ArgumentThe administration of mountain expeditions from the ground created special managerial problems. The Harvard College Observatory's Boyden Expeditions of 1887–1890 sent men and materiel to three sites: Pike's Peak, Colorado; Mount Wilson, California; and Chosica, Peru. Their goal was to test sites in order to find a suitable site for a permanent Boyden station to conduct astrophysical work in service of Harvard's preexisting projects. The logistical difficulties of living on the mountainside combined with the organizational difficulties of administrating a station (...) at a distance. The men who lived on the mountain were professionally vulnerable, and often cut off from their home observatory both by the weather conditions at their own altitude and local politics on the ground below them. Only when an unbroken line of communication could be established between the mountain station and the Harvard Observatory could the astronomers on both ends work together to create a successful expedition. (shrink)

The 1830s and 1840s witnessed a European movement to accumulate data about the terrestrial environment, enterprises including the German and British geomagnetic crusades. This movement was not limited to geomagnetic studies but notably included an important meteorological component. By focusing on observation practices in sedentary and expeditionary contexts, this paper shows how the developing fields of geomagnetism and meteorology were then intimately interlinked. It analyses the circulation and cross-connections of the practices and discourses shared by these two research fields. Departing (...) from a Humboldtian historiography, the paper especially stresses the role of Adolphe Quetelet, director of the Brussels Observatory, whose importance in the development of the earth sciences has until now been largely neglected. It reassesses the involvement of the French scientific community in the British and German geomagnetic crusades, moving beyond the well-known account of Arago's opposition to these undertakings. It is hoped thereby to contribute to a better historical understanding of the renewal of the earth sciences in the second quarter of the nineteenth century. (shrink)

“Today I made the ascent of the highest mountain in this region, which for good reasons is called Ventosum, guided only by the desire to see the extraordinary altitude of the place”. Petrarch's ascent of the Mont Ventoux in 1336, or rather his account of it, established the mountain as a distinctive place for experiencing and understanding nature and self. Since then, the mountain has been sought out in increasing numbers by those pursuing spiritual elevation, bodily exertion, and/or scientific investigation. (...) To this day, a pilgrimage church, several hotels, and an observatory are characteristically perched atop Mont Ventoux. And it is famous among cyclists as a legendarily difficultétapeof the Tour de France. (shrink)

SummaryDuring the 1920s and 1930s, Italian physicists established strong relationships with scientists from other European countries and the United States. The career of Bruno Rossi, a leading personality in the study of cosmic rays and an Italian pioneer of this field of research, provides a prominent example of this kind of international cooperation. Physics underwent major changes during these turbulent years, and the traditional internationalism of physics assumed a more institutionalized character. Against this backdrop, Rossi's early work was crucial in (...) transforming the study of cosmic rays into a branch of modern physics. His friendly relationships with eminent scientists — notably Enrico Fermi, Walther Bothe, Werner Heisenberg, Hans Bethe, and Homi Bhabha — were instrumental both for the exchange of knowledge about experimental practices and theoretical discussions, and for attracting the attention of physicists such as Arthur Compton, Louis Leprince-Ringuet, Pierre Auger and Patrick Blackett to the problem of cosmic rays. Relying on material from different archives in Europe and the United States, this case study aims to provide a glimpse of the intersection between national and international dimensions during the 1930s, at a time when the study of cosmic rays was still very much in its infancy, strongly interlaced with nuclear physics, and full of uncertain, contradictory, and puzzling results. Nevertheless, as a source of high-energy particles it became a proving ground for testing the validity of the laws of quantum electrodynamics, and made a fundamental contribution to the origins of particle physics. (shrink)

Summary The mesotrons, or mesons, were the first elementary particles observed to be inherently unstable. This essay offers a reconstruction of the stream of researches related to mesotron decay, and examines how these researches shaped some of the basic concepts and practices of the emerging field of particle physics. Mass measurements could not settle the question of whether the mesons were a homogeneous kind of particles or an assortment of particles with different masses. The assumption of a single mass prevailed (...) not on experimental grounds but because the mesons were identified tentatively with the carriers of the nuclear force according to a theory formulated by Hideki Yukawa. The identification gained currency because it entailed the prediction of meson decay, and thereby upheld the promise of a unified explanation of nuclear and cosmic-ray phenomena. In turn, the observation of decay and the measurement of the mean lifetime created the conditions for investigating the nuclear interactions of mesons at rest. Interest in these interactions was heightened, immediately after WWII, by the prospect of building and using accelerators to acquire knowledge about fundamental nuclear processes. Using decay to study nuclear capture, however, led to the realization that there exist not only different kinds of mesons but also two nuclear forces. (shrink)

ArgumentFrom 1893 to 1909 when it definitely sunk into the glacier, the Mont-Blanc Observatory (MBO) struggled to find its scientific purpose. In this article, we use recent literature on the social characterization of place to analyze this struggle. Our first goal is to investigate where the observatory may fit in the laboratory-field dyad. We investigate various kinds of conceptual “borderlands” between these places and look at the networking activities between particular knowledge production sites. We argue that part observatory, part laboratory, (...) and part field station, the place of the MBO was “heterotopic” space in Foucault's sense. We then examine the social underpinnings that led to the foundation of this observatory in the context of French Third Republic at the turn of the century. Following some of the ways the MBO was connected to other scientific sites and surveying some of its visitors' scientific practices, we finally hint at the fact that some of these practices played a part in the emergence of a regime of science production that endured into the twentieth century (astrophysical aeronautical practices, spatial stations, polar exploration, etc.). (shrink)