Real-time difference imaging analysis of MOA Galactic bulge observations during 2000     

I.A. Bond  F. Abe  R.J. Dodd  J.B. Hearnshaw  M. Honda  J. Jugaku  P.M. Kilmartin  A. Marles  K. Masuda  Y. Matsubara  Y. Muraki  T. Nakamura  G. Nankivell  S. Noda  C. Noguchi  K. Ohnishi  N.J. Rattenbury  M. Reid  To. Saito  H. Sato  M. Sekiguchi  J. Skuljan  D.J. Sullivan  T. Sumi  M. Takeuti  Y. Watase  S. Wilkinson  R. Yamada  T. Yanagisawa  P.C.M. Yock 《Monthly notices of the Royal Astronomical Society》2001,327(3):868-880

We describe observations carried out by the MOA group of the Galactic bulge during 2000 that were designed to detect efficiently gravitational microlensing of faint stars in which the magnification is high and/or of short duration. These events are particularly useful for studies of extrasolar planets and faint stars. Approximately 17 deg² were monitored at a sampling rate of up to six times per night. The images were analysed in real time using a difference imaging technique. 20 microlensing candidates were detected, of which eight were alerted to the microlensing community whilst in progress. Approximately half of the candidates had high magnifications (≳10), at least one had very high magnification (≳50), and one exhibited a clear parallax effect. The details of these events are reported here, together with details of the on-line difference imaging technique. Some nova-like events were also observed and these are described, together with one asteroid.  相似文献   

Introduction     

M. Takeuti 《Astrophysics and Space Science》1993,210(1-2):1-5

A historical sketch of the nonlinear theory of variable stars is outlined briefly. The main break-through came from the hydrodynamic study of stellar pulsation. From a theoretical point of view, coupling needs to be discussed more carefully. The impact of new opacities on the astrophysical problems is also discussed.  相似文献   

Japan-equator XBT sections in late November 1989 and in early December 1991     

Jiro Yoshida  Hideo Sudo  Masaji Matsuyama  Yoshihiro Kurita  Yuji Mine 《Journal of Oceanography》1993,49(1):121-129

A comparison between Japan-equator XBT sections along 150°E in late November 1989 and along 140°E in early December 1991 is made. The warmest surface water above 29°C diminished to the south of 2–4°N and the surface mixed layer noticeably decreased in thickness in the equatorial region in December 1991; besides, the North Equatorial Countercurrent was intensified. This is considered to be a manifestation of changes in the surface layer of the western equatorial Pacific in the mature phase of El Niño.  相似文献   

Hydrogeochemical investigation of geothermal springs in Erzurum,East Anatolia (Turkey)     

Mine Alacali 《Environmental Earth Sciences》2018,77(24):802

Geothermal water sources located within The Erzurum province were identified and hot water samples were taken from four different geothermal areas. The results of in situ and hydrogeochemical analyses of these hot water samples were interpreted and the properties of hot water, water–rock associations, estimated reservoir temperature and hot water usage areas were determined. The temperatures of the samples collected from the study area vary between 26.2 and 57.7 °C, while pH values change from 6.09 to 7.33, EC values obtained from in situ measurements are between 1829 and 9480 µS/cm and Eh values are (??190) to (26.3) mV. Total dissolved solids of the hot waters have a range from 838.7 to 3914.1 mg/l. The maximum estimated reservoir temperature is calculated as 250 °C by applying chemical geothermometers. However, considering the actual temperatures of Pasinler, Köprüköy, Horasan and Il?ca thermal waters and wells, the most reliable temperature range depending on the applied geothermometers’ results indicate minimum and maximum reservoir temperatures 85–158.9 °C, respectively, taking in account the errors. According to the isotope analysis, the waters circulating within the geothermal system are of meteoric origin and modern waters. In addition, two samples taken from clayey levels observed in the field were analyzed and the mineralogy of the clays was evaluated.  相似文献   

