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排序方式: 共有275条查询结果,搜索用时 15 毫秒
91.
92.
In this short article we show that the sunspot cycle minima exhibit a long cycle (Gleissberg) in addition to the 11-yr cycle. From 1750 onwards, three periods of the Gleissberg cycle can be detected. 相似文献
93.
N. Prithivikumaran M. Fernandez Gomez J.J. Lopez Gonzalez S.P. Bagare N. Rajamanickam 《Astrophysics and Space Science》2002,280(4):319-324
The Franck-Condon (FC) factors (transition probabilities) and r-centroids have been evaluated by the reliable numerical integration procedure for the bands of the A
3 φ4 →X
3 φ4 system of astrophysical molecule CoH, using a suitable potential. The dissociation energy D
0
0 = 2.5 ± 0.05 eV for the electronic ground state of CoH has been estimated by fitting Hulburt-Hirschfelder function to the
experimental potential energy curve, using the correlation coefficient.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
94.
Jane Wigforss‐Lange Vivi Vajda Adriana Ocampo 《Meteoritics & planetary science》2007,42(11):1871-1882
Abstract— Four exposures of Chicxulub impact ejecta along the Mexico‐Belize border have been sampled and analyzed for major and trace element abundances. The ejecta deposits consist of a lower spheroid bed, containing clay and dolomite spheroids, and an upper diamictite bed with boulders and clasts of limestone and dolomite. The matrix of both beds is composed of clay and micritic dolomite. The rare earth element (REE) compositions in the matrix of both units show strong similarities in concentrations and pattern. Furthermore, the Zr/TiO2 scatter plot shows a linear correlation indicating one source. These results indicate that the basal spheroid bed has the same source and was generated during the same event as the overlying diamictite bed, which lends support to a single‐impact scenario for the Albion Formation ejecta deposits. The elevated concentrations of non‐meteoritic elements such as Sb, As, U, and Zn in the matrix of the lower spheroid bed are regarded to have been derived from the sedimentary target rocks at the Chicxulub impact site. The positive Eu and Ce anomalies in clay concretion and in the matrix of the lower part of the spheroid bed in Albion Island quarry is probably related to processes involved in the impact, such as high temperature and oxidizing conditions. Analogous trace element anomalies have been reported from the distal Cretaceous‐Paleogene (K/T) boundary clay layer at different sites. Thus, the trace element signals, reported herein, are regarded to support a genetic link between the Chicxulub impact, the ejecta deposits along the Mexico‐Belize border, and the global K/T boundary layer. 相似文献
95.
M. Merck A. Karle S. Martinez F. Arqueros K. H. Becker M. Bott-Bodenhausen R. Eckmann E. Faleiro J. Fernandez P. Fernandez V. Fonseca V. Haustein G. Heinzelmann I. Holl F. Just F. Krennrich M. Kühn E. Lorenz H. Meyer N. Müller R. Plaga J. Prahl M. Probst M. Rozanska M. Samorski H. Sander K. Sauerland C. Sesea W. Stamm 《Astroparticle Physics》1996,5(3-4):379-392
A precise knowledge of the angular resolution of scintillator arrays used to observe extended air showers (EAS) is of key importance in the search for VHE/UHE γ point sources. Four independent methods have been used to determine the mean resolution for which a value of ΔΘ63 of 0.8°(1.0°) at a proton threshold of 50 (40) TeV has been found for the HEGRA EAS-array. 相似文献
96.
Adriana Valio P. Kaufmann C. G. Giménez de Castro J.-P. Raulin L. O. T. Fernandes A. Marun 《Solar physics》2013,283(2):651-665
We present a new system of two circular polarization solar radio telescopes, POEMAS, for observations of the Sun at 45 and 90 GHz. The novel characteristic of these instruments is the capability to measure circular right- and left-hand polarizations at these high frequencies. The two frequencies were chosen so as to bridge the gap at radio frequencies between 20 and 200 GHz of solar flare spectra. The telescopes, installed at CASLEO Observatory (Argentina), observe the full disk of the Sun with a half power beam width of 1.4°, a time resolution of 10 ms at both frequencies, a sensitivity of 2?–?4 K that corresponds to 4 and 20 solar flux unit (=104 Jy), considering aperture efficiencies of 50±5 % and 75±8 % at 45 and 90 GHz, respectively. The telescope system saw first light in November 2011 and is satisfactorily operating daily since then. A few flares were observed and are presented here. The millimeter spectra of some flares are seen to rise toward higher frequencies, indicating the presence of a new spectral component distinct from the microwave one. 相似文献
97.
