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991.
The vertical mesoscale flux in the nocturnal boundary layer is generally considered to be difficult to estimate because of the small mesoscale vertical velocities and the large random variation of the mesoscale fluxes. However, the mesoscale vertical flux of heat, computed from FLOSSII data, varies quasi-systematically with height, stability and time scale. Such systematic variation requires correction for sonic misalignment and averaging over a large quantity of data. The relation of the mesoscale heat flux to the vertical structure of the nocturnal boundary layer is examined. For the most common conditions, the vertical convergence of the mesoscale heat flux acts to reduce the nocturnal cooling rate. Important uncertainties are discussed as well as the need for improved observations. 相似文献
992.
Milton Rojas Gamarra Mônica Baptista Pereira Estrázulas Steven R. Gullberg César A. Zen Vasconcellos 《Astronomische Nachrichten》2024,345(2-3):e230181
Inferences are made about the relationship that existed between the Ushnus, pyramid-shaped, terraced structures used by the Incas in the most important ceremonies of the Tawantinsuyo, and Inka Astronomy. We draw attention to Ayni, Kawsaypacha, Duality, and Tinkuy principles, multidimensional codes of conduct and wisdom that are at the root of the Andean cosmovision and on their perception of the world and the Cosmos. These principles, examined as postulates, allow to elaborate axiomatic propositions to identify the Ushnus with ancient Astronomy practices. In a complementary statement, starting from a bi-conditional proposition, we may infer through reciprocal corollaries that the Inka earliest roots to a holistic learning and educational ambient in the Tawantinsuyo was not elitist, instead it was based on a epistemological construct that differs from the corresponding Western educational ambients. An epistemological and cognitive approach allows to identify an ancient elaborate process of knowledge construction, based on the four fundamental principles, corresponding to different levels of assimilation and comprehension. As a complementary aspect, we identify some of the most preserved Ushnus of the Inka “Empire.” Then we complement this contribution with a broader interpretation for the Ushnus. 相似文献
993.
Ahmed A. Balogun Jimmy O. Adegoke Sajith Vezhapparambu Matthias Mauder Joseph P. McFadden Kevin Gallo 《Boundary-Layer Meteorology》2009,133(3):299-321
Previous measurements of urban energy balances generally have been limited to densely built, central city sites and older
suburban locations with mature tree canopies that are higher than the height of the buildings. In contrast, few data are available
for the extensive, open vegetated types typical of low-density residential areas that have been newly converted from rural
land use. We made direct measurements of surface energy fluxes using the eddy-covariance technique at Greenwood, a recently
developed exurban neighbourhood near Kansas City, Missouri, USA, during an intensive field campaign in August 2004. Energy
partitioning was dominated by the latent heat flux under both cloudy and near clear-sky conditions. The mean daytime Bowen
ratio (β) values were 0.46, 0.48, and 0.47 respectively for the cloudy, near clear-sky and all-sky conditions. Net radiation (R
n
) increased rapidly from dawn (−34 and −58W m−2) during the night to reach a maximum (423 and 630W m−2) after midday for cloudy and near clear-sky conditions respectively. Mean daytime values were 253 and 370W m−2, respectively for the cloudy and near clear-sky conditions, while mean daily values were 114 for cloudy and 171W m−2 for near clear-sky conditions, respectively. Midday surface albedo values were 0.25 and 0.24 for the cloudy and near clear-sky
conditions, respectively. The site exhibited an angular dependence on the solar elevation angle, in contrast to previous observations
over urban and suburban areas, but similar to vegetated surfaces. The latent heat flux (Q
E
), sensible heat flux (Q
H
), and the residual heat storage ΔQ
s
terms accounted for between 46–58%, 21–23%, and 18–31% of R
n
, respectively, for all-sky conditions and time averages. The observed albedo, R
n
, and Q
E
values are higher than the values that have been reported for suburban areas with high summer evapotranspiration rates in
North America. These results suggest that the rapidly growing residential areas at the exurban fringe of large metropolitan
areas have a surface energy balance that is more similar to the rural areas from which they were developed than it is to the
older suburbs and city centres that make up the urban fabric to which they are being joined. 相似文献
994.
L. González-Miqueo D. Elustondo E. Lasheras R. Bermejo J. M. Santamaría 《Journal of Atmospheric Chemistry》2009,62(1):59-72
A biomonitoring survey using the moss species Hypnum cupressiforme Hedw. was performed in the North of Navarra (Spain) in 2006. The levels of V, Cr, Mn, Ni, Cu, Zn, As, Zr, Cd, Hg and Pb,
and the total nitrogen content were determined in the samples by means of ICP-MS, CV-AA, and the Kjeldahl method. PCA analysis
showed a differentiation between lithogenic (V, Cr, Mn, Ni, As and Zr) and anthropogenic elements (Mn, Cu, Zn, Cd, Hg and
Pb). Spatial distribution maps were drawn using the kriging method, in order to identify the most affected areas and the main
pollution sources. A similar spatial distribution was observed for the elements belonging to each group separated by the PCA,
showing an important contribution from metal industries located in the Basque Country, as well as influence of long-range
transboundary pollution processes. Background levels were also determined for the study area, along with the contamination
factor for the different elements analysed. Mosses seemed to be good biomonitors of N deposition in areas of accumulation. 相似文献
995.
