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地球主磁场B和它的长期变化都起源于地球外核的磁流体发电机过程，但是，它们的空间结构和时间演化特征却有很大差异. 本文采用全球平均的“无符号年变率”X〖DD(-*3〗〖KG*2/3〗·〖DD)〗〖DD(-*2〗〖KG*2/3〗—〖DD)〗、Y〖DD(-*3〗〖KG*2/3〗·〖DD)〗〖DD(-*2〗〖KG*2/3〗—〖DD)〗、Z〖DD(-*3〗〖KG*2/3〗·〖DD)〗〖DD(-*2〗〖KG*2/3〗—〖DD)〗、H〖DD(-*3〗〖KG*2/3〗·〖DD)〗〖DD(-*2〗〖KG*2/3〗—〖DD)〗和F〖DD(-*3〗〖KG*2/3〗·〖DD)〗〖DD(-*2〗〖KG*2/3〗—〖DD)〗来表征长期变化场〖WTHX〗〖AKB·〗〖WTBZ〗的总体强度，利用第9代国际参考地磁场模型IGRF 9，研究〖WTHX〗〖AKB·〗场的变化特征. 结果表明，在1900～2000年的100年当中，〖AKB·〗场经历了3幕变化，最大年变率分别发生在1910～1920、1940～1950、1970～1980年，显示出清晰的30年周期变化，而且，每一周期的上升段比其下降段短得多. 研究结果还表明，非偶极场对〖AKB·〗的贡献约为偶极场的2倍，因此，决定〖AKB·〗场周期特征的主要因素是非偶极场（特别是四极子场），而不是偶极子场. 这一特点与主磁场B〖WTBZ〗中偶极场占绝对优势的特点完全不同. 相似文献
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A subducting oceanic lithospheric slab acts as an efficient heat sink which strongly influences the convection pattern in the neighbouring sub-continental mantle. Laboratory convection experiments show that this thermal coupling induces a roll about 5 times broader than deep underneath the continental lithosphere. The experiments are performed in a tank with imposed top and bottom temperature, and with, in addition, one cooled side wall. The convective pattern is observed by differential interferometry. For upper mantle convection one predicts rolls extending 3000 to 4000 km into the continental domain, parallel to the active margin. We show that, for Gondwana prior to the break-up, this simple convection pattern can explain the tensional state of the crust leading to the emission of flood basalts (Karroo, Parana and Antarctica). The thermal and mechanical effect of the large roll also provides a mechanism for the break-up itself and subsequent drift of the continental fragments. This motion of the continental plate leads finally to the closure of existing marginal basins along the Pacific coast of Gondwana. The laboratory experiments throw some light into another phenomenon of possible geodynamical relevance: within the large convection roll a smaller scale circulation is observed in the form of diapiric upwelling produced by thermal instabilities in the boundary layer. This dynamics may apply to hot spot volcanicity.
Zusammenfassung Die subduzierte ozeanische Lithosphäre beeinflußt die Konvektion unterhalb der kontinentalen Lithosphäre, weil sie die Rolle einer Wärmepumpe spielt. Experimentelle Versuche zeigen, daß diese thermische Kopplung flache Konvektionsrollen im kontinentalen Mantel erzeugt, mit horizontalen Dimensionen zwischen 3000 und 4000 km. Diese flachen Zellen werden als Ursache der Dehnungstektonik in Gondwana vorgeschlagen (Karroo, Parana, Antarktika). Ihre thermische und mechanische Wirkung führt letztlich zum Zerbrechen des Superkontinents. Die Versuche im Laboratorium zeigen auch Instabilitäten kleinerer Dimensionen, welche thermische Diapire erzeugen, ähnlich den sogenannten hot spots.
Résumé La lithosphere océanique en subduction constitue un puits de chaleur qui influence la convection dans le manteau sous-continental voisin. Des expériences de laboratoire montrent que ce refroidissement latéral crèe des rouleaux convectifs sous la lithosphere continentale de 3000 à 4000 km d'extension horizontale pour une convection limitée au manteau supérieur. Appliqué au Gondwana, ceci explique la tectonique en extension accompagnée d'épanchements basaltiques (Karroo, Parana, Antarctique) précédant l'ouverture Atlantique et Indienne. Cette ouverture est elle-même provoquée par l'action thermique et mécanique des grands rouleaux convectifs. Les expériences de laboratoire font également apparaître des instabilités à petite échelle, semblables aux diapirs que l'on pense être à l'origine du volcanisme intraplaque.
, .. . , 3000 4000 , (Karoo, , ). . , , .. (Hot spots) .相似文献
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Frank M. Richter Stephen F. Daly Henri-Claude Nataf 《Earth and Planetary Science Letters》1982,60(2):178-194
Laboratory experiments are used to illustrate how steady convective flows, while efficient at stirring an initial heterogeneity within a single cell, do not produce dispersal of heterogeneous material over scales large compared to the depth. Long-range dispersal requires that the flow be time dependent on a time scale comparable to the overturn time. Convection in an internally heated layer has this property and numerical solutions are used to study the way in which it disperses a set of neutrally buoyant particles that were initially confined to a small space. The horizontal dispersal of these particles is reasonably well represented by an effective diffusivity of 0.3 cm2/s for a Rayleigh number of 106. The concept of an effective diffusivity is then applied to the isotopic evolution of the Sm-Nd and Rb-Sr systems with spatial variations generated by horizontal variations in degree of melting 1.8×109 years ago. The present-day average ε value one would measure in such a system depends on the average degree of melting, the amplitude and length scale of variations in partial melt, and the effective diffusivity assumed. Especially in the case of Nd the differences in average ε value between a uniform and a spatially variable (but with the same average) melting case can be significant. The range of ε values about the average is controlled by the competing effects of generation by the differences in enrichment factor and decay due to the effective diffusivity. 相似文献
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