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Analysis of high-spatial-resolution (approximately 0.8 arcsec) methane band and continuum imagery of Neptune's relatively homogeneous Equatorial Region yields significant constraints on (1) the stratospheric gaseous methane mixing ratio (fCH4,s), (2) the column abundances and optical properties of stratospheric and tropospheric hydrocarbon hazes, and (3) the wavelength-dependent single-scattering albedo of the 3-bar opaque cloud. From the center-to-limb behavior of the 7270-angstroms and 8900-angstrom sCH4 bands, the stratospheric methane mixing ratio is limited to fCH4,s < 1.7 x 10(-3), with a nominal value of fCH4,s = 3.5 x 10(-4), one to two orders of magnitude less than pre-Voyager estimates, but in agreement with a number of recent ultraviolet and thermal infrared measurements, and largely in agreement with the tropopause mixing ratio implied by Voyager temperature measurements. Upper limits to the stratospheric haze mass column abundance and 6190-angstroms and 8900-angstroms haze opacities are 0.61 microgram cm-2 and 0.075 and 0.042, respectively, with nominal values of 0.20 microgram cm-2 and 0.025 and 0.014 for the 0.2-micrometer radius particles preferred by the recent Voyager PPS analysis of Pryor et al. (1992, Icarus 99, 302-316). The tropospheric CH4 haze opacities are comparable to that found in the stratosphere, upper limits of 0.104 and 0.065 at 6190 angstroms and 8900 angstroms, respectively, with nominal values of 0.085 and 0.058. This indicates a column abundance less than 11.0 micrograms cm-2, corresponding to the methane gas content within a well-mixed 3% methane tropospheric layer only 0.1 cm thick near the 1.5-bar CH4 condensation level. Constraints on the single-scattering albedos of these hazes include (1) for the stratospheric component, 6190-angstroms and 8900-angstroms imaginary indices of refraction less than 0.047 and 0.099, respectively, with 0.000 (conservative scattering) being the nominal value at both wavelengths, and (2) CH4 haze single-scattering albedos greater than 0.85 and 0.50 at these two wavelengths, with conservative scattering again begin the preferred value. However, conservative scattering is ruled out for the opaque cloud near 3 bars marking the bottom of the visible atmosphere. Specifically, we find cloud single-scattering albedos of 0.915 +/- 0.006 at 6340 angstroms, 0.775 +/- 0.012 at 7490 angstroms, and 0.803 +/- 0.010 at 8260 angstrom. Global models utilizing a complete global spectrum confirm the red-absorbing character of the 3-bar cloud. The global-mean model has approximately 7.7 times greater stratospheric aerosol content then the Equatorial Region. An analysis of stratospheric haze precipitation rates indicates a steady-state haze production rate of 0.185-1.5 x 10(-14) g cm-2 sec-1, in agreement with recent theoretical photochemical estimates. Finally, reanalysis of the Voyager PPS 7500-angstroms phase angle data utilizing the fCH4,s value derived here confirms the Pryor et al. result of a tropospheric CH4 haze opacity of a few tenths in the 22-30 degrees S latitude region, several times that of the Equatorial Region or of the globe. The factor-of-10 reduction in fCH4,s below that assumed by Pryor et al. implies decreased gas absorption and consequently a decrease in the forward-scattering component of tropospheric aerosols. 相似文献
