Temporal and spatial expansion of the Egyptian goose Alopochen aegyptiacus in The Netherlands, 1967-94

1998 ◽  
Vol 25 (2) ◽  
pp. 251-263 ◽  
Author(s):  
Rob Lensink
Author(s):  
Arturo Arriagada ◽  
Ignacio Siles

This paper explores the configurations of social media’s affordances within the Chilean influencer industry. Chile has a growing number of professional social media influencers who blur global norms and local markets, working with both local brands and international campaigns. We argue for situating affordances within a wider context in which the features of platforms acquire particular meanings. Our analysis focuses on two dynamics. On the one hand, we examine how the Chilean influencer industry is shaped by a technological frame (Bijker, 1995) that structures the valence of affordances. We show that affordances are not “naturally” or “neutrally” imagined by actors but rather culturally located within technological frames that shape the discourses, values, and practices from which they obtain cultural meaning. On the other hand, we analyze how affordances provide a material support for the temporal and spatial expansion of technological frames. Thus, cultural contexts and platforms’ features mutually constitute each other in ways that have not always been recognized in the scholarly literature about affordances. We situate negotiations about what it means to be an influencer in Chile, the role of intermediaries (e.g. branding agencies), communication with followers, and the global influencer industry as part of this mutually constitutive relationship.


2001 ◽  
Vol 9 (3) ◽  
pp. 371-385 ◽  
Author(s):  
Tzung-Pei Hong ◽  
Ke-Yuan Huang ◽  
Wen-Yang Lin

In this paper, we consider the problem of finding good next moves in two-player games. Traditional search algorithms, such as minimax and α-β pruning, suffer great temporal and spatial expansion when exploring deeply into search trees to find better next moves. The evolution of genetic algorithms with the ability to find global or near global optima in limited time seems promising, but they are inept at finding compound optima, such as the minimax in a game-search tree. We thus propose a new genetic algorithm-based approach that can find a good next move by reserving the board evaluation values of new offspring in a partial game-search tree. Experiments show that solution accuracy and search speed are greatly improved by our algorithm.


2017 ◽  
Vol 17 (1) ◽  
Author(s):  
Lenny Hogerwerf ◽  
Manon M. C. Holstege ◽  
Elisa Benincà ◽  
Frederika Dijkstra ◽  
Wim van der Hoek

2004 ◽  
Vol 73 (4) ◽  
pp. 255-261 ◽  
Author(s):  
Daniel F.R. Cleary

Parasitoid assemblages infesting Yponomeuta species in the Netherlands were investigated. Parasitoid species richness and community composition were related to host species, habitat, temporal and spatial variation. Both community structure and species richness did not differ among habitats. There was no significant difference in species richness between years (1994 and 1995) but there was a significant difference in community composition. Community composition and species richness both differed among host species, although this latter result was solely due to the host species Y. evonymellus. There was no significant relationship between community similarity and distance. These results indicate that the parasitoids of the moth genus Yponomeuta in the Netherlands appear to form a spatially stable, but temporally variable community. Most of the variation in community structure was, however, related to the host species. The marked difference in parasitoid species richness and community composition of Y. evonymellus when compared to the other species warrants further study.


2019 ◽  
Vol 16 ◽  
pp. 103-111 ◽  
Author(s):  
Mathilde Marchand ◽  
Mireille Lefèvre ◽  
Laurent Saboret ◽  
Etienne Wey ◽  
Lucien Wald

