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151.
152.
城市增长是二十一世纪人类最大的挑战之一。根据目前的预测,全世界的城市人口每年增长大约五千万。这种增长几乎是指数式的,在本世纪中期就可能达到饱和。因此就有了很多讨论和评估,关于土地消耗、特大城市可管理的面积以及组织而非控制这种快速传播的城市化的简单方法。为此,更好地理解城市增长的空间动力学应该是一个先决条件。实际上,城市规划学、城市地理学、城市经济学以及其它的相关学科已经在这个问题上作了很大的努力。虽然它们对一些细节有了深入研究,但是没有提出蕴含在这些复杂动力学下面的总的机制的大框图。因此有理由考虑是否… 相似文献
153.
Characterization of murine non-adherent bone marrow cells leading to recovery of endogenous hematopoiesis 总被引:1,自引:1,他引:0
Stephan Fricke Christian Fricke Christopher Oelkrug Nadja Hilger Uta Sch?nfelder Manja Kamprad J?rg Lehmann Johannes Boltze Frank Emmrich Ulrich Sack 《Cellular and molecular life sciences : CMLS》2010,67(23):4095-4106
Non-adherent bone marrow-derived cells (NA-BMCs) are a mixed cell population that can give rise to multiple mesenchymal phenotypes
and that facilitates hematopoietic recovery. We characterized NA-BMCs by flow cytometry, fibroblast colony-forming units (CFU-f),
real-time PCR, and in in vivo experiments. In comparison to adherent cells, NA-BMCs expressed high levels of CD11b+ and CD90+ within the CD45+ cell fraction. CFU-f were significantly declining over the cultivation period, but NA-BMCs were still able to form CFU-f
after 5 days. Gene expression analysis of allogeneic NA-BMCs compared to bone marrow (BM) indicates that NA-BMCs contain stromal,
mesenchymal, endothelial cells and monocytes, but less osteoid, lymphoid, and erythroid cells, and hematopoietic stem cells.
Histopathological data and analysis of weight showed an excellent recovery and organ repair of lethally irradiated mice after
NA-BMC transplantation with a normal composition of the BM. 相似文献
154.
Reconstruction of gene association network reveals a transmembrane protein required for adipogenesis and targeted by PPARγ 总被引:1,自引:0,他引:1
Juliane G. Bogner-Strauss Andreas Prokesch Fatima Sanchez-Cabo Dietmar Rieder Hubert Hackl Kalina Duszka Anne Krogsdam Barbara Di Camillo Evelyn Walenta Ariane Klatzer Achim Lass Montserrat Pinent Wing-Cheong Wong Frank Eisenhaber Zlatko Trajanoski 《Cellular and molecular life sciences : CMLS》2010,67(23):4049-4064
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Stolk L Perry JR Chasman DI He C Mangino M Sulem P Barbalic M Broer L Byrne EM Ernst F Esko T Franceschini N Gudbjartsson DF Hottenga JJ Kraft P McArdle PF Porcu E Shin SY Smith AV van Wingerden S Zhai G Zhuang WV Albrecht E Alizadeh BZ Aspelund T Bandinelli S Lauc LB Beckmann JS Boban M Boerwinkle E Broekmans FJ Burri A Campbell H Chanock SJ Chen C Cornelis MC Corre T Coviello AD d'Adamo P Davies G de Faire U de Geus EJ Deary IJ Dedoussis GV Deloukas P Ebrahim S Eiriksdottir G Emilsson V 《Nature genetics》2012,44(3):260-268
To newly identify loci for age at natural menopause, we carried out a meta-analysis of 22 genome-wide association studies (GWAS) in 38,968 women of European descent, with replication in up to 14,435 women. In addition to four known loci, we identified 13 loci newly associated with age at natural menopause (at P < 5 × 10(-8)). Candidate genes located at these newly associated loci include genes implicated in DNA repair (EXO1, HELQ, UIMC1, FAM175A, FANCI, TLK1, POLG and PRIM1) and immune function (IL11, NLRP11 and PRRC2A (also known as BAT2)). Gene-set enrichment pathway analyses using the full GWAS data set identified exoDNase, NF-κB signaling and mitochondrial dysfunction as biological processes related to timing of menopause. 相似文献
157.
Bose-Einstein condensation (BEC)-the macroscopic ground-state accumulation of particles with integer spin (bosons) at low temperature and high density-has been observed in several physical systems, including cold atomic gases and solid-state quasiparticles. However, the most omnipresent Bose gas, blackbody radiation (radiation in thermal equilibrium with the cavity walls) does not show this phase transition. In such systems photons have a vanishing chemical potential, meaning that their number is not conserved when the temperature of the photon gas is varied; at low temperatures, photons disappear in the cavity walls instead of occupying the cavity ground state. Theoretical works have considered thermalization processes that conserve photon number (a prerequisite for BEC), involving Compton scattering with a gas of thermal electrons or photon-photon scattering in a nonlinear resonator configuration. Number-conserving thermalization was experimentally observed for a two-dimensional photon gas in a dye-filled optical microcavity, which acts as a 'white-wall' box. Here we report the observation of a Bose-Einstein condensate of photons in this system. The cavity mirrors provide both a confining potential and a non-vanishing effective photon mass, making the system formally equivalent to a two-dimensional gas of trapped, massive bosons. The photons thermalize to the temperature of the dye solution (room temperature) by multiple scattering with the dye molecules. Upon increasing the photon density, we observe the following BEC signatures: the photon energies have a Bose-Einstein distribution with a massively populated ground-state mode on top of a broad thermal wing; the phase transition occurs at the expected photon density and exhibits the predicted dependence on cavity geometry; and the ground-state mode emerges even for a spatially displaced pump spot. The prospects of the observed effects include studies of extremely weakly interacting low-dimensional Bose gases and new coherent ultraviolet sources. 相似文献
158.
Voyager 2 crossed the solar wind termination shock at 83.7 au in the southern hemisphere, approximately 10 au closer to the Sun than found by Voyager 1 in the north. This asymmetry could indicate an asymmetric pressure from an interstellar magnetic field, from transient-induced shock motion, or from the solar wind dynamic pressure. Here we report that the intensity of 4-5 MeV protons accelerated by the shock near Voyager 2 was three times that observed concurrently by Voyager 1, indicating differences in the shock at the two locations. (Companion papers report on the plasma, magnetic field, plasma-wave and lower energy particle observations at the shock.) Voyager 2 did not find the source of anomalous cosmic rays at the shock, suggesting that the source is elsewhere on the shock or in the heliosheath. The small intensity gradient of Galactic cosmic ray helium indicates that either the gradient is further out in the heliosheath or the local interstellar Galactic cosmic ray intensity is lower than expected. 相似文献
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