2023年中国气候异常特征及主要天气气候事件

2023年,我国气候主要表现为暖干的特征,全国平均气温10.71℃,较1991—2020年气候平均偏高0.82℃,为1951年以来最暖;全国平均降水量615.0 mm,较常年偏少3.9%,为2012年以来第二少。四季气温均较常年同期偏高,其中夏、秋季分别为历史同期次高和最高;除秋季降水偏多外,其余三季降水均偏少。汛期(5—9月),全国平均降水量较常年同期偏少4.3%,为2012年以来第二少,我国中东部降水总体呈“中间多南北少”的分布。2023年,我国区域性气象干旱多发,西南地区遭遇冬春连旱;春季北方沙尘天气过程偏多;夏季前期,华北和黄淮遭受1961年以来最强高温过程;7月底至8月初,受台风杜苏芮影响,京津冀地区发生历史罕见极端强降水过程,华北地区出现“旱涝急转”;华西秋雨开始早、结束晚、雨量多;1月中旬发生年内最强寒潮过程;秋末冬初冷空气频繁入侵,12月华北和黄淮等地降雪日数偏多、积雪偏深。     

饲料中维生素B6对皱纹盘鲍幼鲍蛋白质代谢的影响

以皱纹盘鲍(Haliotis discus hannaiIno)幼鲍为研究对象,探讨维生素B6对其蛋白质代谢的影响。设计了3种维生素B6不同含量(0,40,4 000 mg/kg)的半精制饲料,在循环水养殖系统中养殖幼鲍240 d。结果表明,皱纹盘鲍内脏团和肌肉中磷酸吡哆醛(PLP)的含量随饲料中维生素B6的添加而显著升高(P<0.05)。饲料中不同维生素B6水平对肌肉组织中蛋白含量没有显著影响(P>0.05),而显著升高内脏团中蛋白质的含量(P<0.05)。内脏团和肌肉中的谷丙转氨酶(ALT)和谷草转氨酶(AST)活力随着饲料中维生素B6添加量的升高而显著增强,分别在维生素B6的添加量为4 000 mg/kg时取得最大值(P<0.05)。内脏团中所检测的各种氨基酸的含量与饲料中维生素B6添加量没有显著影响(P>0.05)。然而,肌肉中的天冬氨酸(Asp)、苏氨酸(Thr)、丝氨酸(Ser)、牛磺酸(Tau)的含量随着饲料中维生素B6添加量的升高而显著增加,并且分别在维生素B6添加量为4 000 mg/kg时取得最大值(P<0.05)。肌肉中甘氨酸(Gly)、丙氨酸(Ala)、缬氨酸(Val)、蛋氨酸(Met)的含量在两个维生素B6添加组(40 mg/kg和4 000 mg/kg)之间没有显著差异(P>0.05),但均显著高于维生素B6缺乏组(0 mg/kg)的值(P<0.05)。     

凡纳滨对虾抗WSSV选育家系的抗病与生长特性

从引进的无特定病原（SPF）凡纳滨对虾（Litopenaeusvannamei）亲虾生产的子代中挑选出生长快、体格健壮等性状良好的个体作为亲本建立16个第一代选育家系,并经223d饲养和感染实验从中挑选出抗病力强、生长快的家系建立21个第二代家系．抗WSSV实验的结果表明：第一代选育各家系经感染wssv（投喂）后的成活率在0～61．5％之间,平均成活率为30．0％±16．5％;第二代选育家系成活率在14．5％～70．0％之间,平均成活率为37．3％±15．2％,比第一代提高24．3％．21个第二代选育家系经28d的生长实验显示：21个选育家系体长特定生长率在0．00l5～0．0142之间,体重特定生长率在0．0053～0．0279之间;两代选育家系抗病与生长的结果表明：抗病较强的家系生长快,抗病差的家系生长慢,但抗病最强或生长最快的家系,其对应的生长或抗病性能则不理想．     

嵌入式系统中基于寄存器的编译器优化技术

介绍了嵌入式系统处理器的资源分配原理及其存在问题,为了提高嵌入式系统性能,提出了基于寄存器的编译器优化技术,在寄存器和Cache之间增加一级起特殊缓冲作用的寄存器,用于寄存器的快速恢复和保留。根据优先权公式,把执行频率高的变量尽量存放在缓冲寄存器中,减少了变量存入内存的次数,有效节省了内存资源,提高了嵌入式系统处理器工作效率。采用参考比较的方法,在Md32仿真器上,选用典型算法进行测试,实验证明此优化算法有效。     

长时间序列Radarsat图像的神经网络模拟及土地覆盖变化的快速检测

土地覆盖的短期时空变化模式研究,对土地覆盖的快速、动态监测具有重要意义,也是遥感研究的新热点。本文利用2000—2001年的时间序列Radarsat图像,采用功率谱分析方法,对土地覆盖的短期时—空变化的周期特征进行了分析,由此建立了基于时间序列影像分析的神经网络预测模型,从植被主要生长季节的时间序列雷达卫星影像获取训练样本,对研究区域的典型土地覆盖的短期动态变化过程进行了学习。学习后的模型能够利用多个时间序列的Radarsat影像对下一时刻的影像进行模拟,并进一步检测变化。在模拟结果基础上,定义相对变化距离函数和检测门限,对模拟影像及实际影像中的变化区域进行了检测。检测精度范围在66.67%(农村居民点)—91.67%(水体)之间,平均检测精度为81.66%。由于时间序列信号的引入,神经网络模型能够较好地获取土地覆盖的短期动态变化信息。     

基于索引图的大比例尺图幅自动接边方法研究

针对图幅接边中存在的问题和难点,提出了一套基于索引图多幅大比例尺地图自动接边的方法,采用了组件式编程方法,实现了简单化和自动化图幅接边的功能.     

