三个牙鲆育种群体亲本效应及遗传参数估计

针对牙鲆(Paralichthys olivaceus)养殖品种生长速度变慢、抗病力降低这一问题。近年来构建了牙鲆抗病群体(RS)、日本群体(JS)和黄海群体(YS)3个育种群体,开展牙鲆选择育种,建立了63个家系,收集了所有家系5 328尾鱼苗的体长和体重数据。借助线形混合模型(Linear mixedmodel)、"加性-显性"模型、约束极大似然法(REML)及最佳线性无偏预测(BLUP)分别估计亲本效应值、体重和体长遗传力和遗传相关、父母本效应和杂交效应。预测结果显示,其中父本130,141,146,170,218,229,303和308随机效应达到了极显著效应水平(P<0.01),父本112,122,141,190,212达到显著水平(P<0.05),所有母本体重随机效应达到了极显著水平(P<0.01);体长和体重两性状的加性、显性、表型和基因型相关分量都达到极显著水平(P<0.01),体长和体重的加性方差比率均大于显性方差比率,可见两性状的遗传效应主要取决于基因的加性效应。体长的总遗传效应率为31.20%,体重的总遗传效应率为33.58%,体长和体重的随机方差比率分别达到68.80%和66.41%,说明养殖环境等因素对牙鲆体长和体重的影响较大,同时说明在牙鲆选择育种中消除环境影响极为重要。体长和体重的狭义遗传率分别为0.199和0.256(P<0.01),广义遗传率分别为0.312和0.336(P<0.01),牙鲆在以上两性状上属于中等遗传力,通过选择育种可取得较大的遗传进展。对3个牙鲆育种群体杂交随机效应估计结果显示,抗病群体和黄海群体在体长和体重两性状上加性随机效应显著(P<0.05);抗病群体分别与日本群体、黄海群体杂交,其后代表现出显性随机效应达到0.10的水平(P<0.10),黄海群体自交、日本群体和黄海群体杂交随机效应不显著(P>0.05),因此在杂交组配中选择抗病群体与其他两个群体交配可取得较好的效果。     

The Influence of Two Kinds of El Niño Events on the Strong Tropical Cyclone Generation and Strength in the Pacific Ocean

This paper focuses on the effects of two types of El Niño events on tropical cyclone activity. We classified El Niño events from 1961 to 2015 according to their sea surface temperature (SST) anomalies into an eastern type and a central type. Then we selected strong tropical cyclones to statistically analyze the tropical cyclone characteristics during different events and their effects, as well as to study the possible mechanisms related to thermodynamic and dynamic factors. The tropical cyclone generation areas were found to be very similar during the two kinds of events. The average number of tropical cyclone in the eastern event is more than that in central event, and the hurricane in northeastern Pacific (HNP) has more energy than the typhoon in northwestern Pacific (TNP) in all cases. The seasonal distribution of the TNP high-incidence centers during central El Niño events is opposite to that of the HNP. The TNP accumulated cyclone energy (ACE) intensity is similar in the fall and summer, and the HNP ACE intensity in the summer is greater than that in the fall. The SSTs are consistent with the TNP and HNP movement trends. The Walker circulation intensity was strongly affected by the eastern events, but it quickly returned to its normal state, while the intensity was slightly reduced in the central events, and it slowly returned to its normal state. The vertical velocity distributions in the Pacific are different at different stages of both events, and the distributions of vertical velocity anomalies for typhoons and hurricanes are consistent.     

