Fenton试剂氧化-微电解-接触氧化法处理丙烯腈废水实验研究

实验采用Fenton试剂氧化-微电解-接触氧化组合工艺处理丙烯腈废水。研究了各单元工艺的最佳控制参数和操作条件。结果表明,在废水pH值为3左右、反应时间2 h的前提下,双氧水投加量40 mL/L,二价铁离子质量浓度为0.4 g/L,再经过微电解处理后的出水进入接触氧化阶段。在溶解氧为4.5 mg/L左右,水力停留时间为10 h、容积负荷1.0 kg COD_Cr/（m³·d）左右的条件下,出水COD_Cr小于100 mg/L,可达到国家对丙烯腈废水处理要求的一级标准。     

三相生物流化床处理啤酒废水

通过三相生物流化床处理啤酒废水的实验研究,探讨曝气量和水力停留时间对处理效果的影响,确定最佳曝气量为0.25 m³/h,最佳水力停留时间为1.5 h。在该实验条件下,COD_cr平均去除率在85％以上,生物浓度高达28.31 mg/L,生物膜活性强,同时反应器具有较强的抗冲击负荷能力。     

氧协同菱铁矿降解微囊藻毒素机理研究

已知在无氧条件下天然矿物菱铁矿能成功水解微囊藻毒素-LR(MC-LR),然而实际应用过程中难以避免水中溶解氧(O₂)的存在,因此有必要深入研究不同溶氧量(DOC)条件下菱铁矿对MC-LR降解的影响。本文通过在无氧和有氧条件下菱铁矿对MC-LR的降解实验,发现在有氧条件下(溶氧量1.62～21.87 mg/L), MC-LR的降解速率均比无氧条件(k₀=0.030 16 mg·L^-1·h^-1)高且其降解速率随O₂含量增加而依次增加,当O₂加入量为1.0 mL(溶氧量21.87 mg/L)时,菱铁矿对MC-LR降解速率最大(0.083 34 mg·L^-1·h^-1),为无氧条件下的2.76倍。通过外加腐殖酸(humic acid, HA)和自由基进行捕获实验,发现FeCO₃能直接活化O₂产生超氧自由基(·O~-₂),以实现对MC-LR的氧化,但外加HA抑...     

吗啉废水的生化处理工艺

以含有吗啉、甲基吗啉的高浓度有机废水为研究对象,提出了曝气吹脱-吸附-生物处理的联合工艺,并在室内进行了小试实验。结果表明：原废水经过2次曝气吹脱后,ρ(NH₃-N)从62 500 mg/L降为431 mg/L,ρ(COD)从50 840 mg/L降为26 051 mg/L。通过吸附实验,ρ(COD)从26 051 mg/L降为2 769 mg/L,ρ(NH₃-N)从412 mg/L降为134 mg/L。在生物处理室内小试实验中,采用了活性污泥反应器与曝气生物滤池相结合的处理工艺。在活性污泥反应系统中,当废水pH为7.5、ρ(DO)为4.3 mg/L、水力停留时间为30 h时,COD的去除率最高,可以达到83.1%。在曝气生物滤池中,当ρ(DO)为3.3 mg/L时,COD去除率最高,达到55.8%。在生物处理的最佳参数条件下进行连续监测,当进水ρ(COD)为2 769 mg/L、出水ρ(COD)平均值为387 mg/L时,COD去除率可达到85.9%。吗啉废水经过此联合工艺的处理,ρ(COD)从50 840 mg/L降为387 mg/L。     

电-Fenton法处理苯酚废水影响因素的研究

采用电-Fenton法对含苯酚废水进行处理,以石墨为阴极、铁为阳极,并向阴极不断通入空气,电解过程产生的H2O2与阳极溶解的Fe^2＋形成Fenton试剂,Fenton试剂在电解过程中产生大量活性羟基自由基,能够很好地氧化降解废水中的苯酚。实验结果表明：影响苯酚去除率的因素主次顺序为pH值、电解质浓度、电解电压、电解时间、进水苯酚浓度。单因素分析得出电-Fenton法处理苯酚模拟废水的最优反应条件：pH值控制在2左右,反应时间为60min,电解电压选10V,Na2SO4的浓度为30g／L,进水苯酚浓度为150mg／L。在最优条件下苯酚的去除率为82％。     

