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141.
W. I. Clarkson B. Enoch C. A. Haswell A. J. Norton D. J. Christian A. Collier Cameron S. R. Kane K. D. Horne T. A. Lister R. A. Street R. G. West D. M. Wilson N. Evans A. Fitzsimmons C. Hellier S. T. Hodgkin J. Irwin F. P. Keenan J. P. Osborne N. R. Parley D. L. Pollacco R. Ryans I. Skillen P. J. Wheatley 《Monthly notices of the Royal Astronomical Society》2007,381(2):851-864
142.
A. M. S. Smith A. Collier Cameron D. J. Christian W. I. Clarkson B. Enoch A. Evans C. A. Haswell C. Hellier K. Horne J. Irwin S. R. Kane T. A. Lister A. J. Norton N. Parley D. L. Pollacco R. Ryans I. Skillen R. A. Street A. H. M. J. Triaud R. G. West P. J. Wheatley D. M. Wilson 《Monthly notices of the Royal Astronomical Society》2006,373(3):1151-1158
The evolution of the Alfvén turbulence due to three-wave interactions is discussed using kinetic theory for a collisionless, thermal plasma. There are three low-frequency modes, analogous to the three modes of compressible magnetohydrodynamics (MHD). When only Alfvén waves are considered, the known anisotropy of turbulence in incompressible MHD theory is reproduced. Inclusion of a fast mode wave leads to the separation of turbulence into two regimes: small wave numbers where three-wave processes involving a fast mode are dominant, and large wave numbers where the three Alfvén wave process is dominant. Possible application of the anisotropic Alfvén turbulence to the interstellar medium and dissipation of magnetic energy in magnetars are discussed. 相似文献
143.
Earth, Moon, and Planets - 相似文献
144.
Pollutant emissions such as aerosols and tropospheric ozone precursors substantially influence climate. While future century-scale
scenarios for these emissions have become more realistic through the inclusion of emission controls, they still potentially
lack consistency between surface pollutant concentrations and regional levels of affluence. We find that the default method
of scenario construction, whereby emissions factors converge to similar values in different regions, does not yield pollution
concentrations consistent with historical experience. We demonstrate a methodology combining use of an integrated assessment
model and a three-dimensional atmospheric chemical transport model, whereby a reference scenario is constructed by requiring
consistent surface pollutant concentrations as a function of regional income over the 21st century. By adjusting air pollutant
emission control parameters, we improve consistency between projected PM2.5 and economic income among world regions through time; consistency for ozone is also improved but is more difficult to achieve
because of the strong influence of upwind world regions. Reference case pollutant emissions described here were used to construct
the RCP4.5 Representative Concentration Pathway climate policy scenario. 相似文献
145.
遥感影像正射纠正的GPU-CPU协同处理研究 总被引:1,自引:0,他引:1
提出了一种基于CUDA的遥感影像正射纠正GPU-CPU协同处理方法,以实现重采样操作的GPU细粒度并行化。根据GPU的并行结构和硬件特点,采用执行配置优化技术提高warp占有率,利用共享存储器优化减少对效率低下的全局存储器中坐标变换系数的重复访问,通过纹理存储器代替全局存储器优化对原始影像数据的访问。实验结果表明,并行算法能够充分发挥GPU的并行处理能力,利用GeForce 9500 GT显卡,对大小为6 000像素×6 000像素的全色影像进行多项式纠正对比实验,最邻近灰度内插重采样和双线性灰度内插重采样的最终加速比分别能够达到8倍和10倍以上。 相似文献
146.
A major seismic swarm occurred near Parícutin volcano between the end of May and early July 2006. More than 700 earthquakes
with magnitude (M
L
) exceeding 2.4 were located. Parícutin, located in the Michoacán–Guanajuato volcanic field in western Mexico, is well known
as the site of the 1943 eruption in which a new 400 m cinder cone was constructed in what had been farmland. The 2006 swarm
exhibits all of the characteristics typically associated with swarms of volcanic origins. The earthquake rate showed the typical
ramp up and ramp down over the course of several days. Magnitudes were evenly distributed in time with a notably high b-value
of 2.45. The earthquake locations cluster around a northeast-striking trend extending approximately 6 km. Over the first two
weeks, hypocenters migrated steadily a few hundred meters per day, rising from 9 to 5 km depth and moving northeast about
5 km. On approximately June 7, the ascent of hypocenters stalled. For the next three weeks, hypocenters held their depth while
migrating laterally back to the southwest. Focal mechanisms during the first part of the swarm reflected the increased stress
caused by dike inflation. Following June 7, the stress orientation changed and became more consistent with the inflation of
horizontal sill-like structures. Though only limited information is available from the seismic swarm preceding the 1943 eruption,
several features, including the swarm duration and magnitude relationships, were comparable to those of the 2006 episode.
The strong indicators of a magmatic origin to the 2006 swarm suggest that at this location there are few, if any, traditional
seismic discriminants that could be used to distinguish which seismic swarms and dike emplacement events might culminate in
eruption. 相似文献
147.