5月南极涛动对青藏高原西部夏季气温影响的诊断分析

青藏高原是全球气候变暖最敏感的地区之一,是北半球夏季最大的热源,其气候响应受到广泛关注。然而,有关南极涛动与青藏高原夏季气温的关系和机理知之甚少。为了研究南极涛动与青藏高原夏季气温的关系,基于1979—2020年英国东安哥拉大学气候研究中心（CRU）的逐月气温、美国国家海洋和大气管理局（NOAA）的逐月海表面温度和大气环流再分析数据以及南极涛动指数等数据,采用相关、回归、合成分析等方法进行研究。结果表明,北半球夏季青藏高原西部气温与5月南极涛动存在显著负相关,即当5月南极涛动异常偏弱时,夏季青藏高原西部气温异常偏高。其影响过程为,南极涛动为正位相时,在南印度洋中高纬地区出现“负-正-负”的经向“三极子”海温模态,该模态可持续到夏季,在印度洋形成异常的纬向-垂直环流,相应在热带西印度洋和东印度洋-海洋性大陆之间的降水异常导致热带正“偶极子”降水模态,通过该降水模态在青藏高原西部引起异常反气旋环流和下沉运动,有利于高原西部气温偏高。研究结果显示,海洋的热惯性在“延长”南极涛动影响过程中起着重要的桥梁作用,可为青藏高原夏季气温预测提供科学依据。     

Milestones in the Observations of Cosmic Magnetic Fields

Magnetic fields are observed everywhere in the universe. In this review, we concentrate on the observational aspects of the magnetic fields of Galactic and extragalactic objects. Readers can follow the milestones in the observations of cosmic magnetic fields obtained from the most important tracers of magnetic fields, namely, the star-light polarization, the Zeeman effect, the rotation measures (RMs, hereafter) of extragalactic radio sources, the pulsar RMs, radio polarization observations, as well as the newly implemented sub-mm and mm polarization capabilities. The magnetic field of the Galaxy was first discovered in 1949 by optical polarization observations. The local magnetic fields within one or two kpc have been well delineated by starlight polarization data. The polarization observations of diffuse Galactic radio background emission in 1962 confirmed unequivocally the existence of a Galactic magnetic field. The bulk of the present information about the magnetic fields in the Galaxy comes from anal     

Periodicities in Global Mean TEC from GNSS Observations

As an important measurement parameter, global total electron content (TEC) is appropriate for the study of the Sun–Earth connection. In this paper, the wavelet technique is employed to investigate the periodicities in global mean TEC during 1995–2008. Analysis results show several remarkable components (including 27-day, semiannual and annual cycles) existing in global mean TEC with obvious time-variable characteristics, besides 11-year cycle. After analyzing sunspot numbers and solar extreme ultra-violet (EUV) radiation variations during this time period, except for semiannual variations, close correlation between global mean TEC and solar variations is found, especially, a strong resemblance of the 27-day fluctuation exists in global mean TEC, sunspot and solar EUV radiation variations.     

土工格栅加筋膨胀土渠坡数值模拟研究

对土工格栅加筋膨胀土渠坡这种较新的膨胀土处理措施进行研究,在考虑土工格栅与填土之间的相互作用、膨胀土吸水膨胀、软化特性等膨胀土渠坡关键影响因素的基础上,提出了土工格栅加筋膨胀土渠坡数值计算的新思路,并采用有限差分软件Flac3D进行了验证。数值算例结果表明,土工格栅对膨胀土渠坡有明显的水平位移约束作用,是有效的处理措施,可以在实际工程中采用。     

EXPERIMENTAL STUDY ON FALL VELOCITY OF NON-UNIFORM SEDIMENT IN FLOWING WATER

I INTRODUCTIONThe settlement of particles in fluid has been studied in many fields such as hydraulics, metallurgy andchemistry since the middle of 19 century because of its great importance. Although the settlement ofsingle particle and group settling velocity of uniform particles in still water are relatively well-studied, yetthe settlement of non-uniform particles in flowing water lacks understanding. For instance, Cunningham(1910), Richardson (1954) and Batchelor (1972), have obtained…     

日本古代中心日食记录在地球自转研究中的可能作用

本文介绍了利用古代中心日食记录研究地球自转速率变化的原理以及日本古代的中心日食记载，认为日本中心日食记录的年代虽然不太古老，但能为地球自转变化研究提供有价值的信息。