J. Angel Fernández Angela Ares Ana Rey-Asensio Alejo Carballeira Jesus R. Aboal 《Journal of Atmospheric Chemistry》2009,63(1):1-11
The effects of growth of autoirrigated, shaded transplants of Pseudoscleropodium purum on the quantification of tissue concentrations of Cd, Cu, Hg, V and Zn, were investigated in 4 exposure periods, each of
56 days, at 7 sampling sites (contaminated and uncontaminated). Concentrations of the elements in the basal portions of the
moss shoots were compared with the concentrations in the portions of the shoots that grew during the exposure period. Mercury
and V were present at lower concentrations in the new portions of the shoots than in the basal portions, whereas the opposite
was true for Cd, Cu and Zn. The magnitude of error introduced by growth was not negligible, and in some cases was higher than
40%, relative to the results obtained by analysis of the whole shoot. Devitalization of moss prior to its use as transplant
material is recommended to avoid growth of the plant during the exposure period. 相似文献
996.
Daniel Higuero Juan M. Tirado Jesús Carretero Fernando Félix Antonio de la Fuente 《Astrophysics and Space Science》2009,321(3-4):169-175
Institutions such as NASA, ESA or JAXA find solutions to distribute data from their missions to the scientific community, and their long term archives. This is a complex problem, as it includes a vast amount of data, several geographically distributed archives, heterogeneous architectures with heterogeneous networks, and users spread around the world. We propose a novel architecture that solves this problem aiming to fulfill the requirements of the final user. Our architecture is a modular system that provides a highly efficient parallel multiprotocol download engine, using a publisher/subscriber policy which helps the final user to obtain data of interest transparently. We have evaluated a first prototype, in collaboration with the ESAC centre in Villafranca del Castillo (Spain) that shows a high scalability and performance, opening a wide spectrum of opportunities. 相似文献
997.
István Horváth 《Astrophysics and Space Science》2009,323(1):83-86
The BeppoSAX Catalog has been very recently published. In this paper we analyze—using the Maximum Likelihood (ML) method—the
duration distribution of the 1003 GRBs listed in the catalog with duration. The ML method can identify the long and the intermediate
duration groups. The short population of the bursts is identified only at a 96% significance level. MC simulation has been
also applied and gives a similar significance level; 95%. However, the existence of the short bursts is not a scientific question
after the Compton Gamma-Ray Observatory’s observation. Our minor result is this well-known fact that in the BeppoSAX data
the short bursts are under-represented, mainly caused by the different triggering system. Our major result is the identification
of the intermediate group in the BeppoSAX data. Therefore, four different satellites (CGRO, Swift, RHESSI and BeppoSAX) observed
the intermediate type Gamma-Ray Burst. 相似文献
998.
Jesús López H. Fabio Bresolin Elena Terlevich Roberto Terlevich Daniel Rosa-González 《Astrophysics and Space Science》2009,324(2-4):351-354
We present preliminary results obtained from integral-field (IFU) data of the giant extragalactic Hii region NGC5461, located in a spiral arm (RA=14h03m41.4s, dec=+54°19′05″) of M101. The spatial and spectral information obtained with IFUs allows us to decompose the Hii region and analyze it at high resolution. 相似文献
999.
Javier Rodríguez Zaurín Joanna Holt Clive N. Tadhunter Rosa M. González Delgado 《Astrophysics and Space Science》2009,324(2-4):225-229
We use long-slit spectra taken with the William Herschel Telescope on La Palma and high-resolution Hubble Space Telescope imaging to study the gas kinematic in the halo of the ultraluminous infrared/radio galaxy PKS1345+12 (z=0.122). Our long-slit spectra show line splitting at the locations of massive star clusters ( $10^{6}<M_{\mathrm{SSC}}^{\mathrm{YSP}}<10^{7}$ M⊙), indicating that they are moving at up to 450 km?s?1 with respect to the local ambient gas. Given their kinematics, it is plausible that these super star clusters have been formed either in fast-moving gas streams or tidal tails that are falling back into the nuclear regions as part of the merger process, or as a consequence of jet-induced star formation linked to the extended, diffuse radio emission detected in the halo of the galaxy. 相似文献
1000.
Enrique Pérez Richard de Grijs Rosa M. González Delgado 《Astrophysics and Space Science》2009,324(2-4):79-81