E. Aprile K. Arisaka F. Arneodo A. Askin L. Baudis A. Behrens K. Bokeloh E. Brown J.M.R. Cardoso B. Choi D. Cline S. Fattori A.D. Ferella K.L. Giboni A. Kish C.W. Lam J. Lamblin R.F. Lang K.E. Lim J.A.M. Lopes T. Marrodán Undagoitia Y. Mei A.J. Melgarejo Fernandez K. Ni U. Oberlack S.E.A. Orrigo E. Pantic G. Plante A.C.C. Ribeiro R. Santorelli J.M.F. dos Santos M. Schumann P. Shagin A. Teymourian D. Thers E. Tziaferi H. Wang C. Weinheimer M. LaubensteinS. Nisi 《Astroparticle Physics》2011,35(2):43-49
Results of the extensive radioactivity screening campaign to identify materials for the construction of XENON100 are reported. This dark matter search experiment is operated underground at Laboratori Nazionali del Gran Sasso (LNGS), Italy. Several ultra sensitive High Purity Germanium detectors (HPGe) have been used for gamma ray spectrometry. Mass spectrometry has been applied for a few low mass plastic samples. Detailed tables with the radioactive contaminations of all screened samples are presented, together with the implications for XENON100. 相似文献
98.
Licciano M Terlizzi A Giangrande A Cavallo RA Stabili L 《Marine environmental research》2007,64(4):504-513
The present study investigates the effect of the filtering activity of Sabella spallanzanii on the culturable heterotrophic bacterial community through the comparison of the bacterial diversity in transplanted polychaetes and the surrounding seawater. For isolation of culturable heterotrophic bacteria, seawater samples as well as polychaete homogenates were plated in triplicates onto Bacto Marine Agar 2216 (Difco). All the colonies grown were isolated, subcultured and identified by several morphological, biochemical and cultural methods. Some bacterial genera showed higher average abundances in polychaetes than in seawater (i.e. Lucibacterium and Photobacterium). Aeromonas represented a conspicuous component of the bacterial community both in S. spallanzanii and seawater. The presence of Cytophaga and Pseudomonas was also relevant in the examined seawater samples. The selective concentrations of some bacterial genera inside S. spallanzanii either by grazing on bacteria or their capability as bacterial reservoirs, provides evidence for the role of macrobenthic invertebrates as key determinants for microbial diversity. 相似文献
99.
Benjamin M. Moreton Jean-Michel Fernandez Mathieu B.D. Dolbecq 《Geostandards and Geoanalytical Research》2009,33(2):205-218
An iminodiacetate chelating resin was optimised for the rapid determination of Co, Cu, Fe, Mn and Ni in seawater. Using inexpensive, high-capacity, reusable cartridges allowed high flow rates of up to 25 ml min−1 . High preconcentration factors, of up to 500, were obtained in order to analyse samples using an ICP-OES. The requirement for a buffer was eliminated due to the high tolerance of the ICP-OES to interfering matrix elements, thereby further reducing the potential for contamination. Quantification limits in seawater were: Co = 6 ng l−1 , Cu = 8 ng l−1 , Fe = 6 ng l−1 , Mn = 5 ng l−1 and Ni = 6 ng l−1 . The method was verified by the analysis of near shore seawater (CASS-4) and open ocean seawater (NASS-5) reference materials. In order to satisfy the high sampling demands using the iminodiacetate cartridges, a portable off-line preconcentration unit was developed for routine analysis. The multi-channel preconcentration unit, was capable of treating up to eight samples simultaneously with concentrating times as little as 30 minutes. The technique was also used to determine dissolved metals in fresh and interstitial waters. The technique has been successfully used in a number of environmental studies and impact assessments to evaluate the effects of mining on the New Caledonian lagoon. 相似文献
100.
Adriana Giangrande Margherita Licciano Roberto Schirosi Luigi Musco Loredana Stabili 《Marine Ecology》2014,35(1):36-45
In the marine environment, sessile invertebrates have developed an impressive array of mechanisms to avoid predation, bacterial exploitation, and epibiotic overgrowth. In the present study we investigated several defensive strategies adopted by six sabellids: the hard bottom species Sabella spallanzanii (Gmelin, 1791), Branchiomma luctuosum Grube, 1869, Branchiomma bairdi (McIntosh, 1885), and Sabellastarte spectabilis (Grube, 1878), and the soft bottom species Myxicola infundibulum (Renier, 1804), and Megalomma lanigera (Grube, 1846), which have different morphological characteristics and geographical distribution. We examined and compared some defensive features such as branchial crown toughness, tube structure and strength, amount of released mucus, and antibacterial lysozyme‐activity in the mucus. The investigated species utilize a combination of defence and deterrence strategies that seems to be related to the colonized habitat. Tube strength was, higher in the hard bottom species compared with the soft bottom ones, where the tubes are generally buried and protected within the sediment. Branchial crown appeared stronger and resistant in hard bottom species, except for S. spallanzanii, which is the species showing the strongest tube. Sabella spallanzanii, M. infundibulum and S. spectabilis secreted high amount of mucus with high lysozyme‐like activity. By contrast, B. luctuosum, B. bairdi, and M. lanigera produced low amounts of mucus exerting lower antibacterial activity. 相似文献