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781.
R.H.D. Townsend R.J. Ivison Ian Smail A.W. Blain D.T. Frayer 《Monthly notices of the Royal Astronomical Society》2001,328(2):L19-L22
A numerical model of the Leonid stream is developed, based on an earlier model which has been applied to the Perseid stream. The results for this model are applied to the 2001 Leonid return. By examining the full three-dimensional dispersion of individual 'streamlets' released from the Leonid parent comet, 55P/Tempel–Tuttle, we have derived an estimate for the temporal change in spatial density of each trail. Using this result along with an estimate for the location of the centres for individual streamlets and fits to previous Leonid storm profiles, we estimate that the activity from the shower will be broad and relatively strong (zenithal hourly rates perhaps in excess of 1000). In particular, streamlets from the 1766 and 1799 ejections contribute to activity peaking near 10 and 12 ut on 2001 November 18, respectively. Additional older material from 1633, 1666 and 1699, as well as more recent ejections from 1866 and 1833, contributes to a much broader secondary maximum near 17.5 ut on November 18. Comparison with other published models of predicted Leonid activity in 2001 shows general agreement in terms of timing, but the models differ significantly in terms of the relative magnitude of the activity (which other models suggest will be larger). Significant anisotropy in the impact hazard exists for satellites in the geostationary belt, with those over western longitudes most likely to be affected. Integrated fluences for the 2001 Leonid return suggest a hazard of order one magnitude greater than occurred for the 1999 Leonid storm. 相似文献
782.
783.
T J Millar 《Astronomy& Geophysics》2005,46(2):2.29-2.32
Increasing numbers of observations of deuterium ratios have revealed that all is not as it seemed in interstellar space. Tom Millar describes how fractionation theory has confirmed the importance of interstellar grains in cosmic chemistry. 相似文献
784.
The mean value concept in mono-linear regression of multi-variables and its application to trace studies in geosciences 总被引:3,自引:1,他引:3
A J T JULL 《中国科学D辑(英文版)》2007,50(12):1828-1834
The "mean value concept" in a mono-linear regression of multi-variables is clarified.Its applications to reconstruction of the past 90-year salinity of the sea surface water in Xisha Islands and to tracing the past 80 ka paleo-geomagnetic events from the Luochuan loess 10Be record are introduced in detail,which show the significance and the potential of the "mean value concept" in geoscience research. 相似文献
785.
Automatic Interpretation of Magnetic Data Using Euler Deconvolution with Nonlinear Background 总被引:1,自引:0,他引:1
Pawan Dewangan T. Ramprasad M. V. Ramana M. Desa B. Shailaja 《Pure and Applied Geophysics》2007,164(11):2359-2372
The voluminous gravity and magnetic data sets demand automatic interpretation techniques like Naudy, Euler and Werner deconvolution.
Of these techniques, the Euler deconvolution has become a popular choice because the method assumes no particular geological
model. However, the conventional approach to solving Euler equation requires tentative values of the structural index preventing
it from being fully automatic and assumes a constant background that can be easily violated if the singular points are close
to each other. We propose a possible solution to these problems by simultaneously estimating the source location, depth and
structural index assuming nonlinear background. The Euler equation is solved in a nonlinear fashion using the optimization
technique like conjugate gradient. This technique is applied to a published synthetic data set where the magnetic anomalies
were modeled for a complex assemblage of simple magnetic bodies. The results for close by singular points are superior to
those obtained by assuming linear background. We also applied the technique to a magnetic data set collected along the western
continental margin of India. The results are in agreement with the regional magnetic interpretation and the bathymetric expressions. 相似文献
786.
Abstract The structure and collapse of linear three-dimensional magnetic neutral points is studied by varying the four parameters (p, q,j|,j⊥ ) that define, in general, the linear field of a neutral point. The effect of these parameters on both the skeleton structure (i.e. the fan and spine) and the actual field line structure of the null is considered. It is found that one current component (j⊥ ) causes the skeleton structure of the null to fold up from its potential state, whereas the other current component (j |;) causes the field lines to bend. The two other parameters (p,q) determine the potential structure of the null and cause the null to transform from a three-dimensional null to a two-dimensional null and from a positive (type B) null to a negative (type A) null. To investigate the collapse of three-dimensional nulls, solutions to the linear, low-β ideal magnetohydrodynamic equations are found. It is found that three-dimensional null points can collapse if the field line foot-points are free and energy can propagate into the system. 相似文献
787.
A. N. Rublev I. A. Gorchakova T. A. Udalova 《Izvestiya Atmospheric and Oceanic Physics》2011,47(2):190-200
Based on mathematical simulation, quantitative estimates of the effect that coarse dust particles have on the accuracy of
retrieving the optical characteristics of aerosol have been obtained from the results of ground-based measurements of the
spectral fluxes of both direct and scattered solar radiations. The results of verifying a retrieval algorithm (used at the
AERONET ground-based network) based on special test models showed that the aerosol characteristics retrieved with this algorithm
are unsuitable for calculating integral solar fluxes and for simulating space spectrometric IR measurements when the concentration
of dust particles in the atmosphere exceeds their concentration in the well-known CONT model of continental aerosol by a factor
of two or more. 相似文献
788.
Crustal contamination and fluid/rock interaction in the carbonatites of Fuerteventura (Canary Islands, Spain): a C, O, H isotope study 总被引:7,自引:0,他引:7
Fuerteventura—the second largest of the Canary Islands consists of Mesozoic sediments, submarine volcanic rocks, dike swarms and plutons of the Basal Complex, and younger subaerial basaltic and trachytic series. Carbonatites are found in two Basal Complex exposures: the Betancuria Massif in the central part of the island and the Esquinzo area in the north.
values of the carbonatites increase progressively from south to north of the island. This phenomenon is attributed to different degrees of assimilation of sedimentary carbonate. Homogeneous, typically magmatic
values for carbonatites which have preserved primary igneous textures and minerals suggest a well-mixed reservoir where changes in
values result from the storage of carbonate magmas at different structural levels. The magma storage allowed assimilation of sediment to varying degrees before final emplacement of carbonatites. Shifts in
towards more positive and negative values from presumed primary compositions are observed in the carbonatites. On the basis of the oxygen isotope compositions of calcite, mica and K-feldspar, and the hydrogen isotope compositions of micas, the changes in the
values of the carbonatites can be related to fluid/rock interactions. 相似文献
789.
Stobie R. S. Ishida K. Yoshii Y. Macgillivray H. T. 《Astrophysics and Space Science》1986,118(1-2):419-420
Astrophysics and Space Science - 相似文献
790.