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101.
Elena Lega Massimiliano Guzzo Claude Froeschlé 《Celestial Mechanics and Dynamical Astronomy》2010,107(1-2):129-144
Using a three degrees of freedom quasi-integrable Hamiltonian as a model problem, we numerically compute the unstable manifolds of the hyperbolic manifolds of the phase space related to single resonances. We measure an exponential dependence of the splitting of these manifolds through many orders of magnitude of the perturbing parameter. This is an indirect numerical verification of the exponential decay of the normal form, as predicted by the Nekhoroshev theorem. We also detect different transitions in the topology of these manifolds related to the local rational approximations of the frequencies. The variation of the size of the homoclinic tangle as well as the topological transitions turn out to be correlated to the speed of Arnold diffusion. 相似文献
102.
103.
In this contribution we present our preliminary investigation on pulsar sensitivity of the Large Area Telescope, the main
instrument aboard the GLAST mission. In particular we concentrated our attention to pulsars located at low galactic latitudes.
We created a set of simulated pulsars having different fluxes in an array of galactic coordinates separated by a distance
greater than the LAT Point Spread Function in order to avoid confusion between adjacent sources. Galactic gamma-ray sky background
as used during the second LAT Data Challenge (DC2) is also included. We then run an automatic routine for testing periodicity for all the pulsars considering an opportune
timing solution. In this way we can obtain a map of the sensitivity of the periodic searches for different fluxes and for
various Galactic latitudes. Some assumptions have been made by simulating the pulsar sources, but this study is a first step
toward an estimate for pulsed emission sensitivity of the GLAST LAT. The pulsed flux sensitivity profile we generate could
also be input to a population synthesis code of Galactic pulsars in order to obtain more accurate predictions of the number
of expected pulsar detections by GLAST.
On behalf of the GLAST LAT Collaboration. 相似文献
104.
Alessandro Morbidelli Massimiliano Guzzo 《Celestial Mechanics and Dynamical Astronomy》1996,65(1-2):107-136
The present paper reviews the Nekhoroshev theorem from the point of view of physicists and astronomers. We point out that Nekhoroshev result is strictly connected with the existence of a specific structure of the phase space, the existence of which can be checked with several numerical tools. This is true also for a degenerate system such as the one describing the motion of an asteroid in the so called main belt. The main difference is that in some parts of the belt, the Nekhoroshev result cannot apply a priori. Mean motion resonances of order smaller than the logarithm of the mass of Jupiter and first order secular resonances must be excluded. In the remaining parts, conversely, the Nekhoroshev theorem can be proved, provided someparameters, such as the masses, the eccentricities and the inclinations of the planets are small enough. At the light of this result, a massive campaign of numerical integrations of real and fictitious asteroids should allow to understand which is the real dynamical structure of the asteroid belt. 相似文献
105.
Projection, or conjugate gradient like, methods are becoming increasingly popular for the efficient solution of large sparse sets of unsymmetric indefinite equations arising from the numerical integration of (initial) boundary value problems. One such problem is soil consolidation coupling a flow and a structural model, typically solved by finite elements (FE) in space and a marching scheme in time (e.g. the Crank–Nicolson scheme). The attraction of a projection method stems from a number of factors, including the ease of implementation, the requirement of limited core memory and the low computational cost if a cheap and effective matrix preconditioner is available. In the present paper, biconjugate gradient stabilized (Bi‐ CGSTAB) is used to solve FE consolidation equations in 2‐D and 3‐D settings with variable time integration steps. Three different nodal orderings are selected along with the preconditioner ILUT based on incomplete triangular factorization and variable fill‐in. The overall cost of the solver is made up of the preconditioning cost plus the cost to converge which is in turn related to the number of iterations and the elementary operations required by each iteration. The results show that nodal ordering affects the perfor mance of Bi‐CGSTAB. For normally conditioned consolidation problems Bi‐CGSTAB with the best ILUT preconditioner may converge in a number of iterations up to two order of magnitude smaller than the size of the FE model and proves an accurate, cost‐effective and robust alternative to direct methods. Copyright © 2001 John Wiley & Sons, Ltd. 相似文献
106.
107.
Alessandro Ielpi Mathieu G.A. Lapôtre Alvise Finotello Massimiliano Ghinassi 《地球表面变化过程与地形》2021,46(2):357-370
River bends occasionally meander to the point of cutoff, whereby a river shortcuts itself and isolates a portion of its course. This fundamental process fingerprints a river's long-term planform geometry, its stratigraphic record, and biogeochemical fluxes in the floodplain. Although meander cutoffs are common in fast-migrating channels, timelapse imagery of the Earth surface typically does not offer a long enough baseline for statistically robust analyses of these processes. We seek to bridge this gap by quantifying cutoff kinematics along the Humboldt River (Nevada) – a stream that, from 1994 to 2019, hosted an exceptionally high number of cutoffs (specifically, 174 of the chute type and 53 of the neck type). A coincidence between major floods and cutoff incidence is first suggestive of hydrographic modulation. Moreover, not just higher sinuosity but also upstream planform skewness is associated with higher cutoff incidence and channel widening for a sub-population of chute cutoffs. We propose a conceptual model to explain our results in terms of channel-flow structure and then examine the distances between adjacent cutoffs to understand the mechanisms governing their clustering. We find that both local and nonlocal perturbations together trigger the clustering of new cutoffs, over distances capped by the backwater length and over yearly to decadal timescales. Our research suggests that planform geometry and backwater controls might sway the occurrence of cutoff clusters – both local and nonlocal – thereby offering new testable hypotheses to explore the evolution of meandering-river landscapes that have significant implications for river engineering and stratigraphic modelling. © 2020 John Wiley & Sons, Ltd. 相似文献
108.
