滇西莴中晚始新世高镁富钾火山岩中单斜辉石斑晶环带结构的成因：岩浆补给-混合过程

滇西莴中晚始新世高镁富钾火山岩中单斜辉石斑晶普遍出现正环带结构、反环带结构或韵律环带结构，少量为具绿色核部的单斜辉石(“绿核辉石”)。反环带斑晶和“绿核辉石”的幔部与正环带斑晶的核部具有相似并且相对较窄的成分范围，相对高Mg#（0.83 ~ 0.90）,低TiO2（0.13 % ~ 0.29 %）,Al2O3（0.73 % ~ 1.68 %）和Na2O （0.22 % ~ 0.42 %），为钾质岩浆平衡结晶的产物。反环带斑晶的核部相对低Mg#（0.77 ~ 0.84），但与反环带斑晶的幔部、正环带斑晶的核部均具有相似的Ti/Al比值（0.06 ~ 0.16）；韵律环带结构斑晶的成分变化均在正、反环带斑晶的成分范围之内。莴中高镁富钾火山岩中的这些环带结构单斜辉石斑晶应来源于相似的岩浆体系，反 环带结构表明在岩浆房存在较原始岩浆对较演化岩浆再补给的岩浆混合过程，而韵律环带结构特征揭示曾多次发生这种岩浆混合过程。“绿核辉石”的核部明显低Mg# （0.50 ~ 0.74）,相对富Al2O3（1.66 % ~ 3.63 %）和Na2O（0.87 % ~ 2.17 %），具有明显较低的Ti/Al比值（< 0.05）和较高的AlVI/AlIV比值（0.38 ~ 0.76），为下地壳捕虏晶 来源，证实了在滇西晚始新世富钾岩浆演化过程中存在少量地壳混染作用。     

拉萨地块中南部新生代超钾质岩中单斜辉石斑晶的环带成分研究

在青藏高原拉萨地块中南部的米巴勒、麦嘎乡、赛利普地区分布有新生代的超钾质火山岩,这些火山岩的斑晶中广泛发育单斜辉石正环带,其记录了超钾质岩浆的早期结晶历史.这些单斜辉石的正环带核部到边部Mg*和镁、铬的氧化物含量降低,而铁、钠、铝、钛的氧化物含量升高,它反映了岩浆正常结晶的顺序.米巴勒地区超钾质岩中的单斜辉石还出现反环带和少量的韵律环带,可能与该地区所发现的共生钠质过碱性火山岩有关,韵律环带揭示了其可能是相同成分的超钾质母岩浆从岩浆源区多次补给形成,而反环带则可能是与钠质过碱性火山岩岩浆存在一定程度的混合造成的.尽管三个地区超钾质火山岩的喷发时间稍不同,但是三地区的单斜辉石正环带核部成分基本相同,它们具有相似的Al-Ti值,指示出超钾质岩形成在相同的构造环境并具有相同的岩浆成因.     

阿尔泰南缘中泥盆统北塔山组火山岩的矿物学研究

阿尔泰山南缘中泥盆统北塔山组火山岩极为发育。本文对富辉橄玄岩和玄武岩中的单斜辉石和橄榄石斑晶进行了矿物化学分析,并结合矿物的地质温压计和岩浆结晶模拟,约束了两种岩石中矿物的形成过程,推测了原始岩浆的演化过程。提出富辉橄玄岩和玄武岩的原始岩浆属于拉斑玄武系列,富辉橄玄岩中的高压单斜辉石来源于深部（40～50 km）,其结晶早于橄榄石;玄武岩中单斜辉石大多属于岩浆房结晶产物（30～40km）,其结晶晚于橄榄石;两种岩石中橄榄石均属于岩浆房结晶产物（30～40 km）。     

