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611.
R. Müller J.-U. Grooß D. S. McKenna P. J. Crutzen C. Brühl J. M. Russell III L. L. Gordley J. P. Burrows A. F. Tuck 《Annales Geophysicae》1998,17(1):101-114
Severe chemical ozone loss has been detected in the Arctic in the winter and spring of 1995–96 by a variety of methods. Extreme reductions in column ozone due to halogen catalysed chemistry were derived from measurements of the Halogen Occultation Experiment (HALOE) on board the Upper Atmosphere Research Satellite in the Arctic vortex. Here, we discuss further aspects of the HALOE observations in the Arctic over this period. Potential problems, both in the data themselves and in the methodology of the data analysis are considered and the reason for the differences between the Arctic ozone losses deduced from HALOE data version 17 and 18 is analysed. Moreover, it is shown that HALOE measurements in the Arctic in winter and spring 1995–96 compare well with observations by other ground-based and satellite instruments. 相似文献
612.
Dabrio Cristino J. Zazo Cari Lario Javier Goy José Luis Sierro Francisco J. Borja Francisco González José Ángel Flores José Abel 《Geologie en Mijnbouw》1998,77(3-4):263-281
This first sedimentary interpretation of two incised-valley fills in the Gulf of Cádiz (southern Spain), which accumulated during the last fourth-order eustatic cycle in response to fluvial incision, changes of sea level, and correlative deposition, relates the filling of the estuarine basins and their barriers with four regional progradation phases, H1 to H4. The cases studied are the wave-dominated Guadalete, and the mixed, tide and wave-dominated Odiel-Tinto estuaries. The sequence boundary is a type-1 surface produced during the lowstand of the Last Glacial period ca. 18 000 14C yr BP. No fluvial lowstand deposits were found in the area. Due to rapid transgression the valley fills consist of transgressive and highstand sediments. The maximum landward advance of the estuarine barriers occurred ca. 6500–6000 14C yr BP during the maximum of the Flandrian transgression, but there is no evidence of sea level rising appreciably above the present. A large part of the estuaries was filled during H1 (ca. 6500–4400 14C yr BP) but ravinement by shifting tidal inlets destroyed most of the coeval barriers. During the H2 phase (ca. 4200–2550 14C yr BP) sedimentation was favoured by arid conditions and concentrated in the axial estuarine zones and the barriers. Between H2 and H3 prevailing winds changed from W to WSW, increasing spit growth to the east and south-east. Progradation of bay-head deltas and flood-plains during H3 (ca. 2300–800 14C yr BP) and H4 (500 yr ago to the present) further reduced the accommodation space in the largely-filled valleys, and sediment by-passed the estuaries and accumulated in the estuarine barriers as fast-growing spits. Arid conditions and increasing human activity have caused rapid coastal modifications. 相似文献
613.
Mihály Horányi 《Astrophysics and Space Science》1998,264(1-4):257-271
This is a review of recent in situ and remote sensing observations, and theoretical advances of our understanding dust plasma
interactions in Jupiter's magnetosphere. Dust grains exposed to plasmas and UV radiation collect electrostatic charges and
their dynamics can be altered due to electric and magnetic fields. Hence, magnetospheric effects can shape the size and spatial
distributions of micron sized and smaller dust grains. The ring/halo region, the dust streams and the captured ring at Jupiter
are recent examples where dust plasma interaction effects can best explain the observations.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
614.
The paper is concerning with the light curve analysis of an active binary system of OO Aql. Basic orbital and physical parameters of this system were estimated by analysing photometric observations by Lafta and Grainger (1985) and Essam et al. (1992). Both groups of observations gave quite different light curves with a conspicuous asymmetry arising from unequal height of successive maxima. A slightly changed programme by Djuraevi (1992a) was applied. The programme was based on the Roche model and it included an option of overcontact configuration and active (bright or dark) spotted regions on the system's components. An inverse-problem method by Djuraevi (1992b) was used to estimate the parameters of the system and active regions. The light-curve analysis suggested a significant change in the system. For Lafta and Grainger's light curves our analysis showed the presence of a dark spotted area near the polar region of the primary component. This dark area covered about 22% of the primary's hemisphere. Essam et al.'s light curves had very complex shape. In this case the mechanism of the mass transfer and the exchange of the thermal energy between the components could produce a bright-spot (bs) area on the secondary, near the Lagrange equilibrium point L1 around the neck region between the stars. To explain a sharp increase of the system's brightness in the B filter immediately after the secondary minimum, we had to introduce also a hot-spot (hs) area of a high temperature contrast on the secondary. With the increase of the brightness in the V-filter being of much lower intensity, this hot spot region could be taken as a local eruption. The behaviour of the B–V colour index with the orbital phase is in favour of this hypothesis also. The obtained results show that the light-curve changes are due to development and moving of active spot regions on the components. 相似文献
615.
616.
The Gran Telescopio CANARIAS (GTC) is a high performance 10-m class telescope whose construction has been promoted by the
IAC (Instituto de Astrofísica de Canarias). It will be installed at the Roque de los Muchachos Observatory (ORM), in the island
of La Palma. First light is planned for end-2002. The key science drivers for the project are image quality, operational efficiency
and reliability, as emphasized in the Conceptual Design Document which was finished in mid-97. The Preliminary Design is now
proceeding on all aspects of the project. The GTC Project is presently funded at the 70% level by Spain. The scientific drives
behind the GTC project are described here, as well as the current technical, managerial, and operational baseline.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
617.
618.
Our main goal is to determine the dynamic equations of a certain complex system, as is the case of the mechanical system for
a small aperture telescope. Causes of this complexity are: the lack of documents about the operation of the elements belonging
to the system, and the variation of dynamics with respect to the time and the position of the telescope. To check that we
have obtained a valid set of dynamic equations, we will design a computer control system that will implement a self-guide
system for the telescope.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
619.
Josef Bochníček Tomáš Zelinka Reviewer T. Kolbenheyer 《Studia Geophysica et Geodaetica》1981,25(4):411-412
Summary The authors prove that the solution of Laplace's equation under Neumann's boundary conditions can be transformed to an advantage into determining the field which is generated by charges, induced by the external field at surfaces of discontinuity. 相似文献
620.
Summary The disturbing gravitational effect of the irregularities of the shape of the coremantle boundary are studied at a point on the Earth's surface. The effect is computed for models of local and zonal distribution of the disturbing masses under the assumption that the total mass of the Earth remains constant. Formulae giving the disturbing gravitational effect as a function of the distribution of the disturbing masses and of the position of the point of observation on the Earth's surface are derived for the individual models. Numerical values of the disturbances have been calculate in all cases. 相似文献