Fe/Ag催化臭氧氧化降解苯酚的研究

为研究双金属催化剂去除有机污染物的效果,采用自制Fe/Ag催化剂对模拟苯酚废水进行了臭氧催化氧化处理。通过扫描电子显微镜(SEM)、比表面积分析仪(BET)和X射线衍射(XRD)对催化剂进行表征,并考察了催化剂类型、催化剂投加量和溶液初始pH值对降解效果的影响规律。结果表明:与Fe相比,Fe/Ag比表面积减少了22.8%,在Fe/Ag/O₃与含苯酚废水的反应体系中,反应遵循臭氧直接作用和活性自由基(·OH、·O₂、H₂O₂)共同作用的机理;Fe/Ag在反应过程中体现出良好的协同作用;300 mg/L的苯酚模拟废水在pH=6.3、Fe/Ag投加量为1.00 g的最优反应条件下经60 min反应,苯酚与化学需氧量(COD)去除率比单独臭氧氧化分别提高了18.4%和29.4%。     

UV/H2O2法降解乙酸影响因素的研究

通过采用UV/H₂O₂法,以乙酸为研究对象,高压汞灯为光源,在温度为（35±2）℃、曝空气量为0.8 L/min的条件下,研究了UV/H₂O₂技术对500 mL浓度为8 mmol/L的乙酸溶液进行的光降解反应。考察了各种因素对UV/H₂O₂降解乙酸的影响。实验表明,H₂O₂浓度为15 mmol/L、pH值为3.4时,乙酸降解效果最佳,此时,在240 min内,乙酸、TOC和COD的去除率可分别达到98%、98%和97%,体系中乙酸完全矿化。利用UV/H₂O₂法对实际糠醛废水进行了降解,效果良好。     

电化学循环井驱动模拟含水层化学氧化降解三氯乙烯

传统原位化学氧化地下水修复技术存在氧化剂迁移距离短和利用率低等问题。本研究在双井循环模式促进传质的基础上,通过注水井中的地下水电解原位提供O₂和H₂,配合乙二胺四乙酸(ethylenediamine tetraacetic acid,EDTA)络合溶解出含水层Fe(Ⅱ),活化O₂产生羟基自由基(•OH),实现地下水三氯乙烯(TCE)的氧化降解。在填充了砂土和黏土互层的二维砂槽中,设置电流为0.2 A、流速为72 cm/d、初始TCE浓度为3 mg/L,经过9 d的连续通电处理后,TCE浓度降低到1 mg/L,降解率达到67%。通电前投加0.5 mmol/L EDTA,经过1 d水流循环后含水层中溶解态Fe(Ⅱ)浓度从02 mg/L增加到414 mg/L,黏土区域较高。通电过程中,循环井促进O₂、Fe(Ⅱ)-EDTA和TCE的有效接触与反应,使TCE氧化降解。通电初期,黏土区域Fe(Ⅱ)氧化速率、TCE降解速率较周围慢,后期差异逐渐减小。未通电时加入醋酸钠可促进Fe(Ⅲ)还原,使含水层中铁循环利用。该修复过程通过循环井提升了氧化剂迁移距离,使用源于含水层的Fe(Ⅱ)-EDTA和稳定性较好的O₂提高了氧化剂利用率,有望应用于有机污染地下水修复。     

