牙鲆(Paralichthys olivaceus)TLR21 基因在迟缓爱德华氏菌(Edwardsiella tarda)感染后的表达特征

应用荧光定量PCR技术, 检测了TLR21 基因在牙鲆(Paralichthys olivaceus)感染迟缓爱德华 氏菌(Edwardsiella tarda)后, 在0 h、1 h、3 h、6 h、12 h、1 d、3 d、6 d 后, 在心脏、肝脏、脾脏、 头肾、鳃、小肠、肌肉和血的时空表达特征, 并探讨了它们与牙鲆先天免疫反应的关系。结果表明, 大 多组织在感染病原6 h 后TLR21 基因表达明显上调, 尤其是头肾和小肠。头肾6 h 的表达量达到了 对照组的59.3 倍, 小肠6 h 的表达量为对照组的38.6 倍。迟缓爱德华氏菌感染引起牙鲆体内各组织 中TLR21 的上调表达和变化, 为研究牙鲆对迟缓爱德华氏菌的防御机制提供了理论依据。     

Maintenance and development of the Ural high and its contribution to severe cold wave activities in winter 2020/21

2020年底至2021年初,连续两次强寒潮入侵中国东部地区,导致大范围强降温.本文研究这两次寒潮的特征和形成机理.主要结果如下:从2020年12月中旬到2021年1月中旬,乌拉尔山地区维持一宽阔的高压脊.脊前北风的维持和加强导致局地斜压性增加,导致下游横槽槽底等高线梯度加大,冷平流加强,西伯利亚高压加强和向南扩张.准定...     

The Tully-Fisher relations of the Eridanus group of galaxies

The Tully-Fisher (TF) or the luminosity-linewidth relations of the galaxies in the Eridanus group are constructed using the HI rotation curves and the luminosities in the optical and in the near-infrared bands. The slopes of the TF relations (absolute magnitudevs log2V _flat) are −8.6 ± 1.1, −10.0 ±1.5, −10.7 ±2.1, and −9.7 ±1.3 in the R, J, H, and K bands respectively for galaxies having flat HI rotation curves. These values of the slopes are consistent with those obtained from studies of other groups and clusters. The scatter in the TF relations is in the range 0.5-1.1 mag in different bands. This scatter is considerably larger compared to those observed in other groups and clusters. It is suggested that the larger scatter in the TF relations for the Eridanus group is related to the loose structure of the group. If the TF relations are constructed using the baryonic mass (stellar +HI + Helium mass) instead of the stellar luminosity, nearly identical slopes are obtained in the R and in the near-infrared bands. The baryonic TF (baryonic massvs log2V _flat) slope is in the range 3.5–4.1.     

Open cluster ASCC21 as a probable birthplace of the neutron star Geminga

We analyze the encounters of the neutron star (pulsar) Geminga with open star clusters in the OB association Ori OB1a through the integration of epicyclic orbits into the past by taking into account the errors in the data. The open cluster ASCC21 is shown to be the most probable birthplace of either a single progenitor star for the Geminga pulsar or a binary progenitor system that subsequently broke up. Monte Carlo simulations of Geminga-ASCC21 encounters with the pulsar radial velocity V _r = ?100±50 km s^?1 have shown that close encounters could occur between them within ≤10 pc at about t = ?0.52 Myr. In addition, the trajectory of the neutron star Geminga passes at a distance of ≈25 pc from the center of the compact OB association λ Ori at about t = ?0.39 Myr, which is close to the age of the pulsar estimated from its timing.     

