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溶液中的金属离子对方解石的生长和溶解均有影响,但关于方解石中固有的杂质离子对其溶解的影响还了解甚少.本研究利用原位原子力显微镜(AFM)考察了室温下方解石(10(-1)4)晶面在含Mn2+及含Cd2+溶液中的生长过程,并对其新生长面直接进行原位溶解观察.实验表明,溶液中的Mn2+和Cd2+可参与方解石的生长,分别形成(Ca,Mn)CO3固溶体和(Ca,Cd)CO3固溶体.新生成的含Mn、Cd方解石的溶解速率仅为纯方解石的14.3%~60.3%,说明晶体中的Mn和Cd可抑制方解石的溶解.因此方解石生长阶段可通过在(10(-1)4)晶面形成含重金属固溶体从而固定Mn和Cd,由于新生长的固溶体溶解速率小于纯方解石,从而延缓Mn和Cd的迁移,并降低其环境污染的风险. 相似文献
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本文根据灾害威胁的范围不同,提出了自然灾害与技术灾害在不同的社会时期和不同性质的国家的分布与造成的影响不同的观点,进而从灾害研究的历史中分析自然灾害与技术灾害的内在联系以及人们对灾害研究的观念与方法的历史变革。在上述基础上,重点阐述了灾害评估的基本概念、灾害评估的内容和程序以及灾害管理的过程与方法。 相似文献
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Korzennik SG Brown TM Fischer DA Nisenson P Noyes RW 《The Astrophysical journal》2000,534(2):L147-L150
We present deep Hubble Space Telescope (HST) imaging, as well as ground-based imaging and spectroscopy, of the optical afterglow associated with the long-duration gamma-ray burst GRB 990712 and its host galaxy. The data were obtained 48-123 days after the burst occurred. The magnitudes of the host (R=21.9, V=22.5) and optical afterglow (R=25.4, V=25.8, 47.7 days after the burst) favor a scenario in which the optical light follows a pure power-law decay with an index of alpha approximately -1.0. We find no evidence for a contribution from a supernova like SN 1998bw. This suggests that either there are multiple classes of long-duration gamma-ray bursts or that the peak luminosity of the supernova was more than 1.5 mag fainter than SN 1998bw. The HST images and EFOSC2 spectra indicate that the gamma-ray burst was located in a bright, extended feature (possibly a star-forming region) 1.4 kpc from the nucleus of a 0.2L*B galaxy at z=0.434, possibly a Seyfert 2 galaxy. The late-time afterglow and host galaxy of GRB 990712 bear some resemblance to those of GRB 970508. 相似文献
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Krahn MM Hanson MB Baird RW Boyer RH Burrows DG Emmons CK Ford JK Jones LL Noren DP Ross PS Schorr GS Collier TK 《Marine pollution bulletin》2007,54(12):1903-1911
“Southern Resident” killer whales include three “pods” (J, K and L) that reside primarily in Puget Sound/Georgia Basin during the spring, summer and fall. This population was listed as “endangered” in the US and Canada following a 20% decline between 1996 and 2001. The current study, using blubber/epidermis biopsy samples, contributes contemporary information about potential factors (i.e., levels of pollutants or changes in diet) that could adversely affect Southern Residents. Carbon and nitrogen stable isotopes indicated J- and L-pod consumed prey from similar trophic levels in 2004/2006 and also showed no evidence for a large shift in the trophic level of prey consumed by L-pod between 1996 and 2004/2006. ∑PCBs decreased for Southern Residents biopsied in 2004/2006 compared to 1993–1995. Surprisingly, however, a three-year-old male whale (J39) had the highest concentrations of ∑PBDEs, ∑HCHs and HCB. POP ratio differences between J- and L-pod suggested that they occupy different ranges in winter. 相似文献