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71.
Marek J. Sarna Sinan K. Yerli & Alexander G. Muslimov 《Monthly notices of the Royal Astronomical Society》1998,297(3):760-768
We examine the possibility of probing dynamo action in mass-losing stars, components of Algol-type binaries. Our analysis is based on the calculation of non-conservative evolution of these systems. We model the systems U Sge and β Per where the more massive companion fills its Roche lobe at the main sequence (case AB) and where it has a small helium core (early case B) respectively. We show that to maintain evolution of these systems at the late stages which are presumably driven by stellar 'magnetic braking', an efficient mechanism for producing large-scale surface magnetic fields in the donor star is needed. We discuss the relevance of dynamo operation in the donor star to the accelerated mass transfer during the late stages of evolution of Algol-type binaries. We suggest that the observed X-ray activity in Algol-type systems may be a good indicator of their evolutionary status and internal structure of the mass-losing stellar components. 相似文献
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Marek Kacewicz 《Mathematical Geology》1994,26(8):985-994
The feedforward backpropagation technique provides a model-free estimation with neural networks. The algorithm was used to estimate fracture aperture of natural fractures in three dimensional space. A three-layer neural network with at least 5 nodes in a hidden layer was trained on a data set consisting of formation imaging microscanner logs (FMS)from horizontal boreholes. Sensitivity studies were performed to account for the rate of learning convergence, convergence to local error minima, etc. Among the factors contributing mostly to the overall good or bad performance of the network, the following are worth mentioning: number of data points, data spacing, and data variability. It is shown that a smoothing operation applied to aperture data along the wellbore often helps to reduce disorientation of the network and to switch from oscillations or chaotic jumps to convergence. 相似文献
75.
This paper describes a low earth orbiter micro-satellite attitude determination algorithm using GPS phase and pseudorange
data as the only observables. It is designed to run in real-time, at a rate of 10 Hz, on-board the spacecraft, using minimal
chip and memory resources. The spacecraft design includes four GPS antennas deployed on boom arms to improve the antenna separations.
The boom arms feature smart sensors, from which time-varying deformation data are used to calculate changes in the body-fixed
system (BFS) co-ordinates of the attitude antennas. These data are used as input to the attitude algorithm to improve the
accuracy of the output.
The conventional double-difference phase observation equations have been re-arranged so that the only unknown parameters in
the functions (once the ambiguities have been determined) are the spacecraft Euler angles. This greatly increases the redundancy
in the mathematical model, and is exploited to enhance the algorithm's ability to trap observations contaminated by unmodelled
multipath. This approach has been shown to be successful in identifying phase outliers at the 5–10 mm level. Speed of execution
of the program is improved by utilising numerical differentiation of the model equations in the linearisation process. Furthermore,
as the number of solve-for parameters is reduced to three by the chosen mathematical model, matrix inversion requirements
are minimised. A novel approach to ambiguity resolution and determination of initial estimates of the attitude parameters
has been developed utilising a heuristic technique and the known, and time varying, BFS co-ordinates of the antenna array.
Algorithm testing is based on a simulation of the micro-satellite trajectory combined with variations in attitude derived
from spin-stabilisation and periodic roll and pitch parameters. The trajectory of the spacecraft centre of mass was calculated
by numerical integration of a force model using Earth gravity field parameters, third body effects due to the Sun and the
Moon, dynamic Earth tide effects (solar and lunar), and a solar radiation pressure model. Frame transformations between J2000
and ITRF97 used the IERS conventions. A similar approach was used to calculate the trajectories of all available GPS satellites
during the same period, using initial conditions of position and velocity from IGS precise orbits. RMS differences between
the published precise orbit and the integrated satellite positions were at the 5-mm level. Phase observables are derived from
these trajectories, biased by simulation of receiver and satellite clock errors, cycle slips, random or systematic noise and
initial integer ambiguities. In the actual simulation of the attitude determination process in orbit, GPS satellite positions
are calculated using broadcast ephemerides.
The results show that the aim of 0.05° (two sigma) attitude precision can be met provided that the phase noise can be reduced
to the level of 1–2 mm. Attitude precision was found to vary strongly with constellation geometry, which can change quite
rapidly depending on the variations in spacecraft attitude. The redundancy in the mathematical model was found to be very
effective in trapping and isolating cycle slips to the double difference observations that are contaminated. This allows for
the possibility of correcting for cycle slips without full recourse to the ambiguity resolution algorithm.