黄骅坳陷古近系沙一段下部碳酸盐岩成岩作用

黄骅坳陷古近系沙河街组沙一段下部发育一套厚20～60m的湖相碳酸盐岩,并在生物灰岩、鲕粒灰(云)岩和泥晶白云岩中显示丰富的油气,具有良好的勘探前景。通过对研究区沙一段下部10余口钻井岩心、薄片的宏观及微观观察,结合地球化学特征,对成岩作用类型及特征进行较详细的研究,探讨了成岩作用与储集空间演化的关系。研究发现区内沙一段下部碳酸盐岩的成岩演化过程复杂,各种成岩作用发育,储层质量的好坏受成岩作用影响明显。压实压溶作用、多期方解石和白云石的胶结作用导致粒间孔、生物体腔孔和格架孔大幅度减少;混合水白云石化作用、同生期-准同生期和埋藏期溶解作用是优质储层形成的关键,形成了大量的晶间孔、晶间溶孔、粒内溶孔、铸模孔、生物体腔孔、粒间溶孔和溶蚀缝,成为现今该层段的主要储集空间。     

Elemental abundance analyses with DAO spectrograms: XXX. The middle B through early A stars ξ2 Ceti (B9 III), 21 Aquilae (B8 II‐III), ι Aquilae (B5 III), and ι Delphini (A2V)

This series of high quality elemental abundance analyses of mostly main‐sequence band normal and peculiar B, A, and F stars defines their properties and provides data for the comparison with the analyses of somewhat similar stars and with theoretical predictions. Most use high dispersion and high S/N (≥ 200) spectrograms obtained with CCD detectors at the long camera of the Coudé spectrograph of the 1.22‐m Dominion Astrophysical Observatory telescope. Here we reanalyze 21 Aql with better quality spectra and increase the number of stars consistently analyzed in the spectral range B5 to A2 by analyzing three new stars for this series. In the early A stars the normal and non‐mCP stars have abundances with overlapping ranges. But more stars are needed especially in the B5 to B9 range. ξ² Cet on average has a solar composition with a few abundances outside the solar range while both 21 Aql and ι Aql have abundances marginally less than solar. The abundances of ι Del are greater than solar with a few elements such as Ca being less than solar. It is an Am star (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

新世纪构造地质学的纵深发展:深海、深部、深空、深时四领域成就及关键技术

近10年来,构造地质学面临前所未有的机会和巨大的发展前景,建立超越板块构造理论的时代已经来临,地幔柱理论与板块构造理论的融合必将为太阳系乃至宇宙形成的构造过程提供全新认识。文中从宏观角度,综述了当前深部、深海、深空和深时4个发展方向取得的成就,展望了这4个方面的未来发展趋势。同时,综合概述了推动近10年来构造地质学发展的4个关键技术:针对表面构造形迹的高精度激光高度计(深空星球表面成像)、高分辨率多波束(深海海底地形成像);针对深部构造形态的层析成像(tomography);针对动力学演化(深时)的各种模拟软件(ANSYS、COMSOL、FLAC等);针对物质材料流变学的高温高压实验和成分原位测试技术。     

走向21世纪的矿床学

文章简要回顾了百年来矿床学取得的重要进展，包括：（1）矿床成因分类的建立；（2）层控矿床研究与矿床多成因理论的兴起；（3）板块构造与区域成矿规律；（4）矿床模型；(5)型矿床研究；（6）海洋现代热液成矿作用的发现；（7）成矿演化的不可逆性与节律性等。针对21世纪中人类社会可持续发展的需要，矿床学研究出现了两个新趋势；（1）全球化；（2）矿业开发与环境保护一体化。面临着三个主要研究领域；（1）成矿理论的推陈出新；（2）研究开发新型矿产资源，建立广义的矿产资源地质学；（3）建立绿色矿业体制所需的矿床学基础研究。     

中国近半个世纪最高气温变化特征

本文根据中国164个站1951－1995年极端气温资料分析了中国各地区平均最高气温45年来的多年变化特征,指出中国北方趋势变化并不明显,80年代后期有明显上升,西南地区80年代后期急剧下降,长江流域以南6O年代降温后变化不大,青藏高原变化较小。冬季的多年变化也各不相同,有区域性差异。EOF分析表明中国各地大多数年份有相似变化趋势,也有一些年份长江流域以南与其它各地变化相反。