{"title":"德干火山省西海岸孟买地区岩脉的古地磁研究:对德干火山喷发年龄和跨度的启示","authors":"S. Patil, B. Arora","doi":"10.3809/JVIRTEX.2003.00077","DOIUrl":null,"url":null,"abstract":"Through detailed AF and thermal demagnetizations of 35 samples (161 specimens) collected from 6 dykes located at Murud region, south of Mumbai, we report the first mean characteristic remanent magnetization direction as D=341°; I= -42°(μ95=5.7; N=6 dykes) for the dykes intruded into the West Coast zone of the Deccan Volcanic Province. The virtual geomagnetic pole (VGP) position (44°N; 83°W; A95=5.8°; N=6 dykes) calculated from this study is compared with those of the Narmada-Tapti zone dykes and with the Deccan Super Pole, proposed by Vandamme et al. (1991). Based on the concordance of these poles and recently reported 40Ar/39Ar and 87Rb/86Sr dates on the dykes of the studied region (Murud), it is proposed that the entire Deccan flows and the associated dykes were erupted in a short interval close to the Cretaceous-Tertiary Boundary at 65.5 Ma. Thermal demagnetization spectra along with isothermal remanent magnetizations and LF test experiments indicated that the SD type titano-magnetite was the major ChRM carrying magnetic mineral in the samples. Out of the 6 studied dykes, one dolerite dyke showing the “reverse magnetic polarity”, could have acted as a feeder dyke to the Poladpur Formation flows, which host the dykes in the studied area. The remaining four dolerite dykes and one lamprophyre dyke, yielding “normal polarity” directions, might have fed to the youngest formations of Wai Subgroup flows, viz., Panhala Formation and Desur Formation, which were eroded in the studied region. INTRODUCTION It is a widely accepted view that the Deccan flood basalts of Indian sub-continent, covering at present an area of 500,000 sq.km., is the result of outburst of immense magma material from the Reunion Hot spot source that impinged on the northerly drifting Indian lithosphere in the Late Cretaceous (Morgan, 1981). The Deccan Province is traversed by three major rift zones, namely the Narmada-Tapti-Son rift, the Cambay rift and the West Coast rift, which form a triple junction at the CambayBasin (Sheth and Chandrashekharam, 1997). Over the last 30 years the Deccan Traps have attained the attention of geochronologists, palaeomagnetists, geochemists and petrologists alike with its impressive horizontal lava piles, enormous size and volume along with its rapid eruptions at the K/T boundary coinciding with the much debated mass extinctions (Sen, 2001; Subbarao, 1999a and 1999b). Palaeomagnetic investigations on the Deccan Traps have been successful in strengthening the plate-tectonic theory as well as establishing the magnetostratigraphy of the flow sequence permitting constraints on the ages and span of eruption of the flows. From the compilation of the available good quality palaeomagnetic data on the flows, Vandamme et al. (1991) proposed a normal-reversenormal polarity sequence that correspond to the chrons 30 N-29 R-29 N; a major part of the eruptions is limited to the chron 29 R. From detailed geochronological studies on the 2.5 km thick lava pile in the Western Ghats, Duncan and Pyle (1988) have suggested the age to be 67.4±0.7 Ma as compared to 65.5±2.5 Ma reported by Vandamme et al. (1991). In both these studies, a short duration of less than 1 Ma long has been proposed for the Deccan Traps. Recent 40Ar/39 Ar dating of mineral separates and whole rocks from the Western Ghats lava pile, has reinforced these views by (Hofmann et al., 2000). In contrast, Venkatesan et al. (1993, 1994) suggested the flow duration to be not less than 3 Ma with eruption pre-dating the KTB by at least 1.0 Ma. Dhandapani and Subbarao (1992) had also favored a longer duration of more than 6 Ma for the Deccan flows by identifying normal polarity in the lowermost Deccan flow coinciding with the Cretaceous Long Normal Superchron. Most of the rock magnetic and palaeomagnetic studies till date have focused on measurements from different lava flows. In order to have a better