Shock chemistry in the molecular clouds associated with SNR IC 443

Several interstellar molecules have been detected toward the highly perturbed B and G clouds associated with the supernova remnant IC 443 via their 3 mm transitions, including N2H+, SiO, SO, CN, HNC, and H13CO+. The (J, K) = (1, 1) and (2, 2) inversion lines of metastable ammonia have also been observed, as well as the J = 3-2 transition of HCO+ at 1.2 mm. Analysis of the (1, 1) and (2, 2) inversion lines of NH3 indicates minimum gas kinetic temperatures of TK = 70 K toward cloud B, and TK = 33 K in cloud G. Modeling of the J = 1-0 and J = 3-2 transitions of HCO+ implies densities greater than 10(5) cm-3 toward both positions. These data clearly show that hot and dense material is present in IC 443, and they suggest the presence of shocks in both regions. A careful analysis of the HCO+ lines indicates that the HCO+ abundance is at most enhanced by factors of a few over that found in cold, quiescent gas. This conclusion contradicts past claims of HCO+ abundance enhancements of several orders of magnitude in the perturbed regions. The N2H+ abundance was also found to be similar to that in cold gas, suggesting that there is no increase in ionization in the clouds. The abundances of SO and CS, as well as CN and NH3, do not appear to differ significantly from those found in cold dark clouds, although chemistry models predict sulfur-containing species to undergo high-temperature enhancements. SiO, however, is found to have an abundance in the perturbed gas 100 times larger than the upper limits observed in the dark cloud TMC 1, a result in agreement with high temperature chemistry models. In addition, the HNC/HCN ratio in both IC 443 B and G was found to be approximately 0.1--far from the ratio of 1 predicted by low-temperature ion-molecule chemistry, but similar to the values observed in clouds where elevated temperatures are present.     

地震前兆仪器嵌入TCP/IP协议的初步试验

根据“十五”总体设计方案的要求，对TCP／IP协议在地震前兆仪器上的实现进行了试验，在有关设备上进行了程序开发，取得了预期的效果。     

发展基于IPv6的地震传感器网络是科技自主创新的实践

IPv6的网络架构为传感器网络的发展创造了良好的环境，基于IPv6的地震传感器网络已列为CNGI（China Next Generation Intemet）具有行业特色的，在中国下一代互联网示范项目中的应用项引。以科学的发展观研究和发展基于IPv6的地震传感器网络，是贯彻十六届五中全会精神，科技自主创新的实践；是推进地震监测和预报进一步发展的重要契机；我们需要认真努力，为我国下一代互联网建设和防震减灾事业做出贡献。[编者按]     

苏鲁超高压地体部分熔融时间的厘定：荣成花岗质片麻岩中浅色条带的锆石U-Pb定年、微量元素和Lu-Hf同位素证据

威海-荣成地区混合岩化花岗质片麻岩为研究超高压地体折返过程中的部分熔融提供了理想的窗口。本文通过对荣成地区鲍村花岗质片麻岩中浅色条带野外观察、岩相学以及锆石的CL图像、U-Pb定年、微量元素和Lu-Hf同位素的系统研究表明,鲍村花岗质片麻岩中的浅色条带为部分熔融的产物,其主要矿物组成为石英+斜长石+钾长石+黑云母。锆石CL图像显示清楚的核-边结构:继承岩浆核和新生岩浆边。继承核的206Pb/238U协和年龄为620±8～784±7Ma(Mean=701±33Ma);具有典型的岩浆锆石的微量元素特征,如重稀土(HREE)和Y富集,强烈的正Ce异常和负Eu异常,以及极低的(Gd/Lu)N和Hf/Y比值;εHf(t=700Ma)值为-13.0～-8.0(Mean=-10.9±0.8),相应的tDM2为2120～2429Ma(Mean=2303±51Ma)。新生边的206Pb/238U协和年龄为211±6～244±5Ma(226±10Ma);虽然微量元素的整体含量低于继承核,但也具有岩浆锆石的微量元素特征,如稀土元素配分模式显示HREE明显上翘的特征,正Ce异常和负Eu异常,以及极低的(Gd/Lu)N比值;εHf(t=225Ma)值为-17.3～-14.2(Mean=-15.2±0.6),相应的tDM2为2152～2347Ma(Mean=2214±33Ma)。上述特征表明,部分熔融的原岩是由古元古代(2.2～2.3Ga)的地壳物质在新元古代(701±33Ma)重熔而成,部分熔融可能发生在超高压地体折返早期的热折返阶段(榴辉岩相-高压麻粒岩相条件下),时代应为226±10Ma。威海-荣成混合岩化片麻岩内广泛发育的富含钾长石和石英的酸性岩脉(约220～210Ma),可能为折返晚期的角闪岩相冷凝阶段,部分熔融形成的熔体经历了结晶分异作用的产物。     

多排螺旋CT五个剂量测量点位的统计学差异

目的:探讨螺旋CT五个辐射剂量测量点位(CTDI₁₀₀)值之间的差异和相关性统计学关系,以及该机器的辐射稳定性。方法:通过辐射剂量计和辐射剂量模体对螺旋CT五个测量点位进行12次重复测定,对各个点位的测量结果计算其相对偏差,然后用单因素方差分析(One-Way ANOVA)方法分析各点位测量结果之间的显著性。结果:5个点位重复测量的相对标准差分别为0.33%(中心点)、0.73%(3点位)、0.32%(6点位)、1.00%(9点位)和0.32%(12点位);3点位和9点位的平均值接近,单因素方差分析无显著性差异;12点位和6点位的平均值与3点位平均值的相对偏差在0.5%以下。结论:测试螺旋CT辐射稳定性良好,测试机型3点位和9点位在CTDI₁₀₀上测量等效。在非验收测试和状态测试场合CTDI_P可以进行简化。     

Study on electric variations of media in epicentral area by geomagnetic transfer functions

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