The Holocene Mitchell Megafan, Gulf of Carpentaria, Australia
AbstractAs the world’s lowest and flattest continent, Australia exhibits numerous gently inclined topographic basins that have generated a large number of megafans. One of the most extensive contiguous arrays occurs on the western flank of Cape York Peninsula. These megafans are derived from a compl...
Gespeichert in:
1. Verfasser: | |
---|---|
Format: | Buchkapitel |
Sprache: | eng |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 241 |
---|---|
container_issue | |
container_start_page | 219 |
container_title | |
container_volume | |
creator | Lane, Tessa I. |
description | AbstractAs the world’s lowest and flattest continent, Australia exhibits numerous gently inclined topographic basins that have generated a large number of megafans. One of the most extensive contiguous arrays occurs on the western flank of Cape York Peninsula. These megafans are derived from a complex network of modern and ancient distributary channels that have debouched into the epicontinental seaway of the Gulf of Carpentaria since at least Pliocene times. The Mitchell megafan-delta represents the largest of these fans. In this case study we examine the modern processes and resulting sedimentary facies and architecture of a type example. Mapping, field exploration and chronologic investigations were used to characterise these channel-belt facies and to link them to specific forcing conditions. These Holocene surficial deposits are associated with a network of modern streams and recent palaeochannels overlying, and sometimes incised into, older, fine-grained, partially indurated Quaternary alluvium. Where present, the partially indurated alluvium restricts channel migration, thereby promoting anabranching as a means of channel adjustment. Additionally, channel-belt distribution, morphology and sediment infilling are strongly affected by marine backwater dynamics operating in the downstream reaches. This has had an overriding influence on the position of avulsion nodes and channel-belt distribution in this zone. |
doi_str_mv | 10.1017/9781108525923.015 |
format | Book Chapter |
fullrecord | <record><control><sourceid>cambridge</sourceid><recordid>TN_cdi_cambridge_corebooks_9781108525923_CN_bp_12</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><cupid>9781108525923_CN_bp_12</cupid><sourcerecordid>9781108525923_CN_bp_12</sourcerecordid><originalsourceid>FETCH-LOGICAL-c127t-dfee37cf8ff03b337a55611d27cfc29dd3f03502f881246f739d777f35019303</originalsourceid><addsrcrecordid>eNpVz7FOwzAUBVAjhASUfgCbP6ApfnZd2wNDFUGL1MKSoVvk2H5twMRVnP4_kYqQmJ7uGa7uI-QR2BwYqCejNADTkkvDxZyBvCL3f7C_voQFF0Ltb8k050_GGNdcasPuyHN1DHSTYnKhC3TXDu4YYqS7cLBouxldnyPShLS0_Sl0g-1bO6Orcx56G1v7QG7Qxhymv3dCqteXqtwU24_1W7naFg64GgqPIQjlUCMy0YxDrJRLAM9Hc9x4L0aXjKPWwBdLVMJ4pRSOBkYwMSFwqXX2u-lbfwi1S31oUvrK9b_36_K9bk41cPEDcQhNrQ</addsrcrecordid><sourcetype>Publisher</sourcetype><iscdi>true</iscdi><recordtype>book_chapter</recordtype></control><display><type>book_chapter</type><title>The Holocene Mitchell Megafan, Gulf of Carpentaria, Australia</title><source>Ebook Central Perpetual and DDA</source><creator>Lane, Tessa I.</creator><creatorcontrib>Lane, Tessa I.</creatorcontrib><description>AbstractAs the world’s lowest and flattest continent, Australia exhibits numerous gently inclined topographic basins that have generated a large number of megafans. One of the most extensive contiguous arrays occurs on the western flank of Cape York Peninsula. These megafans are derived from a complex network of modern and ancient distributary channels that have debouched into the epicontinental seaway of the Gulf of Carpentaria since at least Pliocene times. The Mitchell megafan-delta represents the largest of these fans. In this case study we examine the modern processes and resulting sedimentary facies and architecture of a type example. Mapping, field exploration and chronologic investigations were used to characterise these channel-belt facies and to link them to specific forcing conditions. These Holocene surficial deposits are associated with a network of modern streams and recent palaeochannels overlying, and sometimes incised into, older, fine-grained, partially indurated Quaternary alluvium. Where present, the partially indurated alluvium restricts channel migration, thereby promoting anabranching as a means of channel adjustment. Additionally, channel-belt distribution, morphology and sediment infilling are strongly affected by marine backwater dynamics operating in the downstream reaches. This has had an overriding influence on the position of avulsion nodes and channel-belt distribution in this zone.