南海扩张前序岩浆活动:解译华南三水盆地古近纪玄武质岩浆作用过程

华南三水盆地古近纪玄武岩（64～43 Ma）记录了南海扩张前大陆裂解过程中的岩浆-构造活动,但其岩浆演化过程及其动力学机制并不清楚。为此,作者对其开展了详细的岩石学和矿物学研究。三水盆地古近纪玄武岩具有OIB型的微量元素组成特征,由软流圈地幔源区部分熔融形成。该玄武岩中单斜辉石斑晶显示复杂的环带结构,包括正环带、反环带及韵律环带结构,指示了复杂的岩浆作用过程。正环带单斜辉石斑晶为核-边结构,其核部圆化或呈不规则形状,边部自形,指示了早期晶体与晚期演化岩浆混合后发生熔蚀-再生长过程。绝大部分反环带单斜辉石斑晶为核-幔-边结构,其核部相对低Mg,并被部分熔蚀呈不规则状或圆化,幔部相对高Mg,边部自形,反映了相对原始岩浆的补给作用。个别反环带单斜辉石为核-边结构,其核部Al₂O₃、TiO₂含量和Mg^#值明显偏低,为下地壳捕虏晶,表明岩浆从地幔源区上升汇聚到地壳岩浆房的过程中经历了轻微的地壳同化混染作用。韵律环带结构单斜辉石核部常为不规则状,幔部成分呈韵律状变化,边部自形,记录了岩浆对流及多次岩浆演化-补给...     

内蒙古天和永玄武岩成因：岩相学与矿物学分析

天和永地区南北向出露的小面积单层碱性玄武岩,岩石中出现至少三种矿物共生组合关系。所有岩石均以橄榄石作为主要斑晶矿物,大颗粒环带橄榄石斑晶中心镁值为89．5,边缘镁值为70．3,小颗粒环带橄榄石镁值46．2～78．9。粒径最小的橄榄石聚集体和散布的基质橄榄石均无明显环带,前者镁值67．4～68．1,后者镁值65．5—72．1;单斜辉石由相对高钛高铝贫硅的散布柱状辉石和相对低钛低铝富硅的聚集粒状辉石组成,前者形成于低压快速淬火环境,镁值65．1—77．1,后者形成于富含挥发份的低压低过冷度环境,镁值77．7～78．0。所有单斜辉石均以次透辉石为主,个别为深绿辉石;斜长石以包含结构产出为主,为相对偏酸性的中长石An=33．7～37．4,CaO含量低与早期大量单斜辉石结晶有关。由于残余岩浆内K,0和Na20含量富集且极不均一,晚期结晶的长石同时出现了高钠长石、K-高钠长石（歪长石）和K-透长石;钛铁氧化物多数为晚期结晶的细粒基质矿物,少量以0．3ram左右的斑晶和橄榄石斑晶中的包裹体形式存在,可归属为钛铁尖晶石（Usp）-磁铁矿（Mt）固溶体系列,晚期逐渐向贫铝、铬和富钛方向演化。由于以上各种造岩矿物的晶出,导致残余岩浆形成的火山玻璃向贫镁、铁、钙和富铝、钾方向演化,火山玻璃的全碱含量变异趋势与全岩类似,均和SiO2含量无明显相关性,火山玻璃具有响岩和粗面安山岩成分特征,K2O／Na2O值变化大0．68～1．61,均为钾玄岩系列,Na2O含量依然呈现宽区间特征,是天和永玄武岩由钾质过渡到钠质的主要原因。天和永玄武质岩浆从地幔运移到地表仅需5小时-5天,大颗粒斑晶橄榄石和小颗粒基质橄榄石生长仅需几小时到几天,前者形成无须深部岩浆房停留,后者近似晚期岩浆快速淬火时间。高镁橄榄石斑晶与残余岩浆的扩散平衡时间约42天～252天。深部结晶的橄榄石在运移途中和地表流动过程中缺乏足够的时间和适宜的动力学条件而无法离开岩浆体系。全岩与火山玻璃间缺少中间过渡成分,呈两个相对集中的端元组分存在亦由晶出矿物无法离开岩浆体系所致。天和永玄武岩的成岩时间尺度远小于同化混染和岩浆分异的时间尺度,是岩浆作用过程未能明显影响其不均一原生岩浆性质的主要原因。因此,岩浆作用的某些物理过程分析是认识岩浆起源与岩浆作用过程及其对火成岩多样性的贡献的重要方面,同时对于理解和约束岩浆作用的某些化学过程也是十分有益的。     

