极地研究
極地研究
겁지연구
CHINESE JOURNAL OF POLAR RESEARCH
2014年
2期
177-185
,共9页
冯梅%安美建%安春雷%史贵涛%赵越%李院生%Douglas Wiens
馮梅%安美建%安春雷%史貴濤%趙越%李院生%Douglas Wiens
풍매%안미건%안춘뢰%사귀도%조월%리원생%Douglas Wiens
地壳厚度%接收函数%昆仑站%东南极%南极内陆科考
地殼厚度%接收函數%昆崙站%東南極%南極內陸科攷
지각후도%접수함수%곤륜참%동남겁%남겁내륙과고
crustal thickness%seismic station%Dome A%East Antarctica%Antarctic expedition
自第4个国际极地年2007/2008开始至2013年,中国南极内陆冰盖科考队相继在自南极大陆边缘的中山站至东南极地形最高点昆仑站(Dome A)一线进行了低温甚宽频地震观测。本文对7个天然地震台站数据进行了分析,提取了这些台站的S波接收函数,据此反演获得了这些台站下的地壳厚度分布。结果显示:随着纬度的升高,地壳厚度由大陆边缘的中山站下的约38 km逐渐增加至CHNB台下的58 km,随后又于CHNA台站下方减薄至47 km,然后快速增大到南极地形最高点昆仑站(Dome A)下的62 km。昆仑站或Dome A是南极大陆地壳最厚的地方。从中山站至昆仑站之间地壳厚度的变化与冰下地貌变化存在明显的相关性,它们都说明了从中山站至CHNB之间地壳构造相对均匀。在距昆仑站约200 km的CHNA台下的地壳厚度(约47 km)明显比临近台站地壳偏薄,这可能说明了甘伯采夫山脉地壳侧向变化较大,即其形成时所遭受的构造作用较复杂。
自第4箇國際極地年2007/2008開始至2013年,中國南極內陸冰蓋科攷隊相繼在自南極大陸邊緣的中山站至東南極地形最高點昆崙站(Dome A)一線進行瞭低溫甚寬頻地震觀測。本文對7箇天然地震檯站數據進行瞭分析,提取瞭這些檯站的S波接收函數,據此反縯穫得瞭這些檯站下的地殼厚度分佈。結果顯示:隨著緯度的升高,地殼厚度由大陸邊緣的中山站下的約38 km逐漸增加至CHNB檯下的58 km,隨後又于CHNA檯站下方減薄至47 km,然後快速增大到南極地形最高點昆崙站(Dome A)下的62 km。昆崙站或Dome A是南極大陸地殼最厚的地方。從中山站至昆崙站之間地殼厚度的變化與冰下地貌變化存在明顯的相關性,它們都說明瞭從中山站至CHNB之間地殼構造相對均勻。在距昆崙站約200 km的CHNA檯下的地殼厚度(約47 km)明顯比臨近檯站地殼偏薄,這可能說明瞭甘伯採伕山脈地殼側嚮變化較大,即其形成時所遭受的構造作用較複雜。
자제4개국제겁지년2007/2008개시지2013년,중국남겁내륙빙개과고대상계재자남겁대륙변연적중산참지동남겁지형최고점곤륜참(Dome A)일선진행료저온심관빈지진관측。본문대7개천연지진태참수거진행료분석,제취료저사태참적S파접수함수,거차반연획득료저사태참하적지각후도분포。결과현시:수착위도적승고,지각후도유대륙변연적중산참하적약38 km축점증가지CHNB태하적58 km,수후우우CHNA태참하방감박지47 km,연후쾌속증대도남겁지형최고점곤륜참(Dome A)하적62 km。곤륜참혹Dome A시남겁대륙지각최후적지방。종중산참지곤륜참지간지각후도적변화여빙하지모변화존재명현적상관성,타문도설명료종중산참지CHNB지간지각구조상대균균。재거곤륜참약200 km적CHNA태하적지각후도(약47 km)명현비림근태참지각편박,저가능설명료감백채부산맥지각측향변화교대,즉기형성시소조수적구조작용교복잡。
Since the 4th International Polar Year in 2007/2008 until 201 3,the Chinese have deployed cold-mode very-broadband seismic stations along the traverse from Zhongshan to Kunlun (Dome A),East Antarctica.Using obser-vations recorded by the stations,we retrieved the S-receiver functions of seven stations from seismic waveform data, and inverted them for crustal thicknesses beneath the stations using the receiver functions.The results show that the crustal thickness increases along the traverse from 38 km beneath Zhongshan Station to approximately 58 km be-neath EAGLE and CHNB.The thickness then decreases to 47 km beneath CHNA,and finally increases to 62 km beneath the highest point of Antarctica,at Kunlun Station (Dome A).This thickness variation is consistent with the bedrock surface variation along the path,and indicates that the tectonics between Zhongshan and CHNB are rel-atively homogeneous.The crustal thickness beneath Kunlun Station of Dome A is not only the largest in Antarctica, but is also substantially greater than that beneath the cratons of other continents.The crust beneath CHNA is ap-proximately 1 0 km thinner than at neighboring stations,which may be due to the short duration of observations at the station,and may indicate that the crustal structure lateral variation is very large beneath the Gamburtsev Subgla-cial Mountains.