understanding of the Deccan volcanic episode, in particular, the precise age, span and mechanism of eruption as well as the original extent of the Deccan Province, it is desirable to extend palaeomagnetic studies to the associated intrusive phases. There are only three published palaeomagnetic reports on the Deccan traps dykes -(i) Mandaleshwar dykes in the south of Narmada river (Subbarao et al., 1988), (ii) Dhadgaon and Nandurbar dykes respectively from the south of Narmada and Tapti rivers (Prasad et al., 1996) and (iii) Goa dykes, which exist around 70 km beyond the present day southern margin of the Deccan Province, along the west coast of India (Patil and Rao, 2002). Besides these three reports, Radhakrishna et al. (1994) have studied the central Kerala dykes, based on palaeomagnetic and 40Ar/39 Ar ages (69±1 Ma), as the feeders to the Deccan volcanic Patil, S.K. and Arora, B.R. 2003. Palaeomagnetic Studies on the Dykes of Mumbai Region, West Coast of Deccan Volcanic Province: Implications on Age and Span of the Deccan Eruptions. Journal of the Virtual Explorer 12, 107-116. Patil and Arora, 2003. Journal of the Virtual Explorer 12, 107-116 107 sequences and suggested that the Deccan eruptions were widespread and extended southward into Central Kerala. The most prominent region of Deccan Traps Province, the Western Ghat Section, where flows yielded good quality palaeomagnetic, isotopic dates and geochemical data sets, is lacking in detailed palaeomagnetic studies on the intrusive bodies. Only one report by Subbarao et al. (1992) identifying the dyke polarities is available to the best of authors” knowledge. However, at present palaeomagnetic and geochemical investigations along with geochronological studies are initiated on the dykes and recently Sahu et al. (2003) have presented 87 Rb/86 Sr ages and Sr isotopic composition of alkaline dykes near Mumbai. In this present article, we have reported new palaeomagnetic results from the dykes along the West Coast, south of Mumbai (Bombay), and compared the results with those of the previous studies for constraining the age and duration of the Deccan trap flows and also discussed their genetic relation with the flows. GEOLOGY OF THE STUDY AREA Mafic dykes are concentrated in clusters and swarms in the two tectonic belts paralleling the N-S trending West Coast and Sahyadri Mountains and E-W trending Narmada-Tapti-Satpura lineament zones in the Deccan volcanic province (Figure 1). According to Deshmukh and Sehgal (1988) dyke swarms cover areas of 32,500 km2 and 87,000 km2 in the Narmada-Tapti and West Coast belts respectively. These dykes are mainly dolerites of tholeiitic character and they occupy dilatory tensional fractures, which are formed due to tectonic movements in the two tectonic belts. The Murud region, the present study area (Figure 2), lies in the Konkan Coastal belt of the Western Ghat Section, and is predominantly covered by flows of Poladpur and Ambenalli Formations of Wai Subgroup of the Deccan Basalts (Subbarao and Hooper, 1988). Powar and Vadetwar (1995) identify these flows as simple and compound types that range in thickness from about 5m to 40m or more. The “Panvel Flexure” is the most prominent tectonic feature in this region (Auden, 1949). In this area tholeiitic to mildly alkaline flows of Deccan basalts are intruded by a number of basic (dolerite) dykes associated with plugs of gabbrodiorite. The dykes of this region are mostly oriented N-S, parallel to the “Panvel lineament”. According to Powar and Vadetwar (1995), over 32% of the dykes occur in the azimuth range N 0-9° and nearly 60% in the range N 030°. The dykes show sharp contacts with the basalts and have chilled margins. The dykes are vertical or steeply inclined up to 70°. Based on their field characteristics, Dessai and Viegas (1995) distinguished these dykes into four generations. Powar and Vadetwar (1995) observed close similarity in the mineralogy and chemistry of basalts and dolerite dykes of this region and suggested that both dykes and flows represent