南海新生代玄武岩中单斜辉石矿物化学及成因意义

从南海南大陆坡底至北大陆坡底采集的玄武岩样品,基本可以代表南海新生代岩浆活动的代表性样品.本文中对这些玄武岩中单斜辉石的矿物化学成分进行了研究,研究的单斜辉石以顽透辉石为主(占3/4),还有少量普通辉石及次透辉石等,也出现少量较为罕见的富钙辉石,位于深绿辉石区域内.基质微晶辉石比辉石斑晶更富钙、钛、铁,可能反映了岩浆演化向着富钙、钛、铁方向发展,且碱度逐渐降低.与碱性系列的演化趋势基本一致.由单斜辉石-熔体平衡温压计计算的岩浆房深度分别为:碱玄岩岩浆房约49km左右,粗面玄武岩岩浆房约25km;玄武岩岩浆房约15km.由碱玄岩→粗面玄武岩→玄武岩,平衡温度(K)依次降低:从1535～1498→1429→1369.南海新生代玄武岩为板内碱性玄武岩.碱性玄武岩系列可能是地幔柱在上升过程中在不同深度处发生部分熔融并伴随有分离结晶作用等物理化学过程的连续演变的产物.     

松辽盆地东南隆起区营城组珍珠岩斑晶矿物研究

松辽盆地早白垩世营城组火山岩系含有丰富的珍珠岩,为松辽盆地重要的油气勘探目的层位。在松辽盆地边缘东南隆起九台地区出露有比较新鲜的珍珠岩,内部斑晶保存完好,裂隙发育;斑晶矿物主要有斜长石、黑云母、角闪石,还有镁铁质的单斜辉石和斜方辉石。对含斑晶珍珠岩和剔除斑晶后的珍珠岩玻璃质分别进行地球化学分析,斑晶矿物进行单矿物电子探针成分研究。其结果表明：该珍珠岩属于酸性高钾钙-碱性系列,微量和稀土元素特征显示与上部地壳相似;斑晶矿物单斜辉石为斜紫苏辉石和次透辉石,斜方辉石为紫苏辉石,均显示变质成因,属于捕虏晶;与珍珠岩相邻层位玄武岩的斑晶斜长石为拉长石,单斜辉石为铁次透辉石,属于岩浆成因。这些特征表明,珍珠岩原岩可能来自于上部地壳,其辉石等捕虏晶为岩浆上侵运移过程与围岩发生混染作用的结果。     

内蒙锡盟新生代玄武岩的岩石学研究

依照地层顺序和火山机构的完好程度,内蒙锡盟新生代玄武岩可粗略划分为三期。各期玄武岩又可分出若干层(次)。玄武岩由含量不等的橄榄石、单斜辉石和斜长石斑晶及基质组成。部分玄武岩含有二辉橄榄岩等深源包体。斑晶矿物均具有成分环带。矿物化学、岩石化学资料揭示出本区玄武岩从原生岩浆到进化岩浆的主要演化机制是以橄榄石为主的分离结晶作用,同时在部分进化岩浆中还存在岩浆混合作用。稀土元素资料还指出了一个形成本区原生岩浆以及派生岩浆的原生母岩浆的重要机制:上地幔渐进的部分熔融作用。     

