Proper elements for highly inclined asteroidal orbits     

Anne Lemaitre  Alessandro Morbidelli 《Celestial Mechanics and Dynamical Astronomy》1994,60(1):29-56

Based on Williams' work and rewritten in action angle variables, a method for the calculation of proper elements is here presented. The averaging over the long periodic terms is performed by the semi numerical method developed by Henrard (1990); no series expansion in eccentricity or inclination of the asteroid is used which allows calculating proper elements for highly inclined orbits. Conversely, the theory is truncated at the first degree in the eccentricity and the inclination of the perturbing planets. A few tests about accuracy and consistency are presented.  相似文献   

Volume and surface sources due to laterally varying boundaries of elastic homogeneous layers     

Georges Jobert  Anne Suteau 《Geophysical Journal International》1978,55(3):669-677

Summary. Various methods have been applied to solve propagation problems in media composed of homogeneous layers, the boundaries of which have slight lateral variations. In this paper, volume sources, introduced in a previous paper to describe the effects of lateral irregularities, are replaced by an equivalent body force and by surface sources concentrated on the irregular boundaries. The surface sources we find are similar to those obtained by Kennett for a two-dimensional structure and we generalize his results to a three-dimensional structure and to the case when an external body force is present.  相似文献   

Upcoming International Events     

Anne Marie de Grosbois 《Environmental Geology》2008,56(3-4):803-808

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A physical mechanism for the Atlantic–Pacific flow reversal in the early Miocene     

Anne Willem Omta  Henk A. Dijkstra   《Global and Planetary Change》2003,36(4):265

Barotropic wind-driven steady ocean circulation patterns have been calculated for several different continental geometries during the Tertiary. Using a shallow-water model, flows are computed at 5-Ma intervals within the 60–20 Ma period, while keeping a fixed pattern of the wind-stress forcing. The most interesting changes in ocean circulation occur between 35 and 20 Ma, in which (i) the Antarctic Circumpolar Current appears because of the widening of Drake Passage, (ii) the Tethys Current disappears because of the closure of the Tethys Seaway and (iii) the transport through Panama Straits (between North and South America) reverses. The results are qualitatively in agreement with interpretations of changes in ocean surface currents drawn on the basis of proxy studies. A physical mechanism of the flow reversal through the Panama Straits is proposed based on a detailed analysis of the changes in wind-driven transport of both the Tethys Current and the Antarctic Circumpolar Current.  相似文献   

A perturbation method for problems with two critical arguments     

Jacques Henrard  Anne Lemaitre 《Celestial Mechanics and Dynamical Astronomy》1986,39(3):213-238

We develop a semi-numerical perturbation method for problems with two critical arguments. We apply it to a truncated model of the restricted, elliptic three body problem in case of a resonance 2/1 We identify regions of the phase space where chaotic motion is expected because of the presence of homoclinic orbits. One of these regions, the largest one, sits at the entrance to the resonance zone and is associated with a 2/1 resonance between the two critical arguments. The results are compared with numerical results due to Murray (1986)  相似文献   

Introduction     

Anne Buttimer 《GeoJournal》1992,26(2):100-102

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Magmatic infiltration and melting in the lower crust and upper mantle beneath the Cima volcanic field,California     

H. G. Wilshire  Anne V. McGuire 《Contributions to Mineralogy and Petrology》1996,123(4):358-374

 Xenoliths of lower crustal and upper mantle rocks from the Cima volcanic field (CVF) commonly contain glass pockets, veins, and planar trains of glass and/or fluid inclusions in primary minerals. Glass pockets occupy spaces formerly occupied by primary minerals of the host rocks, but there is a general lack of correspondence between the composition of the glass and that of the replaced primary minerals. The melting is considered to have been induced by infiltration of basaltic magma and differentiates of basaltic magma from complex conduits formed by hydraulic fracturing of the mantle and crustal rocks, and to have occurred during the episode of CVF magmatism between ∼7.5 Ma and present. Variable compositions of quenched melts resulted from mixing of introduced melts and products of melting of primary minerals, reaction with primary minerals, partial crystallization, and fractionation resulting from melt and volatile expulsion upon entrainment of the xenoliths. High silica melts ( >∼60% SiO₂) may result by mixing introduced melts with siliceous melts produced by reaction of orthopyroxene. Other quenched melt compositions range from those comparable to the host basalts to those with intermediate Si compositions and elevated Al, alkalis, Ti, P, and S; groundmass compositions of CVF basalts are consistent with infiltration of fractionates of those basalts, but near-solidus melting may also contribute to formation of glass with intermediate silica contents with infiltration only of volatile constituents. Received: 15 June 1995 / Accepted: 13 December 1995  相似文献   

Influence of Late-Holocene Climate on Northern Rocky Mountain Mammals     

Elizabeth Anne Hadly 《Quaternary Research》1996,46(3):298-310

An exceptionally rich paleontological site containing thousands of mammalian fossils and well-dated with 18 radiocarbon samples provides evidence of late-Holocene ecological response to climatic change in northern Yellowstone National Park, Wyoming. The mammalian fauna, composed of 10,597 identified specimens, shows surprising affinity to the local habitat with little evidence of long-distance transport of faunal elements, thus revealing the faithfulness of a fossil site to the community from which it is derived. The mammals illustrate ecological sensitivity to a series of mesic to xeric climatic excursions in the sagebrush-grassland ecotone during the past 3200 yr. From 3200 cal yr B.P. to a maximum of 1100 cal yr B.P., the species composition of mammals indicates wetter conditions than today. Beginning about 1200 cal yr B.P., the fauna becomes more representative of xeric conditions with maxima in xeric-indicator taxa and minima in mesic-indicator taxa, concordant with the Medieval Warm Period (circa 1000 to 650 yr B.P.). Cooler, wetter conditions which prevailed for most of the Little Ice Age (700 to 100 yr B.P.) in general correspond to a return to a more mesic mammalian fauna. A warm period within the Little Ice Age is documented by a xeric fauna. These data show that mammalian ecological sensitivity to climatic change over this intermediate time scale holds promise for predictions about the impacts of future global warming.  相似文献   

Author index for volume 43     

André Marten  Régis Courtin  Daniel Gautier  Anne Lacombe 《Icarus》1980,43(3):410-422

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Segmentation of the Central Indian Ridge between 12°12′ S and the Indian Ocean Triple Junction     

Lindsay M. Parson  Philippe Patriat  Roger C. Searle  Anne R. Briais 《Marine Geophysical Researches》1993,15(4):265-282

The present morphology and tectonic evolution of more than 1500 kilometres of the Central Indian Ridge are described and discussed following the integration of GLORIA side-scan sonographs with conventional geophysical datasets. Segmentation of the ridge occurs by a series of ridge axis discontinuities ranging in periodicity along strike from 275 km to less than 30 km. These segment boundaries we have classified into two types: first order fracture zones of offsets greater than 50 km which bound five major (mega-) segments, and smaller scale structures of a variety of offset styles and amplitudes which cut four of these segments. We refer to these as ridge-axis discontinuities. The frequent opposite sense of offset identified between the first order structures and the subordinate discontinuities between these major structures is interpreted as resulting from the adjustment to new kinematic parameters after magnetic anomaly 20. As far as our data allows us to determine, the central major segment is not subdivided by minor ridge axis discontinuities, which we suggest is a result of its proximity to the Rodriguez hotspot.  相似文献