Electronic Publication 相似文献
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The Sudetes Mountains (Central Europe) were under a particularly intense long-term air pollution load during the 1970s and 1980s. Intense industrial activity in this area led to large-scale forest dieback and reductions in tree growth rates, potentially limiting the use of tree-ring data from this region in dendroclimatic research. In this paper, ring-width chronologies were constructed for 493 Norway spruce trees (Picea abies L. Karst.) from 17 sampling sites within five major mountain ranges in the Sudetes Mountains of Poland. Growth-climate response data indicate that April?July temperatures are the main factor affecting radial growth of trees in the study area. Our data also indicate the strong influence of slope aspect on temperature signal strength. The lowest correlation values were obtained for sites located on western slopes with effective fog deposition, which are strongly affected by pollution. An appropriate sampling strategy resulted in the creation of a temperature-sensitive proxy record (rAMJJ = 0.70), exceptional for areas under strong pressure from human activity. Based on a regional master chronology, growing season (April?July) temperatures over the past 200 years were then reconstructed. Four warm and four cold periods were distinguished and compared with other reconstructions and long-term instrumental data. 相似文献
78.
Jing-Zhao Qi Shuo Cao Marek Biesiada Teng-Peng Xu Yan Wu Si-Xuan Zhang Zong-Hong Zhu 《天文和天体物理学研究(英文版)》2018,(6)
In this paper, we propose a new parametrization for Om(z) diagnostics and show how the most recent and significantly improved observations concerning the H(z) and SN Ia measurements can be used to probe the consistency or tension between the ΛCDM model and observations. Our results demonstrate that H0 plays a very important role in the consistency test of ΛCDM with H(z)data. Adopting the Hubble constant priors from Planck 2013 and Riess, one finds considerable tension between the current H(z) data and ΛCDM model and confirms the conclusions obtained previously by others. However, with the Hubble constant prior taken from WMAP9, the discrepancy between H(z) data and ΛCDM disappears, i.e., the current H(z) observations still support the cosmological constant scenario. This conclusion is also supported by the results derived from the Joint Lightcurve Analysis(JLA) SN Ia sample. The best-fit Hubble constant from the combination of H(z)+JLA(H00 = 68.81+1.5-1.49 km s-1 Mpc-1) is very consistent with results derived both by Planck 2013 and WMAP9, but is significantly different from the recent local measurement by Riess. 相似文献
79.
Concentrated, ‘pulsed’ axial glacier flow: structural glaciological evidence from Kvíárjökull in SE Iceland 下载免费PDF全文
Emrys Phillips Jez Everest David J.A. Evans Andrew Finlayson Marek Ewertowski Ailsa Guild Lee Jones 《地球表面变化过程与地形》2017,42(13):1901-1922
A detailed structural glaciological study carried out on Kvíárjökull in SE Iceland reveals that recent flow within this maritime glacier is concentrated within a narrow corridor located along its central axis. This active corridor is responsible for feeding ice from the accumulation zone on the south‐eastern side of Öræfajökull to the lower reaches of the glacier and resulted in a c. 200 m advance during the winter of 2013–2014 and the formation of a push‐moraine. The corridor comprises a series of lobes linked by a laterally continuous zone of highly fractured ice characterised by prominent flow‐parallel crevasses, separated by shear zones. The lobes form highly crevassed topographic highs on the glacier surface and occur immediately down‐ice of marked constrictions caused by prominent bedrock outcrops located on the northern side of the glacier. Close to the frontal margin of Kvíárjökull, the southern side of the glacier is relatively smooth and pock‐marked by a number of large moulins. The boundary between this slow moving ice and the active corridor is marked by a number of ice flow‐parallel strike‐slip faults and a prominent dextral shear zone which resulted in the clockwise rotation and dissection of an ice‐cored esker exposed on the glacier surface. It is suggested that this concentrated style of glacier flow identified within Kvíárjökull has affinities with the individual flow units which operate within pulsing or surging glaciers. © 2017 The Authors Earth Surface Processes and Landforms © 2017 John Wiley & Sons, Ltd. 相似文献
80.
Acta Geotechnica - The paper examines three-dimensional (3D) analyses of the load bearing capacity of square and strip footings on a spatially variable cohesive–frictional (c–φ)... 相似文献