加勒比海小安德列斯岛弧Kick’emJenny海底火山岩的斜长石成分环带:示踪大洋岛弧岩浆房的演化

我们对采自于加勒比海地区小安德列斯岛弧(Lesser Antilles Arc)Kick’em Jenny(KEJ)海底火山玄武岩中的斜长石斑晶进行了矿物形态和成分分析。利用电子探针(EMPA)和LA-ICP-MS测定了具有环带结构的斜长石斑晶中主量元素的空间分布,同时也利用LA-ICP-MS分析了斜长石中Sr的分布。结果表明,在不同的矿物斑晶中,元素含量均表现出和环带结构相联系的空间分布变化。斜长石斑晶中最主要的结构为韵律环带以及熔蚀结构,所测定的矿物边缘都存在An值从由内向外迅速降低的致密韵律环带,可能反映了快速结晶时的不平衡;而晶体内部的稀疏韵律环带结构是由岩浆填充或对流活动导致的。部分斜长石的熔蚀层An值由内向外升高,反映了高Ca岩浆填充的过程。这说明斜长石斑晶的矿物形态和元素环带可以用来制约俯冲带海底火山岩浆从源区上升到岩浆房再到喷发的复杂过程,包括岩浆演化、熔体多次填充、熔体与结晶矿物之间的反应、以及矿物再熔融等。这对于理解海底火山的喷发以及岛弧岩浆岩的演化有重要意义。     

云南禄劝县朗茂二叠纪玄武玢岩的岩石学特征及其对高钛玄武岩成因的指示意义

云南禄劝县朗茂次火山岩体位于峨眉山大火成岩省的东部,由下部的玄武玢岩和上部的多斑玄武玢岩组成。全岩主要元素分析结果表明,其TFe2O3和TiO2含量较高,分别为14.05%~14.86%、3.12%~4.69%,属于高钛玄武岩的范围,但是两者的主要元素也存在一定的差别,表现在前者有相对低的S iO2、TiO2、A l2O3和Na2O含量以及相对高的MgO和CaO含量。矿物电子探针分析结果表明,单斜辉石均为相对富铁钛的普通辉石,斜长石为中-拉长石,而钛磁铁矿以异常高的TiO2含量(24.25%~26.65%)为特征。根据单斜辉石温度计和压力计以及斜长石的温度计估算结果,玄武玢岩和多斑玄武玢岩的形成温度和压力均有明显的差别,后者温度和压力较低,分别为1 143~1 176℃、0.23~0.86 MPa;而前者较高,分别为1 316~1 370℃、1.98~2.25 MPa。另外,钛磁铁矿中异常高的XUsp含量以及单斜辉石中低的Fe3+指示岩浆的低氧逸度,估算的氧逸度为1.013×10-6~1.013×10-10Pa。因此可以推测,由于低的氧逸度抑制了钛磁铁矿在早期结晶,导致晚期岩浆富集铁和钛,所以高钛玄武岩可以通过正常的低钛玄武岩岩浆在早期发生硅酸盐矿物的分离结晶演化而成。但是由于有一部分铁和钛在单斜辉石结晶过程中进入单斜辉石晶体中,导致在残留岩浆中没有高度富集铁钛,因而在该地区没有形成钒钛磁铁矿矿床。     

Flood and Shield Basalts from Ethiopia: Magmas from the African Superswell

The Ethiopian plateau is made up of several distinct volcaniccentres of different ages and magmatic affinities. In the NE,a thick sequence of 30 Ma flood basalts is overlain by the 30Ma Simien shield volcano. The flood basalts and most of thisshield volcano, except for a thin veneer of alkali basalt, aretholeiitic. In the centre of the province, a far thinner sequenceof flood basalt is overlain by the 22 Ma Choke and Guguftu shieldvolcanoes. Like the underlying flood basalts, these shieldsare composed of alkaline lavas. A third type of magma, whichalso erupted at 30 Ma, is more magnesian, alkaline and stronglyenriched in incompatible trace elements. Eruption of this magmawas confined to the NE of the province, a region where the lavaflows are steeply tilted as a result of deformation contemporaneouswith their emplacement. Younger shields (e.g. Mt Guna, 10·7Ma) are composed of Si-undersaturated lavas. The three maintypes of magma have very different major and trace element characteristicsranging from compositions low in incompatible elements in thetholeiites [e.g. 10 ppm La at 7 wt % MgO (=La₇), La/Yb = 4·2],moderate in the alkali basalts (La₇ = 24, La/Yb = 9·2),and very high in the magnesian alkaline magmas (La₇ = 43, La/Yb= 17). Although their Nd and Sr isotope compositions are similar,Pb isotopic compositions vary considerably; ²⁰⁶Pb/²⁰⁴Pb variesin the range of     

