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1.
Arnaud M. Aubourg E. Bareyre P. Br';ehin S. Caridroit R. de Kat J. Dispau G. Djidi K. Gros M. Lachièze-Rey M. Laigneau Y. Laurent B. Lesquoy E. Lavocat Ph. Magneville C. Mazeau B. Milsztajn A. Moscoso L. Pasquaud J. Paul B. Perrin P. Petibon J. Piret Y. Queinnec F. Rich J. Spiro M. de Trogoff J. Vigroux L. Zylberajch S. Ansari R. Cavalier F. Moniez M. Beaulieu J. P. Ferlet R. Grison Ph. Vidal-Madjar A. Adrianzyk G. Berger J. P. Burnage R. Delclite J. C. Kohler D. Magnan R. Richaud A. Guibert J. Moreau O. Tajahmady F. Baranne A. Maurice E. Prévôt L. Gry C. 《Experimental Astronomy》1994,4(3-4):265-278
A 20cm
2
CCD mosaic camera has been especially built to search for dark galactic halo objects by the gravitational microlensing effect. The sensitive area is made of 16 edge-buttable CCDs developped by Thomson-CTS, with 23×23 µm
2
pixels. The 35 kg camera housing and mechanical equipment is presented. The associated electronics and data acquisition system are described in a separate paper. The camera resides at the focal plane of a 40 cm, f/10, Ferson reflector. The instrument has been in operation since December 1991 at the La Silla Observatory (ESO). 相似文献
2.
近年来月球探测已经进入了一个全新的时代。特别是 1 990年以来 ,多个月球探测计划已经被成功实现 ,而且另外还有多个探测计划也在准备当中 ,并将在未来的几年内发射升空。在这种背景之下 ,中国的航天机构和有关的科学家也开始积极酝酿和开发自己的月球探测计划。这些月球探测计划将利用卫星上搭载的各种仪器探测和测量月球的地质和地理特性、化学成分和矿物组成、月球物理学特征以及包含地球大气在内的地月空间环境和行星际空间环境 ;进一步研究月球的起源和演化 ,探明月面环境 ,研究太阳等离子体物理 ,提供月面天文台和月面长期科研基地的候选地址 ,调查月球上的可利用资源 ,为将来开发月球提供充实的背景资料。参与新一轮的月球探测同样也为中国天文学研究带来了新的机会。 相似文献
3.
4.
H. Flanquart C. Meur-Férec Ph. Deboudt V. Morel A.-P. Hellequin et al. 《GeoJournal》1991,24(2):223-223
Reports
Littoral '92 相似文献5.
1Introduction Since the last glacial maximum, the Holocenehas been marked by a rapid rise in sea level. After6 000 a BP, the present-day level was reached andthe rate of sea-level rise (SLR) decreased rapidly(Morzadec -Kerfourn, 1974; Kidson, 1986 ).These… 相似文献
6.
7.
Toward a generic method for studying water renewal, with application to the epilimnion of Lake Tanganyika 总被引:3,自引:0,他引:3
Olivier Gourgue Eric Deleersnijder Laurent White 《Estuarine, Coastal and Shelf Science》2007,74(4):628
We present a method, based on the concept of age and residence time, to study the water renewal in a semi-enclosed domain. We split the water of this domain into different water types. The initial water is the water initially present in the semi-enclosed domain. The renewing water is defined as the water entering the domain of interest. Several renewing water types may be considered depending on their origin. We present the equations for computing the age and the residence time of a certain water type. These timescales are of use to understand the rate at which the water renewal takes place. Computing these timescales can be achieved at an acceptable extra computer cost.The above-mentioned method is applied to study the renewal of epilimnion (i.e. the surface layer) water in Lake Tanganyika. We have built a finite element reduced-gravity model modified to take into account the water exchange between the epilimnion and the hypolimnion (i.e. the bottom layer), the water supply from precipitation and incoming rivers, and the water loss from evaporation and the only outgoing river. With our water renewal diagnoses, we show that the only significant process in the renewal of epilimnion water in Lake Tanganyika is the water exchange between the epilimnion and the hypolimnion, other phenomena being negligible. 相似文献
8.
