海洋学报(中文版)
海洋學報(中文版)
해양학보(중문판)
ACTA OCEANOLOGICA SINICA
2014年
5期
177-185
,共9页
王昆山%石学法%吴永华%邹建军%姜晓黎
王昆山%石學法%吳永華%鄒建軍%薑曉黎
왕곤산%석학법%오영화%추건군%강효려
鄂霍次克海%岩心沉积物%重矿物%火山灰层%物质来源
鄂霍次剋海%巖心沉積物%重礦物%火山灰層%物質來源
악곽차극해%암심침적물%중광물%화산회층%물질래원
Okhotsk Sea%sediment core%heavy mineral%tephra%matter source
对鄂霍次克海东南部科学院隆起区 OS03-1岩心碎屑重矿物及火山灰层进行了详细分析。岩心重矿物以紫苏辉石、绿帘石和普通角闪石为主,特征矿物为钛磁铁矿和普通辉石,矿物特征表明本岩心的物质主要来源于冰筏搬运(陆源)和火山喷发。陆源物质大部分来源于鄂霍次克海西部和北部地区,少量来自堪察加半岛冰川携带沉积物;火山物质则来源于堪察加半岛和千岛群岛的火山喷发产物。在岩心中识别出3个火山灰层,各种证据表明火山灰层1与已知的K2火山灰层相同,形成年代为26 ka B P;火山灰层3具有明显火山物质与陆源物质混合特征,而火山灰层2则只能通过碎屑矿物的含量特征来判定,外在颜色不明显,已经明显的被陆源物质所稀释。研究表明,碎屑矿物组分参数可以有效地指示物质来源,也是识别火山灰层存在(特别是被陆源物质稀释)的可靠指标。
對鄂霍次剋海東南部科學院隆起區 OS03-1巖心碎屑重礦物及火山灰層進行瞭詳細分析。巖心重礦物以紫囌輝石、綠簾石和普通角閃石為主,特徵礦物為鈦磁鐵礦和普通輝石,礦物特徵錶明本巖心的物質主要來源于冰筏搬運(陸源)和火山噴髮。陸源物質大部分來源于鄂霍次剋海西部和北部地區,少量來自堪察加半島冰川攜帶沉積物;火山物質則來源于堪察加半島和韆島群島的火山噴髮產物。在巖心中識彆齣3箇火山灰層,各種證據錶明火山灰層1與已知的K2火山灰層相同,形成年代為26 ka B P;火山灰層3具有明顯火山物質與陸源物質混閤特徵,而火山灰層2則隻能通過碎屑礦物的含量特徵來判定,外在顏色不明顯,已經明顯的被陸源物質所稀釋。研究錶明,碎屑礦物組分參數可以有效地指示物質來源,也是識彆火山灰層存在(特彆是被陸源物質稀釋)的可靠指標。
대악곽차극해동남부과학원륭기구 OS03-1암심쇄설중광물급화산회층진행료상세분석。암심중광물이자소휘석、록렴석화보통각섬석위주,특정광물위태자철광화보통휘석,광물특정표명본암심적물질주요래원우빙벌반운(륙원)화화산분발。륙원물질대부분래원우악곽차극해서부화북부지구,소량래자감찰가반도빙천휴대침적물;화산물질칙래원우감찰가반도화천도군도적화산분발산물。재암심중식별출3개화산회층,각충증거표명화산회층1여이지적K2화산회층상동,형성년대위26 ka B P;화산회층3구유명현화산물질여륙원물질혼합특정,이화산회층2칙지능통과쇄설광물적함량특정래판정,외재안색불명현,이경명현적피륙원물질소희석。연구표명,쇄설광물조분삼수가이유효지지시물질래원,야시식별화산회층존재(특별시피륙원물질희석)적가고지표。
Composition and assemblage characteristics of heavy minerals were analyzed in core OS 03 -1 sediment collected from the Academy of Sciences Rise of southeastern Okhotsk Sea .The results show that the dominant minerals are hyperthene ,epidote and common hornblende ,and characteristic minerals are titanomagnetite and au-gite;the sediments are mostly ice-rafted debris (IRD) and volcanogenic matter .IRD were mainly derived from the western and northern Okhotsk Sea ,and a little from Kamchatka peninsula .Volcanogenic matter was mainly from Kamchatka Peninsula and Kurile Islands .Three tephra layers were identified .The first layer is characterized by special color ,grain size and mineral composition ,which was same to the well studied K2 tephra layer and deposited at 26.0 ka BP .The third layer could be recognized by color ,but was clearly diluted by terrigenous sediment .The second tephra layer couldn't be distinguished by color and grain size because of mixing with terrigenous sediment . T he study also show s that composition and assemblage of heavy minerals are both effective indicators of sediment sources ,and credible indentifying index of tephra ,especially those diluted by terrigenous matter .