New paleomagnetic and paleointensity data from Pliocene lava flows from the Lesser Caucasus

A paleomagnetic, rock-magnetic and paleointensity study has been carried out on 14 basaltic lava flows from two Pliocene (K–Ar age between 3.09 ± 0.10 Ma and 4.00 ± 0.15 Ma) sequences (Apnia and Korxi) from the eastern Djhavakheti Highland in southern Georgia (Caucasus).Measurement of strong-field magnetisation versus temperature curves yielded three types of thermomagnetic curves: (i) Reversible curves with magnetite as only remanence carrier (type H); (ii) irreversible curves with magnetite as only carrier of remanence (type H⁻) and (iii) irreversible curves showing a low Curie-temperature phase and magnetite (type L). Analysis of hysteresis curves showed that samples were characterised by a mixture of single-domain and multi-domain grains.Paleomagnetic experiments allowed determining characteristic components for all flows and normal polarities (6 flows), reversed polarities (7 flows) and intermediate polarities (1 flow) were observed.. Paleomagnetic poles were calculated using only those sites unequivocally showing normal or reversed polarities. The paleomagnetic pole obtained from flows of both combined sequences (latitude λ = 77.9°N, longitude ϕ = 152.1°E, n = 13, A₉₅ = 11.8°, k = 13.4) showed a good agreement with the 5 Ma window of the European synthetic apparent polar wander path of Besse and Courtillot (2002). The paleomagnetic direction of the combined Apnia-Korxi flows agrees well with the expected one, showing no significant tectonic rotation. The latter cannot be however, completely excluded in the Korxi section. In that section, analysis of the angular dispersion of virtual geomagnetic poles yields a much higher value than expected.Paleointensity experiments using the Coe method were performed on 31 specimens from 10 flows. After application of specific selection criteria, 19 samples from 8 flows were observed to provide successful determinations, with mean flow values showing a wide scatter. If only flows with more than one successful paleointensity determination are taken into account, virtual dipole moments (VDMs) vary between 3.5 × 10²² A m² and 8.3 × 10²² A m². In intermediate polarity site AP2 no weak transitional paleostrength values were observed.     

Climatic cycles inferred from the aminostratigraphy and aminochronology of Quaternary dunes and palaeosols from the eastern islands of the Canary Archipelago

Aminochronological and aminostratigraphical methods have been used to study the Quaternary aeolian deposits from the islands located east of the Canary Archipelago (Fuerteventura and Lanzarote islands and La Graciosa, Montaña Clara and Alegranza islets). The extent of racemisation/epimerisation of four amino acids (isoleucine, aspartic acid, phenylalanine and glutamic acid) was measured in land snail shells of the genus Theba. The age calculation algorithms of these amino acids have been determined to permit the numerical dating of these deposits. Eight Aminozones, each defining dune/palaeosol‐formation episodes, have been distinguished and dated at 48.6 ± 6.4, 42.5 ± 6.0, 37.8 ± 4.6, 29.4 ± 4.8, 22.4 ± 4.5, 14.9 ± 3.6, 11.0 ± 4.0 and 5.4 ± 1.1 ka BP, the first five of them defining cycles of 5–7 ka. The alternation of palaeosols and aeolian deposits, which are related to abrupt transitions from humid to arid conditions, are the reflection of globally induced changes in North Africa palaeoenvironmental conditions linked to the effect of African palaeomonsoons on the trade winds and the Saharan Air Layer. Probably these aeolian cycles, with a recurrence period of 5–7 ka, are the expression of multiples of the ～2.4 ka solar‐cycle. Copyright © 2005 John Wiley & Sons, Ltd.     