铜陵冬瓜山层状铜矿同位素地球化学及成矿机制研究   总被引：12，自引：0，他引：12       下载免费PDF全文

徐兆文陆现彩  高庚方长泉  王云健杨小男蒋少涌  陈帮国 《地质论评》2007,53(1):44-51

长江中下游地区是中国重要的铜、金、硫产地,区内分布着一系列喷流沉积及喷流沉积热液叠加改造型层状铜金矿床。本文以冬瓜山层状铜矿床为例,通过热液流体和矿石同位素地球化学研究,探讨层状铜矿床的成矿机制,重点分析了成矿物质的来源。冬瓜山铜矿床热液流体氢、氧、碳和锶同位素分析表明,成矿热液流体主要来自岩浆,混有少量大气降水;CO2可能主要来自被岩浆同化的原始地层中海相沉积碳酸盐;ISr具有地壳物质来源的特征。各种类型矿石的硫、铅同位素研究显示,硫具有海底喷流沉积和后期岩浆热液叠加作用的特征,铅则以上地壳铅为主,混有少量的地幔铅。上述同位素地球化学特征表明冬瓜山层状铜矿床是在原始沉积基础上,经燕山期岩浆热液叠加成矿作用所形成。  相似文献   

矿震及其前兆初探   总被引：11，自引：1，他引：11  

车用太  宁挺文 《中国地震》1993,9(4):334-340

本文通过对山东霜矿的矿震（冲击地压）发生条件、时空分布与某些征兆的调查研究，提出了利用矿震及其前兆观测探索天然地震前兆与预报方法的初步设想。  相似文献   

Oscillations de l'atmosphère de l'étoile pulsante     

Mine Takeuti 《Astrophysics and Space Science》1969,3(2):219-228

Résumé On étudie les oscillations non-adiabatiques d'une atmosphère stellaire sous l'approximation du premier ordre, en déduisant les solutions générales des équations différentielles. On confirme les conditions aux limites de la pulsation d'étoile. Pour les étoiles variables des supergéantes rouges l'onde progressive est possible dans l'atmosphère, avec l'oscillation stationnaire.

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Non-adiabatic linear oscillations of the stellar atmosphere are studied by deriving the general solution of the equation of the problem. Boundary conditions which we obtained at the stellar surface are confirmed for the pulsation of the cepheid variables. It is shown that the progressive wave coupling with the stellar pulsation is possible in the atmospheres of red supergiants.

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白云鄂博矿床东矿段深部及白云向斜核部探矿的可行性探讨   总被引：5，自引：0，他引：5  

柳建勇苏胜旺  张台荣章雨旭 《地质论评》2006,52(6):821-825

白云鄂博东矿（铁矿石）已属于轻度危机矿山，解决白云鄂博东矿的资源接续问题已迫在眉睫。依据老地质资料和生产过程中的新发现，参考多位矿床成因研究专家的成果，笔者等认为在白云鄂博东矿体深部及白云向斜核部探矿是可行的。  相似文献   

The effect of synchronization on the modal selection in classical cepheids     

M. Takeuti 《Astrophysics and Space Science》1985,109(1):99-109

The coupled self-exciting oscillator model is investigated in the non-resonant case and applied to classical cepheids. The modal selection in these models is explained as the result of the synchronization caused by the mutual interaction between different modes. By using linear adiabatic coupling coefficients, it is shown that the fundamental mode suppresses the first overtone mode marginally in short-period classical cepheids. The double periodicity of several cepheids is expected as the result of a small change of physical state in the outer envelopes of these stars.  相似文献   

Study of time-evolving hydrodynamic cepheid models     

Mine Takeuti 《Astrophysics and Space Science》1986,119(1):37-40

For studying modal coupling, we ran the hydrodynamic models of cepheids and observed the growth and disappearance of various modes in their pulsation. The existence of modal coupling has been confirmed.Paper presented at the IAU Third Asian-Pacific Regional Meeting, held in Kyoto, Japan, between 30 September–6 October, 1984.  相似文献