the Poladpur magma-type. They also opined that the dykes were emplaced immediately after the outpouring of basalts of Poladpur Formation, but are not the feeders to the flows. SAMPLING AND MEASUREMENTS 35 oriented block samples were collected from 5 dolerite dykes (4 dykes, RID 1 to 4, belong to south of Rat Island, 1 dyke (TBD-1) from north-west of Borlai (Figure2b) and 1 lamprophyre dyke (ELD-1) from Beacon Hill region (Figure 2-c). It has been taken care that minimum 5 samples from each dyke was collected. Rat Island dykes trend N10°W and their widths range from 1 to 2 m. Borlai dyke trends N50°W and has the width of around 2.5 m, whereas, Beacon Hill lamprophyre dyke trends NNESSW direction with a width of 3 m. From the collected 35 samples around 160 standard cylindrical specimens of size 2.2 cm height and 2.5 cm diameter were prepared in the laboratory. The Natural Remanent Magnetization (NRM) intensities of all the prepared specimens were measured with JR-5A Spinner magnetometer (M/S Agico, Czech Republic) having the sensitivity of 3 pT. NRM intensities of dolerite dyke specimens were in the range of 0.22 to 3.31 A/m, whereas, lamprophyre dyke specimens were in the range of 0.60 to 1.19 A/m. The magnetic susceptibilities were measured by MS-2B Bartington susceptibility meter. The magnetic susceptibilities of dolerite and lamprophyre dyke specimens were in the ranges of (1599 – 5932) x 10-5 SI and (11610 – 12220) x10-5 SI respectively. Koenigsberger (Qn) ratios were calculated and it was noticed that the dolerite specimens had relatively higher values (mean=0.68) than those of lamprophyre dykes specimens (mean=0.20). Both the alternating field (AF) and thermal demagnetization methods were used to isolate the characteristic remanent magnetization (ChRM) directions from the specimens. For the AF demagnetizations M/S. Molspin AF demagnetizer was used and for the thermal demagnetizations, MAVACS system manufactured by Geofyzica, Brono, was used. Initially 36 specimens representing 6 dykes ","PeriodicalId":201383,"journal":{"name":"Journal of The Virtual Explorer","volume":"49 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2003-01-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"3","resultStr":"{\"title\":\"Palaeomagnetic studies on the dykes of Mumbai region, West coast of deccan volcanic province: implications on age and Span of the deccan Eruptions\",\"authors\":\"S. Patil, B. Arora\",\"doi\":\"10.3809/JVIRTEX.2003.00077\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Through detailed AF and thermal demagnetizations of 35 samples (161 specimens) collected from 6 dykes located at Murud region, south of Mumbai, we report the first mean characteristic remanent magnetization direction as D=341°; I= -42°(μ95=5.7; N=6 dykes) for the dykes intruded into the West Coast zone of the Deccan Volcanic Province. The virtual geomagnetic pole (VGP) position (44°N; 83°W; A95=5.8°; N=6 dykes) calculated from this study is compared with those of the Narmada-Tapti zone dykes and with the Deccan Super Pole, proposed by Vandamme et al. (1991). Based on the concordance of these poles and recently reported 40Ar/39Ar and 87Rb/86Sr dates on the dykes of the studied region (Murud), it is proposed that the entire Deccan flows and the associated dykes were erupted in a short interval close to the Cretaceous-Tertiary Boundary at 65.5 Ma. Thermal demagnetization spectra along with isothermal remanent magnetizations and LF test experiments indicated that the SD type titano-magnetite was the major ChRM carrying magnetic mineral in the samples. Out of the 6 studied dykes, one dolerite dyke showing the “reverse magnetic polarity”, could have acted as a feeder dyke to the Poladpur Formation flows, which host the dykes in the studied area. The remaining four dolerite dykes and one lamprophyre dyke, yielding “normal polarity” directions, might have fed to the youngest formations of Wai Subgroup flows, viz., Panhala Formation and Desur Formation, which were eroded in the studied region. INTRODUCTION It is