Structural evolution in elliptical galaxies: the age–shape relation

We test the hypothesis that the apparent axial ratio of an elliptical galaxy is correlated with the age of its stellar population. We find that old ellipticals (with estimated ages t >7.5 Gyr) are rounder on average than younger ellipticals. The statistical significance of this shape difference is greatest at small radii; a Kolmogorov–Smirnov test comparing the axial ratios of the two populations at R = R _e/16 yields a statistical significance greater than 99.96 per cent. The relation between age and apparent shape is linked to the core/power-law surface brightness profile dichotomy. Core ellipticals have older stellar populations, on average, than power-law ellipticals and are rounder in their inner regions. Our findings are consistent with a scenario in which power-law ellipticals are formed in gas-rich mergers, while core ellipticals form in dissipationless mergers, with cores formed and maintained by the influence of a binary black hole.     

Emission-line properties of Seyfert 2 nuclei

This is the third paper of a series devoted to the study of the global properties of Joguet's sample of 79 nearby galaxies observable from the southern hemisphere, of which 65 are Seyfert 2 galaxies. We use the population synthesis models of Paper II to derive 'pure' emission-line spectra for the Seyfert 2 galaxies in the sample, and thus explore the statistical properties of the nuclear nebular components and their relation to the stellar populations. We find that the emission-line clouds suffer substantially more extinction than the starlight, and we confirm the correlations between stellar and nebular velocity dispersions and between emission-line luminosity and velocity dispersions, although with substantial scatter. Nuclear luminosities correlate with stellar velocity dispersions, but Seyferts with conspicuous star-forming activity deviate systematically towards higher luminosities. Removing the contribution of young stars to the optical continuum produces a tighter and steeper relation,   L ∝σ⁴_★  , consistent with the Faber–Jackson law.
Emission-line ratios indicative of the gas excitation such as [O  iii ]/Hβ and [O  iii ]/[O  ii ] are statistically smaller for Seyferts with significant star formation, implying that ionization by massive stars is responsible for a substantial and sometimes even a dominant fraction of the Hβ and [O  ii ] fluxes. We use our models to constrain the maximum fraction of the ionizing power that can be generated by a hidden active galactic nucleus (AGN). We correlate this fraction with classical indicators of AGN photoionization (i.e. X-ray luminosity and nebular excitation), but find no significant correlations. Thus, while there is a strong contribution of starbursts to the excitation of the nuclear nebular emission in low-luminosity Seyferts, the contribution of the hidden AGN remains elusive even in hard X-rays.     

抽真空引起周围土体竖向变形的有限元分析

真空预压法加固深厚超软土地基时,一方面使地基土体产生侧向收缩变形,有利于地基的稳定;但另一方面向真空预压区的侧向变形对周围房屋、地下管线、道路等建筑物也产生不利影响,甚至会出现管道断裂、围墙倒塌、路堤被毁等严重工程事故。结合真空预压加固软基工程中出现的对周围环境影响的问题,进行了考虑土体拉裂影响的有限元分析,研究抽真空过程及加固区外不同距离、不同土体深度沉降的变化规律。研究结果表明,采用Biot固结理论、考虑土体拉裂的有限元计算结果与现场加固区外土体沉降及影响区范围的实测结果基本一致。     

Chemical abundances and ionizing clusters of H ii regions in the LINER galaxy NGC 4258

We present long-slit observations in the optical and near-infrared of eight H  ii regions in the spiral galaxy NGC 4258. Six of the observed regions are located in the south-east inner spiral arms, and the other two are isolated in the northern outer arms. A detailed analysis of the physical conditions of the gas has been performed. For two of the regions, an electron temperature has been derived from the [S  iii ] λ 6312 line. For the rest, an empirical calibration based on the red and near-infrared sulphur lines has been used. The oxygen abundances derived by both methods are found to be significantly lower (by a factor of 2) than previously derived by using empirical calibrations based on the optical oxygen lines.
In the brightest region, 74C, the observation of a prominent feature caused by Wolf–Rayet (WR) stars provides an excellent constraint over some properties of the ionizing clusters. In the light of the current evolutionary synthesis models, no consistent solution is found to explain at the same time both the WR feature characteristics and the emission-line spectrum of this region. In principle, the presence of WR stars could lead to large temperature fluctuations and also to a hardening of the ionizing radiation. None of these effects is found in region 74C, for which the electron temperatures found from the [S  iii ] λ 6312 line and the Paschen discontinuity at 8200 Å are equal within the errors, and the effective temperature of the ionizing radiation is estimated at around 35 300 K.
Both more observations of confirmed high-metallicity regions and a finer metallicity grid for the evolutionary synthesis models are needed in order to understand the ionizing populations of H  ii regions.