A World Made for Money: Economy, Geography, and the Way We Live Today

2016 ◽  
Vol 106 (4) ◽  
pp. e62-e64
Author(s):  
William Wyckoff
Keyword(s):  
2017 ◽  
pp. 55-62
Author(s):  
Lisa Gitelman

Although mostly forgotten today, nickel-in-the-slot phonographs were a popular and telling symptom of acoustic modernity around 1890. At the rate of a minute or two of recorded sound per nickel deposited, these machines paved the way for the widespread private ownership of phonographs by pioneering their use a public venue where the uncanny experience of listening to absent voices was standardized by the logics of exchange and exhibition. The sound of money falling into the slots was answered automatically by the siren’s call of a voice with no speaker, calling for more money to be deposited. Because they flickered briefly at a conjunction of publics and markets, automatic phonographs provide a way to parse some of the conflicts attending the money economy during the 1890s, that crucial decade in the establishment of modernity as a technological way of life. Canning popular music, and privatizing its audition in serial acts of consumption, these devices were instrumental in the progressive abstraction of public space. Considering both the design and contexts of use of the devices helps to illuminate the conflicted subjectivities of markets and publics in the fin de siècle.


1972 ◽  
Vol 13 (3) ◽  
pp. 419-441 ◽  
Author(s):  
Martin A. Klein

This article is an effort to examine the way in which events during and, in some cases, before the nineteenth century shaped modern Senegambian society. It concludes:(1) That the slave trade contributed to the development of military structures and to the polarization of Senegambian societies between a warrior élite and an industrious Muslim peasant population.(2) That the change from the slave trade to legitimate commerce weakened the élites while strengthening the Muslim agriculturalists, who were able to accumulate guns and horses.(3) That tensions between the two conflicting groups go back at least to the seventeenth century, and that after 1860 they led to a series of revolutionary struggles. The agents of this revolution were a series of charismatic religious leaders.(4) That the course of this revolution was shaped by the involvement of European interests, and after 1854 increasingly by the incorporation of Senegambia in European spheres of influence.(5) That this merely postponed certain changes. By the beginning of the colonial period, Islam was clearly dominant, and Senegambia's rural populations were heavily involved in the money economy.


2018 ◽  
Vol 41 ◽  
Author(s):  
Maria Babińska ◽  
Michal Bilewicz

AbstractThe problem of extended fusion and identification can be approached from a diachronic perspective. Based on our own research, as well as findings from the fields of social, political, and clinical psychology, we argue that the way contemporary emotional events shape local fusion is similar to the way in which historical experiences shape extended fusion. We propose a reciprocal process in which historical events shape contemporary identities, whereas contemporary identities shape interpretations of past traumas.


2020 ◽  
Vol 43 ◽  
Author(s):  
Aba Szollosi ◽  
Ben R. Newell

Abstract The purpose of human cognition depends on the problem people try to solve. Defining the purpose is difficult, because people seem capable of representing problems in an infinite number of ways. The way in which the function of cognition develops needs to be central to our theories.


1976 ◽  
Vol 32 ◽  
pp. 233-254
Author(s):  
H. M. Maitzen

Ap stars are peculiar in many aspects. During this century astronomers have been trying to collect data about these and have found a confusing variety of peculiar behaviour even from star to star that Struve stated in 1942 that at least we know that these phenomena are not supernatural. A real push to start deeper theoretical work on Ap stars was given by an additional observational evidence, namely the discovery of magnetic fields on these stars by Babcock (1947). This originated the concept that magnetic fields are the cause for spectroscopic and photometric peculiarities. Great leaps for the astronomical mankind were the Oblique Rotator model by Stibbs (1950) and Deutsch (1954), which by the way provided mathematical tools for the later handling pulsar geometries, anti the discovery of phase coincidence of the extrema of magnetic field, spectrum and photometric variations (e.g. Jarzebowski, 1960).


Author(s):  
W.M. Stobbs

I do not have access to the abstracts of the first meeting of EMSA but at this, the 50th Anniversary meeting of the Electron Microscopy Society of America, I have an excuse to consider the historical origins of the approaches we take to the use of electron microscopy for the characterisation of materials. I have myself been actively involved in the use of TEM for the characterisation of heterogeneities for little more than half of that period. My own view is that it was between the 3rd International Meeting at London, and the 1956 Stockholm meeting, the first of the European series , that the foundations of the approaches we now take to the characterisation of a material using the TEM were laid down. (This was 10 years before I took dynamical theory to be etched in stone.) It was at the 1956 meeting that Menter showed lattice resolution images of sodium faujasite and Hirsch, Home and Whelan showed images of dislocations in the XlVth session on “metallography and other industrial applications”. I have always incidentally been delighted by the way the latter authors misinterpreted astonishingly clear thickness fringes in a beaten (”) foil of Al as being contrast due to “large strains”, an error which they corrected with admirable rapidity as the theory developed. At the London meeting the research described covered a broad range of approaches, including many that are only now being rediscovered as worth further effort: however such is the power of “the image” to persuade that the above two papers set trends which influence, perhaps too strongly, the approaches we take now. Menter was clear that the way the planes in his image tended to be curved was associated with the imaging conditions rather than with lattice strains, and yet it now seems to be common practice to assume that the dots in an “atomic resolution image” can faithfully represent the variations in atomic spacing at a localised defect. Even when the more reasonable approach is taken of matching the image details with a computed simulation for an assumed model, the non-uniqueness of the interpreted fit seems to be rather rarely appreciated. Hirsch et al., on the other hand, made a point of using their images to get numerical data on characteristics of the specimen they examined, such as its dislocation density, which would not be expected to be influenced by uncertainties in the contrast. Nonetheless the trends were set with microscope manufacturers producing higher and higher resolution microscopes, while the blind faith of the users in the image produced as being a near directly interpretable representation of reality seems to have increased rather than been generally questioned. But if we want to test structural models we need numbers and it is the analogue to digital conversion of the information in the image which is required.


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