芬兰晕彩斜长石晕彩成因探讨——包裹体及其与晕彩的关系

对芬兰斜长岩中斜长石的宏观和微观观测显示,无晕彩的斜长石包裹体不发育,有晕彩的斜长石发育定向排列的针状包裹体。依据斜长石中包裹体的发育程度,可将包裹体分为两类:密集型包裹体(35～50条/mm)和稀疏型包裹体(25～35条/mm)。发育密集型包裹体的斜长石的晕彩以蓝色为主,发育稀疏型包裹体的斜长石的晕彩以红色或橙红色为主。电子探针、扫描电镜和激光拉曼光谱的分析结果表明,该晕彩斜长石中的所有包裹体在成分上一致,均为磁铁矿,有晕彩的斜长石和无晕彩的斜长石的成分也一致。这表明该斜长岩中的斜长石是否具有晕彩与斜长石的成分、包裹体的成分及斜长石的双晶发育程度无关,而与包裹体的发育程度有关。斜长石和其中定向排列的磁铁矿针状包裹体类似于光学中的光栅效应,斜长石中晕彩的出现可能是光栅衍射和干涉造成的。     

Land-sea correlations for the last glaciation inferred from a pollen and dinocyst record from the portuguese margin

Pollen and dinoflagellate cyst assemblages from Core SU 81-18 recovered off Portugal (37°46′N, 10°11′W; 3135-m water depth) have been used to document the short-term environmental changes that occurred in southwest Europe since 25,000 yr B.P. The relationship between the oceanic and continental environments has been further examined by the use of other marine proxies (coarse sedimentary fraction, foraminifera) and by comparison with proximal land pollen records. Heinrich 2 (H2) and Heinrich 1 (H1) events were the most extreme parts of the highly variable last glacial period, with the maximum extension of dry steppe on land and the occurrence of cool and dilute waters at the core site. Our study shows that H1 and H2 are divided in two distinct phases: one with Neogloboquadrina pachyderma left coiling associated with the maximum input of ice rafted debris, reflecting the in situ release of icebergs and the occurrence of cool and dilute seawater at the core site; the other with dinoflagellate cysts of subpolar affinity, Bitectatodinium tepikiense, reflecting a seasonal control marked by warm summer SST and cold winter SST.     

Manganese and Molybdenum in Phosphorites from the Ocean

The behavior of molybdenum and manganese is studied in phosphorite samples from shelves, seamounts, and islands of the ocean. In shelf phosphorites, molybdenum and manganese contents are 2–128 and 12–1915 ppm, respectively, while the Mo/Mn ratio ranges from 0.004 to 4.5. Phosphorites from oceanic seamounts impregnated with ferromanganese oxyhydroxides contain 0.84–14.5 ppm of Mo and 0.1–17% of Mn. The Mo/Mn ratio ranges within 0.0008–0.004. Phosphate-bearing ferromanganese crusts overlying the seamount phosphorites contain 54–798 ppm of Mo and 10–20% of Mn; Mo/Mn ratio varies within 0.002–0.005. Corresponding values for most island phosphorites are 0.44–11.2 ppm, 27–287 ppm, and 0.008–0.20, respectively. Phosphorites from reduced environments are characterized by a relative enrichment in Mo and depletion in Mn, whereas the Mo/Mn ratio reaches maximum values. The ratio decreases with transition to suboxic and oxic conditions. Molybdenum content in recent shelf sediments is commonly higher than that in authigenic phosphorites from these sediments. Recent phosphorite nodules from the Namibian shelf become depleted in Mo and Mn during their lithification, but Pliocene–Pleistocene nodules of similar composition and origin from the same region are enriched in Mo and characterized by a variable Mn content. The higher Mo content in phosphate-bearing ferromanganese crusts is a result of coprecipitation of Mo and Mn from seawater. Nonweathered phosphorites on continents and phosphorites from oceanic shelves are largely enriched in Mo with the Mo/Mn ratio ranging from 0.01 to 1.0. This is an evidence of their formation in reducing conditions.     