a widely accepted view that the Deccan flood basalts of Indian sub-continent, covering at present an area of 500,000 sq.km., is the result of outburst of immense magma material from the Reunion Hot spot source that impinged on the northerly drifting Indian lithosphere in the Late Cretaceous (Morgan, 1981). The Deccan Province is traversed by three major rift zones, namely the Narmada-Tapti-Son rift, the Cambay rift and the West Coast rift, which form a triple junction at the CambayBasin (Sheth and Chandrashekharam, 1997). Over the last 30 years the Deccan Traps have attained the attention of geochronologists, palaeomagnetists, geochemists and petrologists alike with its impressive horizontal lava piles, enormous size and volume along with its rapid eruptions at the K/T boundary coinciding with the much debated mass extinctions (Sen, 2001; Subbarao, 1999a and 1999b). Palaeomagnetic investigations on the Deccan Traps have been successful in strengthening the plate-tectonic theory as well as establishing the magnetostratigraphy of the flow sequence permitting constraints on the ages and span of eruption of the flows. From the compilation of the available good quality palaeomagnetic data on the flows, Vandamme et al. (1991) proposed a normal-reversenormal polarity sequence that correspond to the chrons 30 N-29 R-29 N; a major part of the eruptions is limited to the chron 29 R. From detailed geochronological studies on the 2.5 km thick lava pile in the Western Ghats, Duncan and Pyle (1988) have suggested the age to be 67.4±0.7 Ma as compared to 65.5±2.5 Ma reported by Vandamme et al. (1991). In both these studies, a short duration of less than 1 Ma long has been proposed for the Deccan Traps. Recent 40Ar/39 Ar dating of mineral separates and whole rocks from the Western Ghats lava pile, has reinforced these views by (Hofmann et al., 2000). In contrast, Venkatesan et al. (1993, 1994) suggested the flow duration to be not less than 3 Ma with eruption pre-dating the KTB by at least 1.0 Ma. Dhandapani and Subbarao (1992) had also favored a longer duration of more than 6 Ma for the Deccan flows by identifying normal polarity in the lowermost Deccan flow coinciding with the Cretaceous Long Normal Superchron. Most of the rock magnetic and palaeomagnetic studies till date have focused on measurements from different lava flows. In order to have a better understanding of the Deccan volcanic episode, in particular, the precise age, span and mechanism of eruption as well as the original extent of the Deccan Province, it is desirable to extend palaeomagnetic studies to the associated intrusive phases. There are only three published palaeomagnetic reports on the Deccan traps dykes -(i) Mandaleshwar dykes in the south of Narmada river (Subbarao et al., 1988), (ii) Dhadgaon and Nandurbar dykes respectively from the south of Narmada and Tapti rivers (Prasad et al., 1996) and (iii) Goa dykes, which exist around 70 km beyond the present day southern margin of the Deccan Province, along the west coast of India (Patil and Rao, 2002). Besides these three reports, Radhakrishna et al. (1994) have studied the central Kerala dykes, based on palaeomagnetic and 40Ar/39 Ar ages (69±1 Ma), as the feeders to the Deccan volcanic Patil, S.K. and Arora, B.R. 2003. Palaeomagnetic Studies on the Dykes of Mumbai Region, West Coast of Deccan Volcanic Province: Implications on Age and Span of the Deccan Eruptions. Journal of the Virtual Explorer 12, 107-116. Patil and Arora, 2003. Journal of the Virtual Explorer 12, 107-116 107 sequences and suggested that the Deccan eruptions were widespread and extended southward into Central Kerala. The most prominent region of Deccan Traps Province, the Western Ghat Section, where flows yielded good quality palaeomagnetic, isotopic dates and geochemical data sets, is lacking in detailed palaeomagnetic studies on the intrusive bodies. Only one report by Subbarao et al. (1992) identifying the dyke polarities is available to the best of authors” knowledge. However, at present palaeomagnetic and