Abstract. The present work deals with two well-known databases of hourly mean of solar irradiance that are derived from satellite imagery: the CAMS Radiation Service version 3.2, abbreviated as CAMS-Rad and part of the Copernicus Atmosphere Monitoring Service version 3.2 (CAMS), and the HelioClim-3 version 5, abbreviated as HC3v5. It adds up to the continuous documentation of these two databases that demonstrates that both databases capture the temporal and spatial variability of the solar radiation and are reliable sources of data. The spatial consistency of the uncertainties of these databases is verified against measurements performed within a dense network of ground stations in the Netherlands from the Royal Meteorological Institute KNMI for the period 2014–2017. For the CAMS-Rad database, the correlation coefficients between ground measurements and estimates are around 0.94–0.97 for irradiance E and 0.85–0.89 for clearness index KT. The bias ranges between −12 and 27 W m−2 (−4 % and 10 %). The standard deviation for E is almost constant at all stations and around 67 W m−2 (24 %) except at Valkenburg (57 W m−2, 20 %) and De Bilt (73 W m−2, 27 %). For this database, the statistical indicators are constant at inland stations showing the spatial consistency of the performances of CAMS-Rad dataset. At seashore stations, statistical indicators are more variable. The sea proximity influences CAMS-Rad performances and a weak spatial consistency is observed near seashore. For the HC3v5 database, the correlation coefficients are around 0.96–0.98 for E and 0.86–0.91 for KT. The bias ranges between −3 and 15 W m−2 (−1 % and 5 %). The standard deviation ranges between 48 (17 %) and 60 W m−2 (22 %). It is constant at inland stations and around 54 W m−2 (20 %) with peaks at Ell (59 W m−2, 21 %) and De Bilt (60 W m−2, 22 %). For this database, statistical indicators are constant at all stations as a whole, showing a strong spatial consistency of uncertainties. An exception is the standard deviation which tends to decrease at the seashore stations and is close to 50 W m−2 (17 %); this could be related to the general trend of decreasing standard deviation with increasing KT already reported in the scientific literature. As a whole, it is found that both databases are reliable sources on solar radiation in the Netherlands.


GeoResJ ◽  
2015 ◽  
Vol 5 ◽  
pp. 23-35 ◽  
Author(s):  
A. Poortinga ◽  
J.G.S. Keijsers ◽  
S.M. Visser ◽  
M.J.P.M. Riksen ◽  
A.C.W. Baas

2018 ◽  
Vol E101.D (1) ◽  
pp. 116-129 ◽  
Author(s):  
Shusaku EGAMI ◽  
Takahiro KAWAMURA ◽  
Akihiko OHSUGA

2018 ◽  
Vol 25 ◽  
pp. 9
Author(s):  
Gerrit Van Oosterom

This article claims that the influence of the nobility on the temporal and spatial development of the country house landscapes in the areas of Amstelland and the Oude Rijn was stronger than has previously been argued and remained visible long after the nobles themselves had left. In Amstelland the economic, social and cultural focus of the Catholic nobility that still owned land here shifted at the end of the seventeenth century to the southern part of the Netherlands and abroad. It offered the merchant elite of Amsterdam the opportunity to buy their prime locations and turn them into modern dairy farms combined with the first country houses in Amstelland. Along the Oude Rijn river many locations carried various noble connotations, which seemed to attract the status-sensitive members of the urban elite of both Amsterdam and Utrecht. They used the location – formerly a noble seat – and name of the place so as to associate themselves with a (true or fabricated) noble past.


1994 ◽  
Vol 144 ◽  
pp. 275-277
Author(s):  
M. Karlický ◽  
J. C. Hénoux

AbstractUsing a new ID hybrid model of the electron bombardment in flare loops, we study not only the evolution of densities, plasma velocities and temperatures in the loop, but also the temporal and spatial evolution of hard X-ray emission. In the present paper a continuous bombardment by electrons isotropically accelerated at the top of flare loop with a power-law injection distribution function is considered. The computations include the effects of the return-current that reduces significantly the depth of the chromospheric layer which is evaporated. The present modelling is made with superthermal electron parameters corresponding to the classical resistivity regime for an input energy flux of superthermal electrons of 109erg cm−2s−1. It was found that due to the electron bombardment the two chromospheric evaporation waves are generated at both feet of the loop and they propagate up to the top, where they collide and cause temporary density and hard X-ray enhancements.


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