The turbulent motions responsible for ocean mixing occur on scales much smaller than those resolved in numerical simulations
of oceanic flows. Great progress has been made in understanding the sources of energy for mixing, the mechanisms, and the
rates. On the other hand, we still do not have adequate answers to first order questions such as the extent to which the thermohaline
circulation of the ocean, and hence the earth's climate, is sensitive to the present mixing rates in the ocean interior. Internal
waves, generated by either wind or flow over topography, appear to be the principle cause of mixing. Mean and eddy flows over
topography generate internal lee waves, while tidal flows over topography generate internal tides. The relative importance
of these different internal wave sources is unknown. There are also great uncertainties about the spatial and temporal variation
of mixing. Calculations of internal tide generation are becoming increasingly robust, but we do not know enough about the
subsequent behavior of internal tides and their eventual breakdown into turbulence. It does seem, however, that most internal
tide energy flux is radiated away from generation sites as low modes that propagate over basin scales. The mechanisms of wave-wave
interaction and topographic scattering both act to transfer wave energy from low modes to smaller dissipative scales.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
9.
Th sorption and export models in the water column: A review 总被引:2,自引:3,他引:2
Nicolas Savoye Claudia Benitez-Nelson Adrian B. Burd J. Kirk Cochran Matthew Charette Ken O. Buesseler George A. Jackson Matthieu Roy-Barman Sabine Schmidt Marc Elskens 《Marine Chemistry》2006,100(3-4):234
Over the past few decades, the radioisotope pair of 238U / 234Th has been widely and increasingly used to describe particle dynamics and particle export fluxes in a variety of aquatic systems. The present paper is one of five review articles dedicated to 234Th. It is focused on the models associated with 234Th whereas the companion papers (same issue) are focused on present and future methodologies and techniques (Rutgers van der Loeff et al.), C / 234Th ratios (Buesseler et al.), 234Th speciation (Santschi et al.) and present and future applications of 234Th [Waples, J.T., Benitez-Nelson, C.R., Savoye, N., Rutgers van der Loeff, M., Baskaran, M., Gustafsson, Ö., this issue. An Introduction to the application and future use of 234Th in aquatic systems. Marine Chemistry, FATE special issue]. In this paper, we review current 234Th scavenging models and discuss the relative importance of the non-steady state and physical terms associated with the most commonly used model to estimate 234Th flux. Based on this discussion we recommend that for future work the use of models should be accompanied by a discussion of the effect that model and data uncertainty have on the model results. We also suggest that future field work incorporate repeat occupations of sample sites on time scales of 1–4 weeks in order to evaluate steady state versus non-steady state estimates of 234Th export, especially during high flux events (> ca. 800 dpm m− 2 d− 1). Finally, knowledge of the physical oceanography of the study area is essential, particularly in ocean margins and in areas of established upwelling (e.g., Equatorial Pacific). These suggestions will greatly enhance the application of 234Th as a tracer of particle dynamics and flux in more complicated regimes. 相似文献
10.
中伊朗盆地Garmsar区块Qom组沉积微相及储层特征研究 总被引:1,自引:1,他引:0
伊朗Garmsar区块Qom组形成于碳酸盐岩台地沉积环境,岩性以生物屑灰岩、含砂生物屑灰岩、泥晶灰岩为主,是典型的裂缝~孔隙型储层。利用区内野外实测剖面资料和露头岩样测试资料,对Qom组沉积相进行标识及类型划分,并对Qom组沉积微相及其平面展布特征进行分析,指出了该区域开阔台地相~高能红藻滩微相和局限台地相~泻湖夹台内滩微相是研究区储层发育的有利部位。F段中部的粒内溶孔较为发育,而溶缝主要出现在C1、C3亚段,整个Qom组构造微裂缝不甚发育。但储层孔渗条件比较差,属于中~低孔、低渗~特低渗储层,且存在严重的不均一性。为此,从沉积相与储层特征角度研究认为,中伊朗盆地Garmsar区块Qom组油气勘探存在一定的风险。 相似文献