geochemical investigations along with geochronological studies are initiated on the dykes and recently Sahu et al. (2003) have presented 87 Rb/86 Sr ages and Sr isotopic composition of alkaline dykes near Mumbai. In this present article, we have reported new palaeomagnetic results from the dykes along the West Coast, south of Mumbai (Bombay), and compared the results with those of the previous studies for constraining the age and duration of the Deccan trap flows and also discussed their genetic relation with the flows. GEOLOGY OF THE STUDY AREA Mafic dykes are concentrated in clusters and swarms in the two tectonic belts paralleling the N-S trending West Coast and Sahyadri Mountains and E-W trending Narmada-Tapti-Satpura lineament zones in the Deccan volcanic province (Figure 1). According to Deshmukh and Sehgal (1988) dyke swarms cover areas of 32,500 km2 and 87,000 km2 in the Narmada-Tapti and West Coast belts respectively. These dykes are mainly dolerites of tholeiitic character and they occupy dilatory tensional fractures, which are formed due to tectonic movements in the two tectonic belts. The Murud region, the present study area (Figure 2), lies in the Konkan Coastal belt of the Western Ghat Section, and is predominantly covered by flows of Poladpur and Ambenalli Formations of Wai Subgroup of the Deccan Basalts (Subbarao and Hooper, 1988). Powar and Vadetwar (1995) identify these flows as simple and compound types that range in thickness from about 5m to 40m or more. The “Panvel Flexure” is the most prominent tectonic feature in this region (Auden, 1949). In this area tholeiitic to mildly alkaline flows of Deccan basalts are intruded by a number of basic (dolerite) dykes associated with plugs of gabbrodiorite. The dykes of this region are mostly oriented N-S, parallel to the “Panvel lineament”. According to Powar and Vadetwar (1995), over 32% of the dykes occur in the azimuth range N 0-9° and nearly 60% in the range N 030°. The dykes show sharp contacts with the basalts and have chilled margins. The dykes are vertical or steeply inclined up to 70°. Based on their field characteristics, Dessai and Viegas (1995) distinguished these dykes into four generations. Powar and Vadetwar (1995) observed close similarity in the mineralogy and chemistry of basalts and dolerite dykes of this region and suggested that both dykes and flows represent the Poladpur magma-type. They also opined that the dykes were emplaced immediately after the outpouring of basalts of Poladpur Formation, but are not the feeders to the flows. SAMPLING AND MEASUREMENTS 35 oriented block samples were collected from 5 dolerite dykes (4 dykes, RID 1 to 4, belong to south of Rat Island, 1 dyke (TBD-1) from north-west of Borlai (Figure2b) and 1 lamprophyre dyke (ELD-1) from Beacon Hill region (Figure 2-c). It has been taken care that minimum 5 samples from each dyke was collected. Rat Island dykes trend N10°W and their widths range from 1 to 2 m. Borlai dyke trends N50°W and has the width of around 2.5 m, whereas, Beacon Hill lamprophyre dyke trends NNESSW direction with a width of 3 m. From the collected 35 samples around 160 standard cylindrical specimens of size 2.2 cm height and 2.5 cm diameter were prepared in the laboratory. The Natural Remanent Magnetization (NRM) intensities of all the prepared specimens were measured with JR-5A Spinner magnetometer (M/S Agico, Czech Republic) having the sensitivity of 3 pT. NRM intensities of dolerite dyke specimens were in the range of 0.22 to 3.31 A/m, whereas, lamprophyre dyke specimens were in the range of 0.60 to 1.19 A/m. The magnetic susceptibilities were measured by MS-2B Bartington susceptibility meter. The magnetic susceptibilities of dolerite and lamprophyre dyke specimens were in the ranges of (1599 – 5932) x 10-5 SI and (11610 – 12220) x10-5 SI respectively. Koenigsberger (Qn) ratios were calculated and it was noticed that the dolerite specimens had relatively higher values (mean=0.68) than those of lamprophyre dykes specimens (mean=0.20). Both the alternating field (AF) and thermal demagnetization methods were used to isolate the characteristic remanent magnetization (ChRM) directions from the specimens. For the AF demagnetizations M/S. Molspin AF demagnetizer was used and for the thermal demagnetizations, MAVACS system manufactured by Geofyzica, Brono, was used. 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引用次数: 3