This study seeks to quantify the rate and timing of regolith generation in the Critical Zone at the Susquehanna Shale Hills Critical Zone Observatory (SSHO). Meteoric 10Be depth profiles were determined using measurements from 30 hillslope soil and bedrock core samples in an effort to constrain 10Be inventories. The SSHO is located in the temperate climate zone of central Pennsylvania and comprises a first-order watershed developed entirely on a Fe-rich, organic-poor, Silurian-aged shale. Two major perturbations to the landscape have occurred at SSHO in the geologically recent past, including significant and sustained periglacial activity until after the retreat of the Laurentide ice sheet (~21 ka) and deforestation during early colonial land-use. Bulk soil samples (n = 16) were collected at three locations along a planar hillslope on the southern ridge of the catchment, representing the ridge top, mid-slope and valley floor. Rock chip samples (n = 14) were also collected from a 24 m deep core drilled into the northern ridge top. All meteoric 10Be concentration profiles show a declining trend with depth, with most of the 10Be retained in the uppermost decimeters of the soil. Meteoric 10Be inventories are higher at the mid-slope and valley floor sample sites, at 3.71 ± 0.02 × 1010 at/cm2 and 3.69 ± 0.02 × 1010 at/cm2, than at the ridge top site (1.90 ± 0.01 × 1010 at/cm2). The 10Be inventory at the convex ridge top site implies a minimum residence time of ~10.6 ka, or if erosion is steady, an erosion rate of 19.4 ± 0.2 m/My. 相似文献
148.
Niels Hovius Albert Galy Robert G. Hilton Robert Sparkes Joanne Smith Kao Shuh-Ji Chen Hongey Lin In-Tian A. Joshua West 《Applied Geochemistry》2011
Rapidly eroding, coastal mountain belts, where steep rivers and submarine channels connect upland sources to nearby marine sinks are hotspots of organic carbon transfer from life biomass, soil and exhumed bedrock into geological storage. Using observations from the Southern Alps of New Zealand, and Taiwan, we have mapped this organic pathway to geological carbon sequestration, and can evaluate the magnitude and efficiency of transfers between sources and sinks. We demonstrate that POC is harvested by landsliding, but importantly also by common and widespread surface runoff on steep hillslopes. Although terrestrially sourced POC is found in many sedimentary environments associated with mountain belts and frontier basins, it appears to be most abundantly trapped and preserved in marine turbidites. The loss of all forms of POC in onward transport through short, steep routing systems to this repository is limited. This is in marked contrast to larger routing systems, in which only the most resilient forms of POC survive into long-term deposition. 相似文献
149.
The extensive light-toned deposits in canyons and troughs in Valles Marineris provide evidence of formation through water-related processes. As such, these deposits offer a window to past conditions on Mars. We study a small outcrop of light-toned deposits in a closed trough in Coprates Catena, a chain of collapse pits to the south-east of the main Valles Marineris system. A well-exposed sequence of deposits on the base of the north wall of the trough offers a 220 m section for geochemical and morphologic analysis. Using CRISM data we identify the presence of both phyllosilicates and sulfates and/or opaline silica in the light toned deposits, which vary in relative strength with elevation. We observe a trend in the dominant mineralogical signal, with Al phyllosilicates occurring near the base of the deposits, both below and above a band of Fe/Mg phyllosilicates, before a transition to more sulfate- or opaline silica-rich material near the top of the section. This trend likely reflects a change in the chemistry of the water in which the deposits formed. Using a HiRISE Digital Elevation Model, we find that the layers in the light-toned deposits on both sides of the trough dip gently towards the center of the trough, with a dip direction that aligns with the strike of the trough, suggesting that the light-toned deposits formed after the trough. Our general morphologic and mineralogical observations fit well with significant amounts of water in the trough. The deposits are too small to be dated using crater counting techniques, however, our crater analysis suggests that the plains in which the trough formed are probably Late Hesperian in age. If the chemistry of the light-toned deposits reflects the primary depositional mineralogy, then this and other small troughs in Coprates Catena might provide evidence of limited phyllosilicate formation in this region towards the end of the Hesperian era on Mars. 相似文献
150.
We examine an eruptive sequence in late 2007 at Bezymianny Volcano to characterize the magmatic plumbing system and eruption-related seismicity. Earthquake locations reveal seismicity below and offset to the north of the volcano along a tectonic fault. Based on historical seismicity, the magma chamber is postulated to have a top at about 6 km depth. Minor dome explosions, large sub-plinian eruptions and dome collapses are analyzed using an automated event classification scheme. Low-frequency tremor, interpreted as gas escape, and low-frequency earthquakes are a dominant proportion of the energy released. We also examine multiplet earthquakes whose behavior during the study period changed significantly and systematically before the largest eruption, demonstrating the potential of tracking multiplets to assess changing conditions with the conduit. 相似文献