthquake occurred in the intracontinental Linfen basin on September 17, 1303. This is the Hongtong M=8 earthquake in Shanxi Province. It is the first recorded M = 8 earthquake since the Chinese historical seismic records had started. The earthquake killed 200 000 people (LI, 1960; XIE, CAI, 1983). The year 2003 is the 700th anniversary of the earthquake occurrence. In memory of the people died in the earthquake, for further improving earthquake prevention and disas…     

Surface rupture zone of the 1303 Hongtong M=8 earthquake, Shanxi Province

Introduction The 1303 Shanxi Hongtong M=8 earthquake is the earliest M=8 event determined in histori-cal records in China and the largest recorded in Shanxi fault-depression system in history. Some researchers have discussed the tectonic environment of this earthquake (DENG, et al, 1973; DENG, 1984; DENG, XU, 1994, 1995; Seismo-geological Brigade, State Seismological Bureau, Depart-ment of Geology and Geography, Peking University, 1979; LIU, XIAO, 1982; ZHANG, JIA, 1986; SU, …     

Study on the earthquake fault of the Lulong ML=6.2 earthquake by precise relocation of aftershock

Introduction The Lulong county is about 75 km northeast to Tangshan in Hebei Province. An earthquake of ML=6.2 took place on October 19, 1982 about 4 km northeast to the county town. The epicenter of the mainshock is located at 39°57′N, 119°04′E by the Beijing seismic network. The 1976 Tang- shan 7.8 earthquake and the successive Luanxian 7.1, Ninghe 6.9 and the Lulong earthquake spread in NE-SW direction in space. SONG and WANG et al of Institute of Geophysics, China Seismolog…     

Observation and analysis of geomagnetic abnormity associated with the Ms=5.7 Jiujiang-Ruichang earthquake

A three-component geomagnetic survey was carried out during the period from 2002 to 2004 in China including Jiujiang-Ruichang region. Comparing the ＂2005.0 surface spline model of China geomagnetic field＂ created on the basis of the survey data with the ＂1970.0 surface spline model of China geomagnetic field＂, we can see an obvious abnormity in the geomagnetic horizontal component within a range of about 100 km around the epicenter of the Ms=5.7 Jiujiang-Ruichang earthquake occurred on November 26, 2005. After the earthquake, we carded out a repeated geomagnetic survey at 21 stations in the Jiujiang-Ruichang region and created a corresponding ＂2005.0 partially revised surface spline model of China geomagnetic field＂. By comparing the above three models, analyzing the geomagnetic horizontal component at the profile in the Jiujiang-Ruichang region and quantitatively studying the geomagnetic data of every stations around the Ms=5.7 earthquake, we have obtained the geomagnetic abnormity associated with this earthquake. Then the geomagnetic abnormity and its relation with seismic activity are discussed in this paper.     

The true rotational period of the Ap star HD 193722 = V 1584 Cyg

Photometric observations of the Ap star HD 193722 give unambiguous proofs for a rotational period of P=8.5297 days in contradiction to the earlier found value of P=1.13316 days. Spectroscopic measurements yield a line width equivalent to the value v sin i=44.5 km/s. Both findings show convincingly that HD 193722 is an evolved Ap star with a position in the giant region of the HR diagram. This place falls into a domain occupied by the hypothetic Maia sequence.     

A further study of the method of identifying absorption line systems in QSO spectra

The method of identifying absorption line systems in QSO spectra (Cui et al. 1983; Chen et al. 1983) is further developed here. Certain limitations of the method and their improvements are discussed. Certain other problems requiring further study are pointed out. The improved method is applied to PKS 0528-250, and gives two new absorption line systems Z_a = 0.065 and 0.0345 in addition to the four systems Z_a = 2.8110, 2.8130, 2.5275, 2.1410, consistent with the systems A₁A₂, B, C of Norton et al. (1980). However, the systems D₁, D₂, E, F and G of Chen and Norton (1984) are not recovered. The reason for this discrepancy is discussed.     

华北地区强震重复性模式的讨论

根据位错量与地震应变能的关系及岩石不均匀脆性材料在受力后小破裂增加的特点，本文对华北这一相对完整块体的强震、强震丛、中强地震的活动参数与发震时间间隔进行了研究，初步建立了一种强震重复性的非线性简化模式，对强震丛之前中强地震的时间分布入物理力学过程有了一个大概的认识。在此基础上，讨论了中长期地震预测中的两个具体问题：①如何估计地震活动高潮时段开始时间；②高潮时段强震规模与结构的估计。     

NINO晶体的电子自旋共振

报道了 Ｎ Ｉ Ｎ Ｏ 晶体在 Ｔ＝ １．５ Ｋ 温度和 １０１ Ｇ Ｈｚ 频率下的电子自旋共振（ Ｅ Ｓ Ｒ）实验。建立了ｄ８ 离子基态３ Ａ２ （ Ｆ）自旋哈密顿参量 Ｄ、 Ｅ 和ｇ 因子与斜方对称晶场势参量间的关系,并对 Ｎ Ｉ Ｎ Ｏ 晶体进行了计算。所得结果与实验一致,表明所给关系式是合理的。     

A search for decay of with tin-loaded liquid scintillator

A search for the neutrinoless double-beta decay of ¹²⁴Sn was carried out using the tin-loaded liquid scintillator for an active source-detector technique. Tin (32.6%) in weight was successfully loaded into the liquid scintillator, and light output was as high as 57% of the unloaded liquid scintillator. A tin-loaded liquid scintillator with 1.1 ℓ volume was installed at the 700 m underground laboratory in YangYang, and data were taken for 5285 h. No evidence for the 0νββ decay was found and a lower limit on the ¹²⁴Sn half-life was obtained to be 2.0×10¹⁹ year with 90% C.L. The new limit represents a significant improvement with respect to those previously available for ¹²⁴Sn.     

Search for TeV gamma-rays from Geminga pulsar

We present the results of observation of the Geminga pulsar carried out in the TeV energy band during the 6 year period spanning 2000–2006 using the Pachmarhi Array of Cherenkov Telescopes (PACT). A long stretch of data, new computer codes and the “Tempo” package have been used in the present analysis. We have searched for evidence of pulsed emission of γ-rays from the Geminga pulsar using the post-glitch pulsar elements obtained by Jackson and Halpern from X-ray/γ-ray satellite data. We do not see any significant evidence for pulsed emission from the Geminga pulsar at a threshold energy of 825 GeV. In this paper we present our results on the light curve in the TeV energy band, set an upper limit on the time averaged flux of γ-rays, and compare our results with other ground based observations.