为识别四川盆地丁山区龙马溪—五峰组目的层富含页岩气的"甜点区",本文对页岩的有机碳含量、脆性、孔隙度及微裂隙等核心指标进行分析研究.对页岩展开岩石物性特征和岩石物理分析,结果显示"甜点区"具有TOC含量高、高孔隙度、低密度、脆性高(石英含量高)的特点,此外储层的拉梅常数和密度的乘积λρ分布范围是18~30 GPa·g·cm-3,泊松比v范围是0.18~0.22,剪切模量μ范围是13~18 GPa.根据储层的岩石物理特征,同时考虑孔隙度、裂隙纵横比和矿物组分对优质页岩敏感弹性参数的影响,采用等效嵌入体应力平均(EIAS)理论模型构建适合页岩气储层的三维岩石物理模板,进而预测储层的孔隙度、裂隙纵横比和石英矿物含量.基于测井数据,对构建的三维岩石物理模板进行校正,将校正后的模板应用到研究工区,选取过三口井的二维测线和三维区块,进行孔隙度、裂隙纵横比和石英矿物含量的定量预测.对比实际资料分析得出的优质页岩储层孔隙度预测范围与测井结果吻合较好,过三口井的目的层产气情况与预测结果一致性良好,目的层页岩具有高孔隙度、低裂隙纵横比和高石英含量的特征,可有效地指示优质页岩储层分布. 相似文献
109.
Andrea D'Aniello Sigrún Tómasdóttir Bergur Sigfússon Massimiliano Fabbricino 《Ground water》2021,59(5):677-693
Particular attention is paid to the risk of carbon dioxide (CO2) leakage in geologic carbon sequestration (GCS) operations, as it might lead to the failure of sequestration efforts and to the contamination of underground sources of drinking water. As carbon dioxide would eventually reach shallower formations under its gaseous state, understanding its multiphase flow behavior is essential. To this aim, a hypothetical gaseous leak of carbon dioxide resulting from a well integrity failure of the GCS system in operation at Hellisheiði (CarbFix2) is here modeled. Simulations show that migration of gaseous carbon dioxide is largely affected by formation stratigraphy, intrinsic permeability, and retention properties, whereas the initial groundwater hydraulic gradient (0.0284) has practically no effect. In two different scenarios, about 18.3 and 30.6% of the CO2 that would have been injected by the GCS system for 3 days could be potentially released again into the atmosphere due to a sustained leakage of the same duration. As the gaseous leak occurs, the aquifer experiences high pressure buildups, and the presence of a less conductive layer further magnifies these. Strikingly, the dimensional analysis showed that buoyant and viscous forces can be comparable over time within the predicted gaseous plumes, even far from the leakage source. Local pressure gradients, buoyant, viscous, and capillary forces all play an important role during leakage. Therefore, neglecting one or more of these contributions might lead to a partial prediction of gaseous CO2 flow behavior in the subsurface, giving space to incorrect interpretations and wrong operational choices. 相似文献
110.
Ray A. F. Cas Heather M. N. Wright Christopher B. Folkes Chiara Lesti Massimiliano Porreca Guido Giordano Jose G. Viramonte 《Bulletin of Volcanology》2011,73(10):1583-1609
The 2.08-Ma Cerro Galán Ignimbrite (CGI) represents a >630-km3 dense rock equivalent (VEI 8) eruption from the long-lived Cerro Galán magma system (∼6 Ma). It is a crystal-rich (35–60%),
pumice (<10% generally) and lithic-poor (<5% generally) rhyodacitic ignimbrite, lacking a preceding plinian fallout deposit.
The CGI is preserved up to 80 km from the structural margins of the caldera, but almost certainly was deposited up to 100 km
from the caldera in some places. Only one emplacement unit is preserved in proximal to medial settings and in most distal
settings, suggesting constant flow conditions, but where the pyroclastic flow moved into a palaeotopography of substantial
valleys and ridges, it interacted with valley walls, resulting in flow instabilities that generated multiple depositional
units, often separated by pyroclastic surge deposits. The CGI preserves a widespread sub-horizontal fabric, defined by aligned
elongate pumice and lithic clasts, and minerals (e.g. biotite). A sub-horizontal anisotropy of magnetic susceptibility fabric
is defined by minute magnetic minerals in all localities where it has been analysed. The CGI is poor in both vent-derived
(‘accessory’) lithics and locally derived lithics from the ground surface (‘accidental’) lithics. Locally derived lithics
are small (<20 cm) and were not transported far from source points. All data suggest that the pyroclastic flow system producing
the CGI was characterised throughout by high sedimentation rates, resulting from high particle concentration and suppressed
turbulence at the depositional boundary layer, despite being a low aspect ratio ignimbrite. Based on these features, we question
whether high velocity and momentum are necessary to account for extensive flow mobility. It is proposed that the CGI was deposited
by a pyroclastic flow system that developed a substantial, high particle concentration granular under-flow, which flowed with
suppressed turbulence. High particle concentration and fine-ash content hindered gas loss and maintained flow mobility. In
order to explain the contemporaneous maintenance of high particle concentration, high sedimentation rate at the depositional
boundary layer and a high level of mobility, it is also proposed that the flow(s) was continuously supplied at a high mass
feeding rate. It is also proposed that internal gas pressure within the flow, directed downwards onto the substrate over which
the flow was passing, reduced the friction between the flow and the substrate and also enhanced its mobility. The pervasive
sub-horizontal fabric of aligned pumice, lithic and even biotite crystals indicates a consistent horizontal shear force existed
during transport and deposition in the basal granular flow, consistent with the existence of a laminar, shearing, granular
flow regime during the final stages of transport and deposition. 相似文献