Atmospheres of retail and the asceticism of civilized consumption

Abstract. During recent decades, consumption-oriented spaces of comfort and hospitality have proliferated – including, for instance, lounge shopping malls, food court plazas, spas, entertainment retail, visitor centres, and the development of ever larger pedestrian precincts. In this article we explore shopping malls as capitalist "domes" in Sloterdijk's sense. We observe atmospheric production, atmospheric management and atmospheric culture (which we propose to call atmoculture) inside such domes. Processes of retailization and mallification – whereby shopping malls and retail spaces absorb increasing economic and societal energies – can be regarded as correlative to the rise of an atmoculture of civilized consumption. Such atmoculture is visible for instance in stress-avoidance strategies and the production of a pleasurable experience in consumption-oriented public zones. The design of contemporary retail spaces seems to pivot around specific atmospheric strategies developed to promote and sustain civilized consumption. In this piece, we describe four different strategies of atmospheric production, identifying their possible shortcomings and failings. Finally, we advance the hypothesis that the atmospheric production of retail can also be analyzed with reference to Sloterdijk's theorization of asceticism as self-disciplination.</p

Urban animals – domestic, stray and wild: notes from a bear repopulation project in the alps

This piece explores “domesticity” as a social territory defined by its relationship with the conceptual and ecological space of “the wild,” and asks whether these spaces stand in opposition to each other or more subtle relations of co-implication are at play. As we look into the domestic and the wild, a conceptual map of notions emerges, including the public, the common, the civilized, and the barbarian. The paper suggests the domestic and the wild constitute two semiotic-ecological domains constantly stretching into each other without any stable or even clear boundary line, and it elaborates on a series of corollaries for studying non-human animals in urban contexts. As an illustrative case study, we follow the story of Daniza, a wild brown bear introduced in the Brenta Natural Park on the Italian Alps in the 2000s. Declared a “dangerous animal,” Daniza was accidentally, and controversially, killed by the public authorities in 2014.info:eu-repo/semantics/acceptedVersio

Galactic Outflows and the pollution of the Galactic Environment by Supernovae

We here explore the effects of the SN explosions into the environment of star-forming galaxies like the Milky Way. Successive randomly distributed and clustered SNe explosions cause the formation of hot superbubbles that drive either fountains or galactic winds above the galactic disk, depending on the amount and concentration of energy that is injected by the SNe. In a galactic fountain, the ejected gas is re-captured by the gravitational potential and falls back onto the disk. From 3D nonequilibrium radiative cooling hydrodynamical simulations of these fountains, we find that they may reach altitudes up to about 5 kpc in the halo and thus allow for the formation of the so called intermediate-velocity-clouds (IVCs) which are often observed in the halos of disk galaxies. The high-velocity-clouds that are also observed but at higher altitudes (of up to 12 kpc) require another mechanism to explain their production. We argue that they could be formed either by the capture of gas from the intergalactic medium and/or by the action of magnetic fields that are carried to the halo with the gas in the fountains. Due to angular momentum losses to the halo, we find that the fountain material falls back to smaller radii and is not largely spread over the galactic disk. Instead, the SNe ejecta fall nearby the region where the fountain was produced, a result which is consistent with recent chemical models of the galaxy. The fall back material leads to the formation of new generations of molecular clouds and to supersonic turbulence feedback in the disk.Comment: 10 pages, 5 figures; paper of invited talk for the Procs. of the 2007 WISER Workshop (World Space Environment Forum), Alexandria, Egypt, October 2007, Spa. Sci. Rev

Mistura em tanque de boro e herbicidas em semeadura convencional de girassol.

Os objetivos deste experimento foi avaliar a resposta do girassol às aplicações de boro (B), isoladas ou em mistura com herbicidas, e o controle de plantas daninhas por meio de experimento conduzido na Embrapa Soja, Londrina-PR. Os tratamentos foram acetochlor (1,92 kg i.a. ha-1), oxyfluorfen (0,36 kg i.a. ha-1), sulfentrazone (0,35 kg i.a.ha-1), trifluralin (1,80 kg i.a. ha-1) e as testemunhas capinada e sem capina. Todos os tratamentos foram aplicados, isoladamente ou em mistura, com 2 kg ha-1 de B (Na2B4O7.10H20 ? bórax e H3BO3 ? ácido bórico). O tratamento mais eficiente foi acetochlor mais ácido bórico; essa combinação resultou em solução mais homogênea da calda de pulverização, quando comparada com os herbicidas mais bórax. O herbicida acetochlor aplicado isoladamente ou em mistura com as duas fontes de B foi eficiente no controle da trapoeraba (Commelina benghalensis), do picão-preto (Bidens pilosa) e da corda-de-viola (Ipomoea grandifolia). Os herbicidas oxyfluorfen e sulfentrazone, aplicados isoladamente ou em misturas com as duas fontes de B, foram eficientes no controle do amendoim-bravo (Euphorbia heterophylla) e da corda-de-viola, respectivamente. É viável a aplicação de boro juntamente com os herbicidas testados nesta pesquisa em mistura em tanque, evitando a deficiência desse micronutriente e controlando as plantas daninhas na cultura do girassol

Bidens pilosa L. (Asteraceae) control in sunflower with residual herbicides.

