Insight-HXMT observations of the Crab pulsar

We report on X-ray emission properties of the Crab pulsar(PSR B0531+21) using observations by Insight-HXMT during its first year after launch. We obtained high signal-to-noise profiles in the X-ray energy band 11–250 keV. We have confirmed an increase in the flux ratio of the second peak over the main peak with increasing energy, consistent with other missions. The separation of the two peaks shows no significant trend with increasing energy. The phase-averaged spectrum, fitted by a logpar model, and the phase-resolved spectra of the Crab pulsar, fitted by a powerlaw in the different energy bands of HXMT, are consistent with RXTE and NuSTAR in that photon indices evolve as a function of phase as well as a function of energy, contributing to a broadband modeling.     

A low-latency pipeline for GRB light curve and spectrum using Fermi/GBM near real-time data

Rapid response and short time latency are very important for Time Domain Astronomy, such as the observations of Gamma-ray Bursts(GRBs) and electromagnetic(EM) counterparts of gravitational waves(GWs). Based on near real-time Fermi/GBM data, we developed a low-latency pipeline to automatically calculate the temporal and spectral properties of GRBs. With this pipeline, some important parameters can be obtained, such as T_(90) and fluence, within ～ 20 min after the GRB trigger.For ～ 90% of GRBs, T_(90) and fluence are consistent with the GBM catalog results within 2σ errors.This pipeline has been used by the Gamma-ray Bursts Polarimeter(POLAR) and the Insight Hard Xray Modulation Telescope(Insight-HXMT) to follow up the bursts of interest. For GRB 170817 A, the first EM counterpart of GW events detected by Fermi/GBM and INTEGRAL/SPI-ACS, the pipeline gave T_(90) and spectral information 21 min after the GBM trigger, providing important information for POLAR and Insight-HXMT observations.     

Broadband ground motion simulation using a hybrid approach of the May 21, 2021 M7.4 earthquake in Maduo,Qinghai, China

In this study, the broadband ground motions of the 2021 M7.4 Maduo earthquake were simulated to overcome the scarcity of ground motion recordings and the low resolution of macroseismic intensity map in sparsely populated high-altitude regions. The simulation was conducted with a hybrid methodology, combining a stochastic high-frequency simulation with a low-frequency ground motion simulation, from the regional 1-D velocity structure model and the Wang WM et al.(2022) source rupture model,respect...     

日长亚季节变化的振幅调制与厄尔尼诺现象

利用Ｈｉｌｂｅｒｔ变换解算了１９６２年至１９９６年日长亚季节振荡的包络变化．结果显示,日长亚季节变化的振幅调制不仅具有一线性增长趋势,而且包含一个超前厄尔尼诺变化历程的年际变化．分别研究日长亚季节准５０天包络变化以及准１２０天包络变化后发现,这种超前性来自日长亚季节准５０天的振幅变化,这一结论与大气的研究结果一致．日长亚季节准１２０天的振幅变化在１９７２年附近发生了位相１８０°反转,因此日长亚季节准１２０天的振幅变化自１９７６年以来与厄尔尼诺的历程正好同步,１９７２年以前则截然相反．众所周知,日长变化在亚季尺度上具有显著的易变性,然而上述的非线性调制现象不仅表明了日长亚季节变化的内在规律性,而且证实了地球自转运动在不同时间尺度上存在极明显的非线性相互作用．同时也表明,日长变化作为全球风系变化的一个有价值的信息指标,将逐渐成为研究气候系统全球状态的有效手段之一．     

可控式海底取样器的结构及工作原理--海底取样技术介绍之三

介绍了多种型号的冲击打入式和振动式海底取器的结构、工作原理和性能参数,并阐述了远距离空联样器、自动化联样器和水下微型取样器等３种回转式海底取样器的控制方式,结构形成和性能参数。     

赤道海面高亚季节变化的时空特征

本文对赤道海区Topex/Poseidon卫星(1992.10-1998.10)测高资料进行最小二乘法分区拟合,扣除周年和半周年信号之后,再用Vondrak滤波得到30天至150天的亚季节信号。小波振幅谱结果显示了海平面高度变化的亚季节时频时空特性与厄尔尼诺事件存在一定的相关性。     

河南省新一代天气预报业务系统

介绍了河南省气象台新一代天气预报业务流程系统的主要内容和功能,以及系统特点和作用。     

辽河三角洲湿地的景观变化分析

利用遥感、ＧＩＳ手段对辽河三角洲１９８６年和１９９４年两个时段的湿地景观进行研究，认为本区景观是由两种作用力相互作用而形成的，从而形成了本区独具特色的景观变化方式，即半自然湿地（以苇田为主）向代湿地（以稻田为主）转化。     

边界层风廓线雷达测温系统设计

风廓线雷达在气象领域的应用越来越广泛，在风廓线雷达基础上增加电声测温系统（RASS）实现大气温度实时探测是一种经济有效的办法。文中介绍了已实现的某RASS系统设计，讨论了RASS测温的原理，针对RASS测温的精度、高度、影响因素等进行了性能分析，论述了系统的实现方案，最后给出了该RASS的实际测温结果和测温谱图，验证了该设计满足系统要求，能实现实时测温。     

河南省区域暴雨的客观分型

从多层聚类分析入手,利用微机对１９８０～１９９５ 年河南省２１３ 场区域暴雨过程的５００ ｈＰａ 高度场进行客观分型,得出了４ 类天气形势及其与暴雨落区的对应关系。