如何判别干酪根裂解气与原油裂解气

<正> 过去的天然气成因研究只是指出天然气是属于腐泥型、腐殖型还是混合型。但是天然气既可来源于干酪根裂解气,也可来源于原油(包括胶质和沥青质)的裂解气,而对于腐泥型有机质,天然气绝大部分是来自于干酪根先期生成的原油的裂解气,只有少部分天然气来自于干酪根的裂解。因此,对于母质类型好的有机质,干酪根在成熟阶段生成的油能否     

南岭东段早侏罗世沉积岩碎屑锆石U-Pb定年及其地质意义——以东坑盆地为例

印支造山运动是华南早中生代最重要的构造-岩浆事件,它在很大程度上影响了华南现今的地形和地貌特点。本文研究了南岭东段赣南早侏罗世东坑火山岩盆地沉积岩的碎屑锆石U-Pb年代,获得最显著的年龄峰值为196Ma、238Ma、364Ma和427Ma,表明该沉积岩并不是外来的震旦纪-寒武纪变质岩,而是早侏罗世裂谷火山盆地的沉积物。缺乏260～290Ma的锆石年龄,很可能反映物质为近源来源。通过与闽西南晚三叠世和华南内陆中-晚二叠世沉积砂岩中碎屑锆石年龄谱对比,反映华南印支早期(290～260Ma)岩浆活动主体在东南沿海地区,晚期(240～200Ma)主体发育在内陆地区。大量印支期侵入岩锆石的出现也很可能表明华南内陆印支造山带在～190Ma已经经历了相当程度的垮塌。     

Turbulence in the inner solar wind determined from frequency fluctuations of the downlink signals from the ULYSSES and GALILEO spacecraft

The results of several sets of measurements of the frequency of radio signals during coronal-sounding experiments carried out from 1991 to 2000 using the ULYSSES and GALILEO spacecraft are presented and analyzed. The S-band signals (carrier frequency f = 2295 MHz) were received at the three 70-m widely spaced ground stations of the NASA Deep Space Network. As a rule, the frequency-fluctuation spectra at frequencies above 1 mHz are power-laws. At small heliocentric distances, R < 10R_⊙ (R_⊙ is the solar radius), the spectral index is close to zero; this corresponds to a spectral index for the one-dimensional turbulence spectrum p₁ = 1. The index of the frequency-fluctuation spectra in the region of the supersonic solar wind at distances R > 30 R_⊙ is between 0.5 and 0.7 (p₁ = 1.5–1.7). The results demonstrate a substantial difference between the turbulence regimes in these regions: in the region of the established solar wind, the power-law spectra are determined by nonlinear cascade processes that pump energy from the outer turbulence scale to the small-scale part of the spectrum, whereas such cascade processes are absent in the solar wind acceleration region. Near the solar minimum, the change in the turbulence regime of the fast, high-latitude solar wind occurs at greater distances than for the slow, low-latitude solar wind. Spectra with a sharp cutoff at high frequencies have been detected for the first time. Such spectra are observed only at R < 10 R_⊙ and at sufficiently low levels of the electron density fluctuations. The measured cutoff frequencies are between 10 and 30 mHz; the cutoff frequency tends to increase with heliocentric distance. The variance of the plasma-density fluctuations has been estimated for the slow, low-latitude solar wind. These estimates suggest that the relative fluctuation level at distances 7 R_⊙ < R < 30 R_⊙ does not depend on heliocentric distance. The cross correlation of the frequency fluctuations recorded at widely spaced ground stations increases with the index of the frequency-fluctuation spectrum. At distances R ≈ 10 R_⊙, the rate of temporal changes in irregularities on the scale of several thousand kilometers is less than or comparable to the solar wind velocity.