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661.
正As a natural mineral,Potash Magnesium Sulphate fertilizer has a quite high nutrient utilization rate without affecting soil p H in long time running related to Potassium Sulphate.And to displace Potassium Sulphate with Potash 相似文献
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DENG Tianlong WANG Shiqiang MENG Lingzong GUO Yafei YU Xiaoping LIU Yuanhui 《《地质学报》英文版》2014,88(Z1):307-309
正1 Introduction Salt lakes are widely distributed in the world,and salt lakes in China are mainly located in the area of the Qinghai-Xizang(Tibet),and the Autonomous Regions of Xinjiang and Inner Mongolia.There are more than 700salt lakes,each with an area larger than 1 km2,in the 相似文献
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ABSTRACTEquilibrium thermodynamic modelling, quartz in garnet (QuiG) Raman geobarometry, and modelling of garnet nucleation at overstepped conditions were applied to three garnet-bearing blueschists from a 1.5 km-long transect across the eclogite-blueschist unit in Sifnos, Greece, in order to evaluate the accuracy of P?T conditions calculated via equilibrium thermodynamics. QuiG barometry uses the Raman shift of quartz inclusions in garnet to estimate the pressure of garnet nucleation and is independent of chemical equilibrium. Garnet nucleation temperatures were estimated by determining the stability field of the palaeo-assemblage inferred from garnet inclusion suites on mineral assemblage diagrams calculated in the MnNCKFMASH system and on temperatures obtained from Zr in rutile thermometry. These conditions were then compared to P?T conditions calculated at the equilibrium garnet isograd, and the method of intersecting isopleths. The P?T conditions calculated with intersecting garnet isopleths over- and underestimated the temperature of nucleation in samples SPH99-1a and SPH99-7, respectively, whereas they significantly underestimated nucleation pressure in SPH99-5. Nucleation of garnet in SPH99-1a at 12 kbar and ~484°C requires overstepping of ~6 kbar and a reaction affinity of 2.2 kJ mol?1 O. SPH99-5 requires overstepping of ~8 kbar with garnet reaction affinities of at least 2.0 kJ mol?1 O at 15 kbar and ~520°C. SPH99-7 requires overstepping of approximately 15 kbar and affinities of about 2.0–2.4 kJ mol?1 O at ~23 kbar and ~530°C. The geotherms calculated from SPH99-7 (~6.7°C km?1) and SPH99-5 (9.8°C km?1) are in accordance with previous studies. The geotherm calculated from SPH99-1a, however, is warmer (11.3°C km?1), and could reflect changes in the rate of subduction or differences in structural position within the down-going slab. The 10 kbar pressure difference between SPH99-7 and SPH99-1a can be explained by thrusting and accretion of thin slices of underplated wedge material facilitated by slab rollback and gravitational collapse. 相似文献
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N-MORB和E-MORB数据挖掘——玄武岩判别图及洋中脊源区地幔性质的讨论 总被引:11,自引:7,他引:4
MORB分为N-MORB和E-MORB,二者的区分通常是以LREE亏损和富集为标志。玄武岩的基本理论主要是在MORB研究成果的基础上建立起来的。通常认为,N-MORB和OIB是两个独立的端元,E-MORB是N-MORB与OIB不同程度混合形成的。在20世纪70~80年代,玄武岩构造环境判别图的建立极大促进了玄武岩在地球动力学及大地构造背景研究的进展,其方法应用持续盛行了几十年。然而,国外学者现在已逐渐淡化玄武岩判别图解的应用,但在中国仍有方兴未艾之势。本文利用Pet DB数据库5万多个MORB数据的投图表明,全体样品投图的效果显然比抽样和典型样品得出的结果更扎实可靠,许多原先被广泛应用的主量、微量元素判别图无论从实践上还是理论上均存在一些问题。本文的研究结果进一步表明,MORB样品既有LREE亏损的,又有富集的,但亏损和富集程度与早先定义的差异较大,揭示了洋脊下地幔不均一性要比早先认识的更为复杂,成分范围变化更大,仅少数是强烈亏损的,部分可能是相当富集,甚至可以与OIB源区相类比;玄武岩构造环境判别图需要重新审视,基于岩浆成因机理的多维度、高置信度的判别体系有待于建立。 相似文献
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新冠肺炎疫情期间,疫情数据成为民众关注的重点,涌现出了大量可视化图件,及时地向公众传达着疫情的数量信息和时空分布及变化,帮助大众快速了解疫情当前状况、推断发展趋势.本文从疫情数据可视化表达内容的维度出发,分析不同可视化的表达形式以及其对疫情数据的加工程度,结合示例把可视化分为"1阶"、"2阶"和"多阶",并分析各自表达... 相似文献
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A study of four open clusters on Tautenburg Schmidt plates in the direction to the Galactic Centre (l = 17.0°, b = +0.8°) is presented. In a field of 8.95 square degrees proper motions and B, V magnitudes were determined for about 36 500 stars up to the limiting magnitudes B = 17m.9, V = 16m.8. For stars brighter than B = 16m an accuracy of about 3 mas/year has been estimated for proper motions. The rms errors of stellar magnitudes and (B—V) colours is about 0.1 mag. There are two open clusters already known in this sky area: Trumpler 32 (C 1814-133) and NGC 6611 (C 1816-138). By the inspection of the plates two additional anonymous clusters were identified near the double star ADS 11285 or BD −14°5014 (C 1819-146) and near the star BD −14°5016 (C 1820-146). The cluster membership determination was carried out using information on spatial and proper motion distributions of stars in the field. The colour-magnitude diagrams up to the limiting stellar magnitude were constructed. For each cluster interstellar extinction AV, diameters of the core and corona, ages and spatial velocity components (V, W) relative to the LSR in the Y, Z-galactic directions were derived. The distances to the clusters were obtained to 1720 pc, 2260 pc, 2130 pc and 2130 pc for Trumpler 32, NGC 6611, C 1819-146 and C 1820-146, respectively. All clusters are situated in the Sagittarius-Carina spiral arm. Their spatial location confirms the assumption that galactic spiral arms are close to logarithmic spirals with a characteristic angle of about 20 degrees. 相似文献
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