21世纪格陵兰冰川融化速率对海平面变化的影响

本文利用大洋环流模式POP研究RCP4.5情景下21世纪格陵兰冰川不同的融化速率对全球及区域海平面变化的影响。结果显示:当格陵兰冰川的融化速率以每年1%增加时,全球大部分海域的动力和比容海平面变化基本不变,主要是由于格陵兰冰川在低速融化时并不会导致大西洋经向翻转流减弱。当格陵兰冰川的融化速率以每年3%和每年7%增加时,动力海平面在北大西洋副极地、大西洋热带、南大西洋副热带和北冰洋海域呈现出显著的上升趋势,这是因为格陵兰冰川快速融化导致大量的淡水输入附近海域,造成该上层海洋层化加强和深对流减弱,导致大西洋经向翻转流显著减弱;与此同时,热比容海平面在北冰洋、格陵兰岛南部海域和大西洋副热带海域显著下降,而在热带大西洋和湾流海域明显上升;此时盐比容海平面的变化与热比容海平面是反相的,这是由于大量的低温低盐水的输入,造成北大西洋副极地海域变冷变淡、大西洋经向翻转流和热盐环流显著减弱,引起了太平洋向北冰洋的热通量和淡水通量减少,导致了北冰洋海水变冷变淡,同时热带大西洋滞留了更多的高温高盐水,随着湾流被带到北大西洋,北大西洋副极地海域低温低盐的海水,被风生环流输运到副热带海域。     

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。     

胶州湾大桥建设前后湾内泥沙冲淤数值模拟

本研究通过对胶州湾大桥建成前后湾内泥沙冲淤情况进行模拟。探讨了典型时刻胶州湾大桥附近海域的海流流速和流向情况。对比胶州湾大桥建成前湾内的流场模拟结果可知,胶州湾大桥的建设对胶州湾内整体的海流流态影响较小。胶州湾大桥的建设对胶州湾水动力的改变主要在桥墩建设附近海域。通过大桥建设前后冲淤数值模拟结果可知,工程前后工程附近冲淤趋势基本一致,只是在大桥桥墩附近出现冲淤变化较大的情况,表现为在桥墩的南北两侧出现较大桥建设前淤积加强区,在桥墩的东西两侧出现冲刷加强区,在通航孔桥墩跨度较大的海域,冲刷强度增大比较明显。