摘要
通过对孟买南部Murud地区6个岩脉采集的35个样品(161个标本)的AF和热退磁详细分析,得出第一平均特征剩磁方向为D=341°;我= -42°(μ95 = 5.7;N=6条岩脉)为侵入德干火山省西海岸带的岩脉。虚拟地磁极(VGP)位置(44°N;83°W;来说= 5.8°;并与Vandamme et al.(1991)提出的Narmada-Tapti带岩脉和德干超级极(Deccan Super Pole)进行了比较。根据这些极点的一致性和最近报道的研究区(Murud)岩脉上的40Ar/39Ar和87Rb/86Sr测年,认为整个德干流及其相关岩脉是在65.5 Ma白垩纪-第三纪界线附近的短间隔内爆发的。热退磁谱、等温剩余磁化和LF测试实验表明,SD型钛磁铁矿是样品中主要的载磁矿物。在研究的6条岩脉中,有一条白云岩岩脉显示“反向磁极性”,可能是Poladpur组流体的馈线岩脉,该岩脉承载了研究区域的岩脉。其余4条白云岩岩脉和1条煌斑岩岩脉,呈“正极性”方向,可能与围亚群最年轻的Panhala组和Desur组相对应,并在研究区内被侵蚀。人们普遍认为,印度次大陆的德干洪水玄武岩目前覆盖了50万平方公里的面积。,是晚白垩世留尼旺热点源巨大岩浆物质撞击向北漂移的印度岩石圈爆发的结果(Morgan, 1981)。德干省被三个主要裂谷带所穿越,即Narmada-Tapti-Son裂谷、Cambay裂谷和西海岸裂谷,它们在CambayBasin形成了一个三重交界处(Sheth and Chandrashekharam, 1997)。在过去的30年里,德干圈闭已经引起了地质年代学家、古地磁学家、地球化学家和岩石学家的注意,因为它令人印象深刻的水平熔岩堆,巨大的规模和体积,以及它在K/T边界的快速喷发,与备受争议的大灭绝相吻合(Sen, 2001;Subbarao, 1999a和1999b)。德干圈闭的古地磁研究成功地加强了板块构造理论,并建立了流体层序的磁地层学,从而限制了流体喷发的年龄和跨度。Vandamme et al.(1991)利用现有的高质量古地磁资料,提出了对应于30 N-29 R-29 N的正—反正极性序列;根据对西高止山脉2.5公里厚熔岩堆的详细地质年代学研究,Duncan和Pyle(1988)认为其年龄为67.4±0.7 Ma,而Vandamme等人(1991)报告的年龄为65.5±2.5 Ma。在这两项研究中,都提出德干圈闭的持续时间短于1 Ma。最近对来自西高止山脉熔岩堆的矿物分离物和整块岩石进行的40Ar/ 39ar测年,通过(Hofmann et al, 2000)加强了这些观点。相比之下,Venkatesan等人(1993,1994)认为水流持续时间不少于3 Ma,喷发时间至少比KTB早1.0 Ma。Dhandapani和Subbarao(1992)也通过确定与白垩纪长正超时相吻合的最下层德干流的正极性,认为德干流的持续时间超过6 Ma。迄今为止,大多数岩石地磁和古地磁研究都集中在不同熔岩流的测量上。为了更好地认识德干火山事件,特别是精确的喷发年龄、喷发跨度和喷发机制以及德干省的原始范围,有必要将古地磁研究扩展到与之相关的侵入期。关于德干圈闭岩脉的古地磁报告只有三篇——(i)纳尔马达河南部的Mandaleshwar岩脉(Subbarao et al., 1988), (ii)分别位于纳尔马达河和塔普提河南部的Dhadgaon和Nandurbar岩脉(Prasad et al., 1996),以及(iii)果阿岩脉,位于今天的德干省南缘以外约70公里处,沿着印度西海岸(Patil和Rao, 2002)。Radhakrishna et al.(1994)根据古地磁年龄和40Ar/ 39ar年龄(69±1 Ma)研究了喀拉拉邦中部岩脉作为德干火山Patil, S.K.和Arora, B.R. 2003的供给源。德干火山省西海岸孟买地区岩脉的古地磁研究:对德干火山喷发年龄和跨度的启示。
Palaeomagnetic studies on the dykes of Mumbai region, West coast of deccan volcanic province: implications on age and Span of the deccan Eruptions
Through detailed AF and thermal demagnetizations of 35 samples (161 specimens) collected from 6 dykes located at Murud region, south of Mumbai, we report the first mean characteristic remanent magnetization direction as D=341°; I= -42°(μ95=5.7; N=6 dykes) for the dykes intruded into the West Coast zone of the Deccan Volcanic Province. The virtual geomagnetic pole (VGP) position (44°N; 83°W; A95=5.8°; N=6 dykes) calculated from this study is compared with those of the Narmada-Tapti zone dykes and with the Deccan Super Pole, proposed by Vandamme et al. (1991). Based on the concordance of these poles and recently reported 40Ar/39Ar and 87Rb/86Sr dates on the dykes of the studied region (Murud), it is proposed that the entire Deccan flows and the associated dykes were erupted in a short interval close to the Cretaceous-Tertiary Boundary at 65.5 Ma. Thermal demagnetization spectra along with isothermal remanent magnetizations and LF test experiments indicated that the SD type titano-magnetite was the major ChRM carrying magnetic mineral in the samples. Out of the 6 studied dykes, one dolerite dyke showing the “reverse magnetic polarity”, could have acted as a feeder dyke to the Poladpur Formation flows, which host the dykes in the studied area. The remaining four dolerite dykes and one lamprophyre dyke, yielding “normal polarity” directions, might have fed to the youngest formations of Wai Subgroup flows, viz., Panhala Formation and Desur Formation, which were eroded in the studied region. INTRODUCTION It is a widely accepted view that the Deccan flood basalts of Indian sub-continent, covering at present an area of 500,000 sq.km., is the result of outburst of immense magma material from the Reunion Hot spot source that impinged on the northerly drifting Indian lithosphere in the Late Cretaceous (Morgan, 1981). The Deccan Province is traversed by