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在阿根廷科尔多瓦省Pampa平原进行了地下水和黄土沉积物的地球化学研究,该地区面积约30000km~2,位于西经61°45′～63°00′,南纬31°30′～33°55′。在选择的150个地下水水样中,确定其物理化学参数和矿化度(表)1。水样中96％以上为碱性, 相似文献
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陆地生态系统和气候系统紧密相关,特别是植物,土壤和大气圈之间的碳循环。已有人提出气候和大气二氧化碳浓度的变化调整循环,使大量的碳沉淀提供给陆地生态系统,但直接证据很有限。估计了稳定气候态之间变化引起的生态系统碳储备变化,但对生态系统碳流动对短期气候变化的动力响应不了解得不够充分。用一个陆地生物持球化学模式,配合一个一般的循环莱模拟短期气候变化,定量研究１８６１－２０７０年大气ＣＯ２气候引起的短期生 相似文献
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The temporal variability of 210Po and 210Pb was examined in the overlying water of the Zhubi Coral Reef flat to detect nutrient-like behavior of 210Po. Different mechanisms influencing their geochemical behaviors were observed. Excess 210Po relative to 210Pb revealed an additional input of 210Po other than in situ production from 210Pb. The 210Po input comes from the reef flat sediment through diffusion. The diffusion contributes 62% of the total 210Po. This diffusion of 210Po directly highlights its nutrient-like behavior. No input, but the slight removal, of 210Pb was observed. Fractionation factors indicate that particulate matter prefers to adsorb 210Po rather than 210Pb. In combination with particulate composition, 210Po diffusion was closely related to organic matter. These results reveal that 210Po might be a potential tracer for quantifying nutrient recycling in the Coral Reef system. 相似文献
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磷酸一酯（ＲＯ）Ｐ（Ｏ）（ＯＨ）２是一种强极性的有机磷化合物。研究了水体中磷酸一（１－萘）酯的富集和上色谱分析,建立了一个简便快速、高灵敏度、实用的分析方法。富集是采用固相萃取方法,选用载有十八烷基硅烷的尼龙滤膜吸附,甲醇洗脱,回收率达７２％￣７％。它的气相色谱分析选用ＢＳＴＦＡ为衍生剂,反应条件为温度６５℃,反应时间３０ｍｉｎ,获得了满意的结果。方法的最低检测限为０。０６ｎｇ。 相似文献
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甘肃靖远景泰一带泥盆系雪山组和沙流水组以河湖相碎屑岩为主 ,内发育典型的风暴沉积构造 (包括渠铸型、槽筑型、丘状交错层理和洼状交错层理、平等层理、块状层理和递变层理等 )。雪山组和沙流水组的风暴沉积主要包括 3种岩相类型 :A底部具渠铸型或槽筑型的块状层理和递变层理砂岩。 B具丘状或洼状交错层理及平行层理的砂岩。C具均质层理的粉砂岩、泥质岩。上述岩相 A,B,C分别代表风暴事件沉积中风暴流行作用 -风暴后的快速悬浮沉积 (事件沉积 ) ,它们组合成典型的风暴沉积序列。甘肃靖远一带晚加里东 -早海西期位于北祁连造山带北缘同造山盆地的构造背景下 ,泥盆纪雪山组 -沙流水组以河湖相沉积为主。泥盆纪湖相风暴岩的发现表明该区处于低纬度 (5°～ 2 0°)的风暴作用带。中、晚泥盆世北祁连造山带构造隆升渐弱 ,海拔不高 ,不足以阻隔风暴作用对山后湖盆的侵扰。因此在近海湖盆中形成风暴岩沉积。该沉积对于认识北祁连 -河西走廊泥盆纪的古地理、古气候及古构造具有重要意义 相似文献
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论震积作用和震积岩 总被引：93，自引：2，他引：93
地震是一种灾害性的地质事件。地震及其引发的海啸、重力流可以形成震积岩、海啸岩和震浊积岩。在地震过程中,震积作用可以形成特殊的构造标志(地震断裂层、地裂缝、微同沉积断裂、微褶皱纹理、重力断层等)、沉积和成岩标志(砂岩脉、泥岩脉、泥晶脉,即磨牙(molar tooth)构造、枕状层、砂火山、泥火山、同沉积变形构造、丘状层理等)。地震沉积组合包括原地震积岩(A,包括震裂岩、震褶岩、自碎屑角砾岩、内碎屑副角砾岩等)、海啸岩(B,由具丘状层理、平行层理的碎屑岩或内碎屑灰岩组成)、震浊积岩(C,由具块状层理、递变层理或玻马序列的粗碎屑岩或碎屑灰岩组成)及背景沉积(D)4个单元,它们组合成A-B-C-D、A-B-D、A-C-D、A-D、B-D、C-D等6种类型的沉积序列。 相似文献