About: Chimney is a research topic. Over the lifetime, 8036 publications have been published within this topic receiving 43759 citations. The topic is also known as: smokestack & funnel.
TL;DR: In this article, a chimney model for the Galaxy is presented and its underlying physical principles are explained, where the Galactic disk and halo are connected by chimneys which are a consequence of superbubbles bursting out of the disk forming these collimated structures through which the global mass and energy exchange flows from disk to halo.
Abstract: A chimney model for the Galaxy is presented and its underlying physical principles are explained. The crucial point of the model is that the Galactic disk and halo are connected by chimneys which are a consequence of superbubbles bursting out of the disk forming these collimated structures through which the global mass and energy exchange flows from disk to halo. For canonical Galaxy parameters, the chimney phase is found to be associated with a mass flow rate of 0.3-3 solar masses/yr and a global power input of 10 to the 40th to 10 to the 42nd ergs/s. 72 refs.
TL;DR: Very well preserved fossil vent chimneys from the Silurian Yaman-Kasy volcanogenic-hosted massive sulfide have been studied in this article, where trace element distribution patterns across chimneys were found.
Abstract: Very well preserved fossil vent chimneys from the Silurian Yaman-Kasy volcanogenic-hosted massive sulfide
deposit in the Southern Urals range in decreasing temperatures from chalcopyrite-pyrite black smoker to sphalerite-
chalcopyrite-marcasite-pyrite gray smoker to sphalerite-quartz-barite white smoker assemblages. Laserablation
ICPMS analyses show systematic trace element distribution patterns across chimneys. Coarse-grained
layers of chalcopyrite in the central conduits are relatively high in Se and Sn but are low in other elements.
Chalcopyrite at the margins of such layers is enriched in Bi, Co, Au, Ag, Pb, Mo, Te, and As, which reside in
microinclusions of tellurides and/or sulfoarsenides. Sphalerite in the conduits and the outer chimney wall contains
elevated Sb, As, Pb, Co, Mn, U, and V. Antimony, As, and Pb reside in microinclusions of a galena-fahlore
assemblage, whereas the Co and Mn likely substitute for Zn2+ in the sphalerite structure. The highest concentrations
of most trace elements are found in colloform pyrite within the outer wall of the chimneys and likely
result from rapid precipitation under high- temperature-gradient conditions. The trace element concentrations
in the outer-wall colloform pyrite decrease in the following order, from the outer wall inward: Tl > Ag > Ni >
Mn > Co > As > Mo > Pb > Ba > V > Te > Sb > U > Au > Se > Sn > Bi, governed by the strong temperature
gradient. In contrast, pyrite in the high- to mid-temperature central conduits exhibit concentration of Se, Sn,
Bi, Te, and Au. The zone between the inner conduit and outer wall is characterized by recrystallization of colloform
pyrite to euhedral pyrite, which becomes depleted in all trace elements except Co, As and Se.
The mineralogical and trace element variations between chimneys are likely due to increasing fO2 and decreasing
temperature caused by mixing of hydrothermal fluids with cold oxygenated seawater. Average values
of Se (a high-temperature element) decrease in the order from black to gray to white smoker chimneys. The
medium-temperature association (Te, Bi, Co, Mo, and Au) is typically present in the gray smoker chimneys.
The white smoker chimneys are depleted in most elements except for Ag, Tl, Te, Sb, and As, probably due to
the dilution of the vent fluid by seawater which penetrates deeper parts of the hydrothermal system. U and V
are concentrated in the outer wall of most chimneys due to their extraction from seawater associated with the
more reduced fluids of black and gray smokers.
TL;DR: In this article, an analytical and numerical model was developed to estimate power output of solar chimneys as well as to examine the effect of various ambient conditions and structural dimensions on the power output.
TL;DR: In this article, the formation of mineral zoning across the walls of these structures throughout two major growth phases, a sulphate-dominated stage and a sulphide replacement stage, is discussed.
Abstract: Hollow mineral spires known as ‘black smoker’ chimneys precipitate around 350 °C jets of hydrothermal fluid spouting from the sea floor on the East Pacific Rise (EPR) at 21° N (refs 1, 2). I describe and discuss here the formation of mineral zoning across the walls of these structures throughout two major growth phases, a sulphate-dominated stage and a sulphide replacement stage. During the sulphide replacement stage, at least four distinct sulphide mineral zonation sequences develop across chimney walls from interior to exterior. The apparently successive formation of these sulphide zonation sequences is attributed to evolution of radial thermal and chemical gradients accompanying the gradual thickening and sealing of black smoker chimney walls.
TL;DR: In this paper, an experimental solar chimney model with uniform heat flux on one chimney wall with a variable chimney gap-to-height ratio between 1:15 and 2:5 and different heat flux and inclination angles was carried out.