three major rift zones, namely the Narmada-Tapti-Son rift, the Cambay rift and the West Coast rift, which form a triple junction at the CambayBasin (Sheth and Chandrashekharam, 1997). Over the last 30 years the Deccan Traps have attained the attention of geochronologists, palaeomagnetists, geochemists and petrologists alike with its impressive horizontal lava piles, enormous size and volume along with its rapid eruptions at the K/T boundary coinciding with the much debated mass extinctions (Sen, 2001; Subbarao, 1999a and 1999b). Palaeomagnetic investigations on the Deccan Traps have been successful in strengthening the plate-tectonic theory as well as establishing the magnetostratigraphy of the flow sequence permitting constraints on the ages and span of eruption of the flows. From the compilation of the available good quality palaeomagnetic data on the flows, Vandamme et al. (1991) proposed a normal-reversenormal polarity sequence that correspond to the chrons 30 N-29 R-29 N; a major part of the eruptions is limited to the chron 29 R. From detailed geochronological studies on the 2.5 km thick lava pile in the Western Ghats, Duncan and Pyle (1988) have suggested the age to be 67.4±0.7 Ma as compared to 65.5±2.5 Ma reported by Vandamme et al. (1991). In both these studies, a short duration of less than 1 Ma long has been proposed for the Deccan Traps. Recent 40Ar/39 Ar dating of mineral separates and whole rocks from the Western Ghats lava pile, has reinforced these views by (Hofmann et al., 2000). In contrast, Venkatesan et al. (1993, 1994) suggested the flow duration to be not less than 3 Ma with eruption pre-dating the KTB by at least 1.0 Ma. Dhandapani and Subbarao (1992) had also favored a longer duration of more than 6 Ma for the Deccan flows by identifying normal polarity in the lowermost Deccan flow coinciding with the Cretaceous Long Normal Superchron. Most of the rock magnetic and palaeomagnetic studies till date have focused on measurements from different lava flows. In order to have a better understanding of the Deccan volcanic episode, in particular, the precise age, span and mechanism of eruption as well as the original extent of the Deccan Province, it is desirable to extend palaeomagnetic studies to the associated intrusive phases. There are only three published palaeomagnetic reports on the Deccan traps dykes -(i) Mandaleshwar dykes in the south of Narmada river (Subbarao et al., 1988), (ii) Dhadgaon and Nandurbar dykes respectively from the south of Narmada and Tapti rivers (Prasad et al., 1996) and (iii) Goa dykes, which exist around 70 km beyond the present day southern margin of the Deccan Province, along the west coast of India (Patil and Rao, 2002). Besides these three reports, Radhakrishna et al. (1994) have studied the central Kerala dykes, based on palaeomagnetic and 40Ar/39 Ar ages (69±1 Ma), as the feeders to the Deccan volcanic Patil, S.K. and Arora, B.R. 2003. Palaeomagnetic Studies on the Dykes of Mumbai Region, West Coast of Deccan Volcanic Province: Implications on Age and Span of the Deccan Eruptions. Journal of the Virtual Explorer 12, 107-116. Patil and Arora, 2003. Journal of the Virtual Explorer 12, 107-116 107 sequences and suggested that the Deccan eruptions were widespread and extended southward into Central Kerala. The most prominent region of Deccan Traps Province, the Western Ghat Section, where flows yielded good quality palaeomagnetic, isotopic dates and geochemical data sets, is lacking in detailed palaeomagnetic studies on the intrusive bodies. Only one report by Subbarao et al. (1992) identifying the dyke polarities is available to the best of authors” knowledge. However, at present palaeomagnetic and geochemical investigations along with geochronological studies are initiated on the dykes and recently Sahu et al. (2003) have presented 87 Rb/86 Sr ages and Sr isotopic composition of alkaline dykes near Mumbai. In this present article, we have reported new palaeomagnetic results from the dykes along the West Coast, south of Mumbai (Bombay), and