Abstract One of the most damaging species in sunflower crops in Brazil is the hairy beggartick (Bidens pilosa L). The large number of seeds, the various vegetative cycles during the year, the staggered germination and the scarcity of selective and effective herbicides to control this weed in sunflower are some of attributes that hinder the control of hairy beggartick populations. Two experiments were carried out to evaluate the control of hairy beggarticks, as well as sunflower tolerance to herbicides. The treatments were as follows: S-metolachlor (1,200 and 2,400 g ai ha-1), flumioxazin (60 and 120 g ai ha-1), and sulfentrazone (150 and 300 g ai ha-1) and two controls (weedy and weed-free check). The selectivity of the herbicides was higher at low doses. Flumioxazin and sulfentrazone caused injury to sunflowers at the highest doses and mainly in sandy soils. Although S-metolachlor did not cause visual symptoms of injury, the higher dose reduced sunflower yield. The herbicides sulfentrazone and flumioxazin provided satisfactory control of hairy beggartick plants in both types of soils. S-metolachlor presented medium control of hairy beggarticks in clay soil; however, its efficiency was slightly higher when applied in sandy soil. The most efficient herbicide for controlling hairy beggartick plants was flumioxazin, followed by sulfentrazone

Baryonically Closed Galaxy Groups

Elliptical galaxies and their groups having the largest L_x/L_B lie close to the locus in the L_x,L_B diagram expected for closed systems with baryon fractions equal to the cosmic mean value, f_b = 0.16. The estimated baryon fractions for several of these galaxies/groups are also close to 0.16 when the gas density is extrapolated to the virial radius. Evidently they are the least massive baryonically closed systems. Gas retention in these groups implies that non-gravitational heating cannot exceed about 1 keV per particle, consistent with the heating required to produce the deviation of groups from the L_x - T correlation for more massive clusters. Isolated galaxies/groups with X-ray luminosities significantly lower than baryonically closed groups may have undermassive dark halos, overactive central AGNs, or higher star formation efficiencies. The virial mass and hot gas temperatures of nearly or completely closed groups correlate with the group X-ray luminosities and the optical luminosities of the group-centered elliptical galaxy, an expected consequence of their merging history. The ratio of halo mass to the mass of the central galaxy for X-ray luminous galaxy/groups is about 80.Comment: 7 pages; Accepted by ApJ Letter

Manual de identificação e manejo de plantas daninhas em cultivos de cana-de-açúcar.

bitstream/item/26157/1/Manual-Brighenti.pd

3D Numerical Simulations of AGN Outflows in Clusters and Groups

We compute 3D gasdynamical models of jet outflows from the central AGN, that carry mass as well as energy to the hot gas in galaxy clusters and groups. These flows have many attractive attributes for solving the cooling flow problem: why the hot gas temperature and density profiles resemble cooling flows but show no spectral evidence of cooling to low temperatures. Subrelativistic jets, described by a few parameters, are assumed to be activated when gas flows toward or cools near a central SMBH. Using approximate models for a rich cluster (A1795), a poor cluster (2A 0336+096) and a group (NGC 5044), we show that mass-carrying jets with intermediate mechanical efficiencies ($\sim10^{-3}$) can reduce for many Gyr the global cooling rate to or below the low values implied by X-spectra, while maintaining $T$ and $\rho$ profiles similar to those observed, at least in clusters. Groups are much more sensitive to AGN heating and present extreme time variability in both profiles. Finally, the intermittency of the feedback generates multiple generations of X-ray cavities similar to those observed in Perseus cluster and elsewhere. Thus we also study the formation of buoyant bubbles and weak shocks in the ICM, along with the injection of metals by SNIa and stellar winds.Comment: 4 pages, 2 figures, to appear in proceedings of the conference "The Monster's Fiery Breath: Feedback in Galaxies, Groups, and Clusters", June 2009, Madison Wisconsi

Turbulent Mixing in Clusters of Galaxies

We present a spherically-symmetric, steady-state model of galaxy clusters in which radiative cooling from the hot gas is balanced by heat transport through turbulent mixing. We assume that the gas is in hydrostatic equilibrium, and describe the turbulent heat diffusion by means of a mixing length prescription with a dimensionless parameter alpha_mix. Models with alpha_mix ~ 0.01-0.03 yield reasonably good fits to the observed density and temperature profiles of cooling core clusters. Making the strong simplification that alpha_mix is time-independent and that it is roughly the same in all clusters, the model reproduces remarkably well the observed scalings of X-ray luminosity, gas mass fraction and entropy with temperature. The break in the scaling relations at kT \~ 1-2 keV is explained by the break in the cooling function at around this temperature, and the entropy floor observed in galaxy groups is reproduced naturally.Comment: Accepted for publication in ApJ