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121.
John E. Bailey Andrew J. L. Harris Jonathan Dehn Sonia Calvari Scott K. Rowland 《Bulletin of Volcanology》2006,68(6):497-515
An open channel lava flow on Mt. Etna (Sicily) was observed during May 30–31, 2001. Data collected using a forward looking
infrared (FLIR) thermal camera and a Minolta-Land Cyclops 300 thermal infrared thermometer showed that the bulk volume flux
of lava flowing in the channel varied greatly over time. Cyclic changes in the channel's volumetric flow rate occurred over
several hours, with cycle durations of 113–190 min, and discharges peaking at 0.7 m3 s−1 and waning to 0.1 m3 s−1. Each cycle was characterized by a relatively short, high-volume flux phase during which a pulse of lava, with a well-defined
flow front, would propagate down-channel, followed by a period of waning flow during which volume flux lowered. Pulses involved
lava moving at relatively high velocities (up to 0.29 m s−1) and were related to some change in the flow conditions occurring up-channel, possibly at the vent. They implied either a
change in the dense rock effusion rate at the source vent and/or cyclic-variation in the vesicle content of the lava changing
its bulk volume flux. Pulses would generally overspill the channel to emplace pāhoehoe overflows. During periods of waning
flow, velocities fell to 0.05 m s–1. Blockages forming during such phases caused lava to back up. Occasionally backup resulted in overflows of slow moving ‘a‘ā
that would advance a few tens of meters down the levee flank. Compound levees were thus a symptom of unsteady flow, where
overflow levees were emplaced as relatively fast moving pāhoehoe sheets during pulses, and as slow-moving ‘a‘ā units during
backup. Small, localized fluctuations in channel volume flux also occurred on timescales of minutes. Volumes of lava backed
up behind blockages that formed at constrictions in the channel. Blockage collapse and/or enhanced flow under/around the blockage
would then feed short-lived, wave-like, down-channel surges. Real fluctuations in channel volume flux, due to pulses and surges,
can lead to significant errors in effusion rate calculations.
Editorial responsibility: A. Woods 相似文献
122.
123.
《国际泥沙研究》2000,(4)
1 INTRODUCTIONThe exact mechanism of accumulation of sediments in point bars is not clearly known. Many scientistsinvestigated the problem. In the river Klaralven, Sundborg (1956) observed the development of sometransverse bars in the initial stage of the point bar formation. These transverse bars tend to becomelongitudinal as they extend close to the stream bed. Martvall and Nilsson (1972) investigated the problemof point bar formation experimentally in a laboratory flume. The flume st… 相似文献
124.
N. H. de Leeuw S. C. Parker C. R. A. Catlow G. D. Price 《Physics and Chemistry of Minerals》2000,27(5):332-341
We describe the application of atomistic simulation techniques to investigate the effect of associative and dissociative
adsorption of water on the structures and stabilities of the low-index surfaces of forsterite. All surfaces are amenable to
associative adsorption of water, while dissociative adsorption is energetically favourable on all but the non-dipolar {1 0 0}
surface. Often, otherwise unstable (dipolar) surfaces are stabilised to a large extent by hydration, e.g. the dipolar {0 1 0}
surface. However, on thermodynamic grounds we do not expect associatively adsorbed water to dissociate on all surfaces, as
the energies released for dissociative adsorption of water on the non-dipolar {0 1 0} and {1 0 0} surfaces are less than those
released for associative adsorption. As such, there is no energetic incentive for the associatively adsorbed water molecules
to dissociate. The stabilities of the two terminations of the {0 1 0} surface, the main cleavage plane of forsterite, are
reversed when hydroxylated, indicating that some dissolution of the magnesium ions may occur upon hydration, which is shown
to be an exothermic process for both surface terminations. The equilibrium morphology was calculated as a way of assessing
the change in surface energies. The experimental morphology of forsterite is adequately reproduced, suggesting that the relative
stabilities of the surfaces, both unhydrated and hydroxylated, are calculated correctly.
Received: 4 August 1999 / Revised, accepted: 11 October 1999 相似文献
125.
Antonin Genna Jean-Pierre Capdeville Jacques Dubreuilh Cyril Mallet 《Comptes Rendus Geoscience》2005,337(16):1474
A recent multidisciplinary study, comprising existing data analysis and geomorphological and geological fieldwork, has helped clarify marine erosion processes of Pyrenean formations along the Basque Coast. An important discovery was made during our study of an alterite of regional extent, which calls into question recent and present evolution of the Basque Coast and the processes leading to coastline retreat. Modelling these factors has made it possible to propose a predictive scenario for future coastal evolution. To cite this article: A. Genna et al., C. R. Geoscience 337 (2005). 相似文献
126.
Volcanic ash layers in sediment cores are valuable geochronological markers in paleolimnological research. The composition
of volcanic glass is related to identifiable, chronologically distinctive volcanic eruptions. Consequently, tephra layers
provide time horizons allowing regional-scale correlations for lake sediments. Volcanic glass is often present in samples
routinely prepared by paleolimnologists such as diatom slides and thin sections. Knowledge of the morphological and optical
properties of volcanic glass allows for its identification. This is essential for the identification of ash layers that are
not macroscopically visible or to track their vertical migration in soft organic sediments. The purposes of this note are
to: (1) describe how the morphological (i.e., shape, vesicularity) and optical (i.e., refractive index and birefringence)
properties can be used to identify volcanic glass in preparations from lake sediments; and (2) show how the quantification
of volcanic glass from diatom slides is used to quantify the density-induced displacement of a 4.5 cm-thick Mazama ash-layer
through organic sediments and to approximate its timing of initial deposition. 相似文献
127.
128.
Transverse Aeolian Ridges (TARs) are among the unique aeolian bedforms of Mars, which witnessed a series of investigation for the last two decades thanks to the high-resolution remote sensing data. This paper summarized the understanding with respect to distribution, morphology, sedimentology, formation hypotheses and formation time of TARs. It is suggested that TARs are a kind of aeolian bedforms with meter-scale height and decameter-scale wavelength. TARs are primarily distributed in the equator and low-latitude regions, being rare in high and mid-latitude regions, and more popular in the south hemisphere than in the north hemisphere. Higher albedo and symmetric cross-sections are the most outstanding features of TARs, being analogous to the megaripples and reversing dunes on the Earth. The grain-size distribution of TARs’ sediments is generally bimodal, with granule cover and low thermal inertia. Three formation hypotheses were proposed for TARs: Megaripple hypothesis, reversing dune hypothesis and dust induration hypothesis, with more evidences supporting the megaripple hypothesis. Similar to dunes, TARs are geologically recent morphology on Mars, but generally predate dunes, formed in the last few million years so that most TARs are indurated or lithified and are immobile. However, contemporary mobileTARs are also developed in some regions. The unique features of TARs make them the mostenigmatic aeolian bedforms of Mars. It is proposed that high-resolution information on TARs sedimentology and integrated regional surveying should be listed in the priorities of future Mars exploration with respect to TARs study. 相似文献
129.
Charles Harris 《地球表面变化过程与地形》1986,11(6):673-676
A protaius rampart up to 4.75 m high and consisting largely of angular clasts up to boulder size is described. Bulk samples contained up to 35 per cent fines by weight, compared with up to 68 per cent fines in adjacent till. Although the rampart material was clast dominated, fines filled much of the void space, in contrast with most other protalus ramparts described in the literature. 相似文献
130.