Transverse Dinaric zone of increased compression between the Kraški rob and Hrušica Regions, NE Microadria

Q3 Earth and Planetary Sciences
L. Placer, I. Rižnar, Ana Novak
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引用次数: 0

Abstract

The Kvarner fault divides the Microadria (Adria microplate, the Adria stable core) into the Po and Adria segments. The Istra block, which is sandwiched between the right-lateral Kvarner Fault and the left-lateral Sistiana Fault lies at the extreme eastern edge of the Po segment. Both faults run transversely to the Dinarides and reach their thrust boundary in the east. The Microadria has been moving towards the Dinarides since the Middle Miocene. The movement of the Istra block is exposed in relation to the neighbouring blocks, so an extensive pushed area (the Istra Pushed Area) was formed in the External Dinarides, which is bent towards the northeast. It is defined by two flexural zones, one lying in the extension of the Sistiana Fault and the other in the extension of the Kvarner Fault. The structure of the Dinaric thrust border on the north-eastern side of the Istra block is complex. Its prominent structural element is the Črni Kal Anomaly, due to which a zone of increased compression developed within the Istra Pushed Area and transversely to the Dinarides (Kraški rob – Hrušica Traverse), which lies between the Sistiana and Kvarner Flexural Zones. In terms of kinematics, it differs greatly from these two, and various geomorphologically responsive deformations have occurred within it. Mt. Vremščica (1027 m), which represents a transpressive anticline within the wider zone of the Raša Fault is the most prominent. In order to understand the genesis of the Classical Karst relief, it is important to know that the Mt. Vremščica ridge rose from the levelled karst surface.
东北微adria的Kraški rob和Hrušica区域之间的横向Dinaric区压缩增加
Kvarner断裂将Microadria(亚德里亚微板块,亚德里亚稳定核)划分为Po段和Adria段。Istra地块位于Po段的最东端,夹在右旋Kvarner断裂和左旋Sistiana断裂之间。两条断裂都横向延伸至迪纳里德斯,并在东部到达冲断边界。自中新世中期以来,微亚德里亚板块一直在向迪纳里德斯板块移动。伊斯特拉地块的运动相对于邻近的地块暴露出来,因此在外部Dinarides形成了一个广泛的推覆区(伊斯特拉推覆区),它向东北方向弯曲。它被定义为两个弯曲带,一个位于Sistiana断裂的伸展部,另一个位于Kvarner断裂的伸展部。伊斯特拉地块东北侧的迪纳里克逆冲边界构造复杂。其突出的构造元素是Črni Kal异常,由于该异常,在伊斯特拉推区和横向的Dinarides (Kraški rob - Hrušica Traverse)内发育了一个增加压缩的区域,该区域位于Sistiana和Kvarner弯曲带之间。在运动学方面,它与这两者有很大的不同,并且在它内部发生了各种地貌响应变形。其中Vremščica山(1027 m)最为突出,代表了Raša断裂较宽带内的一个逆压背斜。为了了解古典喀斯特地貌的成因,必须了解Vremščica山脊是在平整的喀斯特地表上隆起的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Geologija
Geologija Earth and Planetary Sciences-Geophysics
CiteScore
1.00
自引率
0.00%
发文量
10
审稿时长
10 weeks
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