compared the results with those of the previous studies for constraining the age and duration of the Deccan trap flows and also discussed their genetic relation with the flows. GEOLOGY OF THE STUDY AREA Mafic dykes are concentrated in clusters and swarms in the two tectonic belts paralleling the N-S trending West Coast and Sahyadri Mountains and E-W trending Narmada-Tapti-Satpura lineament zones in the Deccan volcanic province (Figure 1). According to Deshmukh and Sehgal (1988) dyke swarms cover areas of 32,500 km2 and 87,000 km2 in the Narmada-Tapti and West Coast belts respectively. These dykes are mainly dolerites of tholeiitic character and they occupy dilatory tensional fractures, which are formed due to tectonic movements in the two tectonic belts. The Murud region, the present study area (Figure 2), lies in the Konkan Coastal belt of the Western Ghat Section, and is predominantly covered by flows of Poladpur and Ambenalli Formations of Wai Subgroup of the Deccan Basalts (Subbarao and Hooper, 1988). Powar and Vadetwar (1995) identify these flows as simple and compound types that range in thickness from about 5m to 40m or more. The “Panvel Flexure” is the most prominent tectonic feature in this region (Auden, 1949). In this area tholeiitic to mildly alkaline flows of Deccan basalts are intruded by a number of basic (dolerite) dykes associated with plugs of gabbrodiorite. The dykes of this region are mostly oriented N-S, parallel to the “Panvel lineament”. According to Powar and Vadetwar (1995), over 32% of the dykes occur in the azimuth range N 0-9° and nearly 60% in the range N 030°. The dykes show sharp contacts with the basalts and have chilled margins. The dykes are vertical or steeply inclined up to 70°. Based on their field characteristics, Dessai and Viegas (1995) distinguished these dykes into four generations. Powar and Vadetwar (1995) observed close similarity in the mineralogy and chemistry of basalts and dolerite dykes of this region and suggested that both dykes and flows represent the Poladpur magma-type. They also opined that the dykes were emplaced immediately after the outpouring of basalts of Poladpur Formation, but are not the feeders to the flows. SAMPLING AND MEASUREMENTS 35 oriented block samples were collected from 5 dolerite dykes (4 dykes, RID 1 to 4, belong to south of Rat Island, 1 dyke (TBD-1) from north-west of Borlai (Figure2b) and 1 lamprophyre dyke (ELD-1) from Beacon Hill region (Figure 2-c). It has been taken care that minimum 5 samples from each dyke was collected. Rat Island dykes trend N10°W and their widths range from 1 to 2 m. Borlai dyke trends N50°W and has the width of around 2.5 m, whereas, Beacon Hill lamprophyre dyke trends NNESSW direction with a width of 3 m. From the collected 35 samples around 160 standard cylindrical specimens of size 2.2 cm height and 2.5 cm diameter were prepared in the laboratory. The Natural Remanent Magnetization (NRM) intensities of all the prepared specimens were measured with JR-5A Spinner magnetometer (M/S Agico, Czech Republic) having the sensitivity of 3 pT. NRM intensities of dolerite dyke specimens were in the range of 0.22 to 3.31 A/m, whereas, lamprophyre dyke specimens were in the range of 0.60 to 1.19 A/m. The magnetic susceptibilities were measured by MS-2B Bartington susceptibility meter. The magnetic susceptibilities of dolerite and lamprophyre dyke specimens were in the ranges of (1599 – 5932) x 10-5 SI and (11610 – 12220) x10-5 SI respectively. Koenigsberger (Qn) ratios were calculated and it was noticed that the dolerite specimens had relatively higher values (mean=0.68) than those of lamprophyre dykes specimens (mean=0.20). Both the alternating field (AF) and thermal demagnetization methods were used to isolate the characteristic remanent magnetization (ChRM) directions from the specimens. For the AF demagnetizations M/S. Molspin AF demagnetizer was used and for the thermal demagnetizations, MAVACS system manufactured by Geofyzica, Brono, was used. Initially 36 specimens representing 6 dykes