铁盐絮凝法对阳宗海湖泊水体的除砷效果及底泥的稳定性考察

2008年,昆明阳宗海受到严重砷污染,砷浓度高达0.134 mg/L。项目组充分考虑其受污染水体容量大、砷浓度低的实际情况,提出了安全、廉价、高效的FeCl3絮凝法治理方案。实验室小试结果表明,提出的FeCl₃絮凝法对As(Ⅲ)及As(V)均有理想的去除效果,并且湖水中大量存在的阴离子HCO^-₃可使治理过程中水体pH值基本保持不变。因此该方案摒弃了文献普遍报道所需要的预氧化及调节pH值的工艺步骤,将固体FeCl₃·6H₂O溶解、用湖水稀释后通过喷洒船将最终浓度为1%左右的FeCl₃水溶液喷洒到湖面上,使湖水中的AsO^3-₄及AsO^-₂与FeCl₃水解过程产生的Fe(OH)3胶体絮凝形成稳定的沉淀物被固定于底泥中。在对阳宗海进行降砷工程化治理期间,2009年11月-2010年9月砷浓度从0.117 mg/L快速下降到0.021 mg/L并可持续达到Ⅱ-Ⅲ类水标准(<0.05 mg/L),总除砷率高达 82.05%。沉积物中的As绝大部分以残渣态的形式被固定在沉积物中,生态风险很低。     

靖宇县玄武岩区矿泉水特征组分H2SiO3成因实验——以王大山泉为例

以靖宇县典型泉岩样为实验材料,结合野外实际情况,考虑pH值和CO₂影响因素设计了矿泉水中H₂SiO₃实验,对实验结果进行了化学动力学分析,并利用matlab建立数学模型分析了矿物反应的机理。结果表明:1)仅考虑pH值的情况下:初始pH值近中性(pH=7.25)时,实验溶液中H₂SiO₃释放量较小,反应难以发生;初始pH值为碱性(pH=8.10)时,实验溶液中H₂SiO₃缓慢增加,平均释放速率为3.08 mg/(kg·d)。2)在考虑pH值和CO₂情况下:初始pH值为碱性条件时,通入CO₂能够较快促进H₂SiO₃产生,平均释放速率可由4.29 mg/(kg·d)升高为12.00 mg/(kg·d);初始pH值为弱酸性(pH=6.64)时,实验溶液中H₂SiO₃增加较快,通入CO₂,溶液中H₂SiO₃释放速率稍微增加。3)实验溶液中H₂SiO₃释放规律符合Stanford一阶反应动力学模型。靖宇县矿泉水中H₂SiO₃主要来自偏硅酸矿物(斜长石、镁橄榄石、辉石)的反应。在中性条件下,玄武岩矿物很难反应;在碱性条件时,主要是玄武岩矿物的水解,反应缓慢;在弱酸性条件下,主要是玄武岩矿物与H⁺和CO₂的反应,反应强度较大。     

不同碳源对缺氧生物滤池生物脱氮的试验研究

针对生活污水的特点,采用曝气生物滤池技术对不同碳源（甲醇、乙酸钠和葡萄糖）条件下的生物脱氮效果进行了试验研究。结果表明,在C/N为3∶1～4∶1、滤速为1.0 m/h时,不同碳源对缺氧生物滤池的生物脱氮效果影响很大,其中以甲醇和乙酸钠作为外碳源时,脱氮效果较好,而以葡萄糖为碳源时的脱氮效果明显逊于二者。     

Marcasite precipitation from hydrothermal solutions

Pyrite and marcasite were precipitated by both slow addition of aqueous Fe²⁺ and SiO₃²⁻ to an H₂S solution and by mixing aqueous Fe²⁺ and Na₂S₄ solutions at 75°C. H₂S₂ or HS₂⁻ and H₂S₄ or HS₄⁻ were formed in the S₂O₃²⁻ and Na₂S₄ experiments, respectively. Marcasite formed at pH < pK₁ of the polysulfide species present (for H₂S₂, pK₁ = 5.0; for H₂S₄, pK₁ = 3.8 at 25°C). Marcasite forms when the neutral sulfane is the dominant polysulfide, whereas pyrite forms when mono-or divalent polysulfides are dominant. In natural solutions where H₂S₂ and HS₂ are likely to be the dominant polysulfides, marcasite will form only below pH 5 at all temperatures.

