A Measurement of Omega from the North American Test Flight of Boomerang

We use the angular power spectrum of the cosmic microwave background, measured during the North American test flight of the Boomerang experiment, to constrain the geometry of the universe. Within the class of cold dark matter models, we find that the overall fractional energy density of the universe Omega is constrained to be 0.85相似文献   

The Properties of Supernova 1997cy Associated with GRB 970514

The extraordinary SN 1997cy associated with GRB 970514 has been observed photometrically and spectroscopically for nearly 2 yr. At the time of discovery, SN 1997cy was the brightest supernova (SN) ever observed (MV相似文献   

MARINE HAZARDS IN COASTAL AREAS AND HUMAN ACTION AGAINST THEM-A CASE STUDY OF THE CHANGJIANG RIVER ESTUARIES AND QIANTANG RIVER

INTRODUCTIONMarinehedsresultinginenomouslossestousuallyPOpulousandeconondcallyde-veloPedlowandcoastalandestUdrineregi0nsareforngseriousattenti0n.msarticlediscussesP0ssiblepreventivemeasaresagainstInariflehazaIdsbasedonacasestUdyoftheestUedesoftheChanaiiangffiverandQiantanffiver-ThesetwoareasoftheChanaiiangDeltaareboicalofc0astalregionsfreqUenilysufferingfromdrinehazanls,andarethemostsociallyandeconondcallydeveloPedregionsinChina.Theirinhabitantshaveahist0-ryofmorethanathouSandyeare0…     

临汾台摆式倾斜仪平行观测的差异性特征及其观测布局建议

根据临汾地震台石英摆、垂直摆、宽带垂直摆3套摆式倾斜仪器的观测资料,对山西中南部几次中等地震进行分析,发现在地震前各仪器同测向曲线有一定的异常反映,但异常并非呈相关一致性变化,有的还表现出明显的差异性特征;在同一台址条件下,异常的差异性与仪器的工作周期、动态响应范围、记录频段等有关;河津地震前后宽带垂直摆倾斜仪记录到的连续阶跃扰动(错位掉格)可能是慢地震现象,由此说明了宽频段仪器的优越性及发展性;建议在形变台网观测中,同一台站应建立宽频或多种同类型的形变观测仪器,组成尽量具有低、中、高频段的全面观测系统,这可能对于扑捉近震的短临前兆异常有实效意义.     

实时气象业务系统新型高速局域网建设的探讨

介绍了武汉区域气象中心实时气象业务系统的发展及其局限性,结合武汉区域中心的实际情况,以及新的网络系统的开放性、安全性等多方面的要求,提出了网络的改造方案,在气象部门将是有益的探讨。     

EFFECT OF RATION, TEMPERATURE AND BODY WEIGHT ON GROWTH OF BLACK PORGY,SPARUS MACROCEPHALUS (B.)

ChntnbutionNo.3127fromtheInstituteofOceanology,ChinereAcademyofSciences.Project39370542supportedbyNSFCandstudyalsosupportedbyNationalKeyLaboratoryintheInstituteofHydrobiology.ChineseAcademyofSciences.lNTRODUCTIONltisknownthatgroWthrateoffishcanvary'inresponsetotemperatureandfoodavailability-andperhapslessobviously,tolight,oxygenandothervariables.ThispropertyofvariablegroWthinfishcanbereferredtoasplasticity(Weatheriey,l990).TheeffeCtSofenvironmenta1thCtorsongroWthcanbepredictalfor…     

窄线赛弗特Ⅰ星系Markarian478的远紫外成协吸收线(英文)

Markarian 478是典型的窄线赛弗特I星系之一。本文展示了在 2 0 0 1年 1月利用远紫外光谱探测卫星 (FUSE)观测到的Markarian 478的远紫外光谱。我们的光谱覆盖了 91 5Å ;— 1 1 85Å的波长范围 ,分辨率约为 2 0km/s。我们在连续谱上探测到OⅥλλ1 0 3 2 ,1 0 3 8、NⅢλ989和CⅢλ977强发射线。在高电离双线OⅥ以及Lyβ的蓝端线翼上出现了成协吸收线 ,而在NⅢ和CⅢ发射线上没有出现内禀吸收线。这些吸收线被分解成 5个动力学成分 ,它们相对于系统红移zem=0 .0 774的静止坐标系速度覆盖了从 -2 3 0 0～ 3 70km/s的范围     

RECENT RESULTS FORM EARTHBASED OBSERVATIONS OF MARS

Even in an age of increasing spacecraft exploration, telescopic observations of Mars continue to provide new data and new insights into the nature of the Martian surface, atmosphere, and climate. Three major technological advances in the last decade, combinde, have allowed telescopic observations to increase our knowledge of the planet: (1) Advances in infrared, near-infrared, and radio wavelength array detector and telescope technology, allowing high spatial and/ or high spectral resolution imaging in new and diagnostic wavelength regions; (2) The advent of routine space-based telescopic observations of Mars using the Hubble Space Telescope , providing the ability to study the planet at high spatial resolution over a much longer part of its orbit than from groundbased telescopes, and offsetting some of the inherent loss in resolution associated with the recent series of aphelic oppositions of the planet; and (3) The widespread use and availability of CCD cameras and powerful telescopes in the 10 - inch     

Numerical simulation of the general circulation of the atmosphere of Titan

The atmospheric circulation of Titan is investigated with a general circulation model. The representation of the large-scale dynamics is based on a grid point model developed and used at Laboratoire de Météorologie Dynamique for climate studies. The code also includes an accurate representation of radiative heating and cooling by molecular gases and haze as well as a parametrization of the vertical turbulent mixing of momentum and potential temperature. Long-term simulations of the atmospheric circulation are presented. Starting from a state of rest, the model spontaneously produces a strong superrotation with prograde equatorial winds (i.e., in the same sense as the assumed rotation of the solid body) increasing from the surface to reach 100 m sec-1 near the 1-mbar pressure level. Those equatorial winds are in very good agreement with some indirect observations, especially those of the 1989 occultation of Star 28-Sgr by Titan. On the other hand, the model simulates latitudinal temperature contrasts in the stratosphere that are significantly weaker than those observed by Voyager 1 which, we suggest, may be partly due to the nonrepresentation of the spatial and temporal variations of the abundances of molecular species and haze. We present diagnostics of the simulated atmospheric circulation underlying the importance of the seasonal cycle and a tentative explanation for the creation and maintenance of the atmospheric superrotation based on a careful angular momentum budget.