The pH-dependent precipitation of pyrite and marcasite may be caused by electrostatic interactions between polysulfide species and pyrite or marcasite growth surfaces: the protonated ends of H₂S₂ and HS₂ are repelled from pyrite growth sites but not from marcasite growth sites. The negative ions HS₂ and S₂²⁻ are strongly attracted to the positive pyrite growth sites. Masking of 1π_g^* electrons in the S₂ group by the protons makes HS₂ and H₂S₂ isoelectronic with AsS²⁻ and As₂²⁻, respectively ( et al., 1981). Thus, the loellingitederivative structure (marcasite) results when both ends of the polysulfide are protonated.

Marcasite occurs abundantly only for conditions below pH 5 and where H₂S₂ was formed near the site of deposition by either partial oxidation of aqueous H₂S by O₂ or by the reaction of higher oxidation state sulfur species that are reactive with H₂S at the conditions of formation e.g., S₂O₃²⁻ but not SO₄²⁻. The temperature of formation of natural marcasite may be as high as 240°C ( and , 1985), but preservation on a multimillion-year scale seems to require post-depositional temperatures of below about 160°C ( , 1973; and , 1985).     

Status report on stability of K-rich phases at mantle conditions

Experimental research on K-rich phases and observations from diamond inclusions, UHP metamorphic rocks, and xenoliths provide insights about the hosts for potassium at mantle conditions. K-rich clinopyroxene (Kcpx–KM³⁺Si₂O₆) can be an important component in clinopyroxenes at P>4 GPa, dependent upon coexisting K-bearing phases (solid or liquid) but not, apparently, upon temperature. Maximum Kcpx content can reach 25 mol%, with 17 mol% the highest reported in nature. Partitioning ^(K)D_(cpx/liquid) above 7 GPa=0.1–0.2 require ultrapotassic liquids to form highly potassic cpx or critical solid reactions, e.g., between Kspar and Di. Phlogopite can be stable to about 8 GPa at 1250 °C where either amphibole or liquid forms. When fluorine is present, it generally increases in Phl upon increasing P (and probably T) to about 6 GPa, but reactions forming amphibole and/or KMgF₃ limit F content between 6 and 8 GPa. The perovskite KMgF₃ is stable up to 10 GPa and 1400 °C as subsolidus breakdown products of phlogopite upon increasing P. ^(M4)K-substituted potassic richterite (ideally K(KCa)Mg₅Si₈O₂₂(OH,F)₂) is produced in K-rich peridotites above 6 GPa and in Di+Phl from 6 to 13 GPa. K content of amphibole is positively correlated with P; Al and F content decrease with P. In the system 1Kspar+1H₂O K-cymrite (hydrous hexasanidine–KAlSi₃O₈·nH₂O–Kcym) is stable from 2.5 GPa at 400 to 1200 °C and 9 GPa; Kcym can be a supersolidus phase. Formation of Kcym is sensitive to water content, not forming within experiments with H₂O2O>Kspar. Phase X, a potassium di-magnesium acid disilicate ((K_1−x−n)₂(Mg_1−nM_n³⁺)₂Si₂O₇H_2x), forms in mafic compositions at T=1150–1400 °C and P=9–17 GPa and is a potential host for K and H₂O at mantle conditions with a low-T geotherm or in subducting slabs. The composition of phase-X is not fixed but actually represents a solid solution in the stoichiometries □₂Mg₂Si₂O₇H₂–(K□)Mg₂Si₂O₇H–K₂Mg₂Si₂O₇ (□=vacancy), apparently stable only near the central composition. K-hollandite, KAlSi₃O₈, is possibly the most important K-rich phase at very high pressure, as it appears to be stable to conditions near the core–mantle boundary, 95 GPa and 2300 °C. Other K-rich phases are considered.     

Formation of Al-rich titanite (CaTiSiO4O–CaAlSiO4OH) reaction rims on ilmenite in metamorphic rocks as a function of fH2O and fO2

Reaction rims of titanite on ilmenite are described in samples from four terranes of amphibolite-facies metapelites and amphibolites namely the Tamil Nadu area, southern India; the Val Strona area of the Ivrea-Verbano Zone, northern Italy, the Bamble Sector, southern Norway, and the northwestern Austroalpine Ötztal Complex. The titanite rims, and hence the stability of titanite (CaTiSiO₄O) and Al–OH titanite, i.e. vuaganatite (hypothetical end-member CaAlSiO₄OH), are discussed in the light of fH₂O- and fO₂-buffered equilibria involving clinopyroxene, amphibole, biotite, ilmenite, magnetite, and quartz in the systems CaO–FeO/Fe₂O₃–TiO₂–SiO₂–H₂O–O₂ (CFTSH) and CaO–FeO/Fe₂O₃–Al₂O₃–SiO₂–H₂O–O₂ (CFASH) present in each of the examples. Textural evidence suggests that titanite reaction rims on ilmenite in rocks from Tamil Nadu, Val Strona, and the Bamble Sector originated most likely due to hydration reactions such as clinopyroxene + ilmenite + quartz + H₂O = amphibole + titanite and oxidation reactions such as amphibole + ilmenite + O₂ = titanite + magnetite + quartz + H₂O during amphibolite-facies metamorphism, or, as in the case of the Ötztal Complex, during a subsequent greenschist-facies overprint. Overstepping of these reactions requires fH₂O and fO₂ to be high for titanite formation, which is also in accordance with equilibria involving Al–OH titanite. This study shows that, in addition to P, T, bulk–rock composition and composition of the coexisting fluid, fO₂ and fH₂O also play an important role in the formation of Al-bearing titanite during amphibolite- and greenschist-facies metamorphism.     

雪硅钙石的矿物学特征研究

研究发现,雪硅钙石是一种硅酸钙水化物.根据电子探针分析结果计算得到的化学式为（Ca_4.424K_0.021Mg_0.003）_4.448（Si_5.731Al_0.728）_6.465O₁₆（OH）₂·4H₂O,与经典化学式Ca₅Si₆O₁₆（OH）₂·4H₂O基本一致.通过X射线粉晶衍射结果分析认为,该雪硅钙石属于1.4 nm类型雪硅钙石.雪硅钙石矿物呈放射状纤维集合体,颗粒大小为0.2 mm×0.5 mm×0.3 mm,黄褐色,正低突起,最高干涉色为Ⅰ级黄,二轴晶正光性,光轴角为53°.     

弱氧化气氛下烟煤热解特性及热解产物组成

为提高轻质焦油和煤气产率,选取陕西红柳林烟煤为研究对象,采用固定床反应器对比分析N₂气氛和弱氧气氛下（N₂+O₂）煤的热解产物产率分布及组成特性。结果表明:随着O₂的加入,半焦和焦油产率显著降低,CO和CO₂气体产率显著增大,导致总气体产率增大;由于发生氧化燃烧反应,随着热解气氛中氧含量的增大,H₂、CH₄和C₂—C₃产率逐渐降低,在此过程中水产率变化幅度较小;弱氧气氛下焦油分解温度大于N₂气氛,酚类物、脂肪烃及苯系物在弱氧气氛下热解焦油中的相对含量较低,且多环芳烃相对含量明显大于N₂气氛下热解焦油。当热解温度为800℃,过量空气系数ER=0.14时,焦油产率为6.22%,H₂产率14.01 mg/L,焦油和H₂产率达到最佳值。由于弱氧气氛下热解得到半焦的石墨化程度低于N₂气氛下的热解半焦,导致弱氧气氛下半焦反应活性大于N₂气氛。研究结果为固定床热解烟煤制备高值燃料提供基础数据。