</description><identifier>ISBN: 110842337X</identifier><identifier>ISBN: 9781108423373</identifier><identifier>EISBN: 110852592X</identifier><identifier>EISBN: 9781108525923</identifier><identifier>DOI: 10.1017/9781108525923.015</identifier><language>eng</language><ispartof>Fluvial Megafans on Earth and Mars, 2023, p.219-241</ispartof><rights>Cambridge University Press & Assessment 2023</rights><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>779,780,784,793,27925</link.rule.ids></links><search><creatorcontrib>Lane, Tessa I.</creatorcontrib><title>The Holocene Mitchell Megafan, Gulf of Carpentaria, Australia</title><title>Fluvial Megafans on Earth and Mars</title><description>AbstractAs the world’s lowest and flattest continent, Australia exhibits numerous gently inclined topographic basins that have generated a large number of megafans. One of the most extensive contiguous arrays occurs on the western flank of Cape York Peninsula. These megafans are derived from a complex network of modern and ancient distributary channels that have debouched into the epicontinental seaway of the Gulf of Carpentaria since at least Pliocene times. The Mitchell megafan-delta represents the largest of these fans. In this case study we examine the modern processes and resulting sedimentary facies and architecture of a type example. Mapping, field exploration and chronologic investigations were used to characterise these channel-belt facies and to link them to specific forcing conditions. These Holocene surficial deposits are associated with a network of modern streams and recent palaeochannels overlying, and sometimes incised into, older, fine-grained, partially indurated Quaternary alluvium. Where present, the partially indurated alluvium restricts channel migration, thereby promoting anabranching as a means of channel adjustment. Additionally, channel-belt distribution, morphology and sediment infilling are strongly affected by marine backwater dynamics operating in the downstream reaches. This has had an overriding influence on the position of avulsion nodes and channel-belt distribution in this zone.</description><isbn>110842337X</isbn><isbn>9781108423373</isbn><isbn>110852592X</isbn><isbn>9781108525923</isbn><fulltext>true</fulltext><rsrctype>book_chapter</rsrctype><creationdate>2023</creationdate><recordtype>book_chapter</recordtype><sourceid/><recordid>eNpVz7FOwzAUBVAjhASUfgCbP6ApfnZd2wNDFUGL1MKSoVvk2H5twMRVnP4_kYqQmJ7uGa7uI-QR2BwYqCejNADTkkvDxZyBvCL3f7C_voQFF0Ltb8k050_GGNdcasPuyHN1DHSTYnKhC3TXDu4YYqS7cLBouxldnyPShLS0_Sl0g-1bO6Orcx56G1v7QG7Qxhymv3dCqteXqtwU24_1W7naFg64GgqPIQjlUCMy0YxDrJRLAM9Hc9x4L0aXjKPWwBdLVMJ4pRSOBkYwMSFwqXX2u-lbfwi1S31oUvrK9b_36_K9bk41cPEDcQhNrQ</recordid><startdate>20230430</startdate><enddate>20230430</enddate><creator>Lane, Tessa I.</creator><scope/></search><sort><creationdate>20230430</creationdate><title>The Holocene Mitchell Megafan, Gulf of Carpentaria, Australia</title><author>Lane, Tessa I.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c127t-dfee37cf8ff03b337a55611d27cfc29dd3f03502f881246f739d777f35019303</frbrgroupid><rsrctype>book_chapters</rsrctype><prefilter>book_chapters</prefilter><language>eng</language><creationdate>2023</creationdate><toplevel>online_resources</toplevel><creatorcontrib>Lane, Tessa I.</creatorcontrib></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Lane, Tessa I.</au><format>book</format><genre>bookitem</genre><ristype>CHAP</ristype><atitle>The Holocene Mitchell Megafan, Gulf of Carpentaria, Australia</atitle><btitle>Fluvial Megafans on Earth and Mars</btitle><date>2023-04-30</date><risdate>2023</risdate><spage>219</spage><epage>241</epage><pages>219-241</pages><isbn>110842337X</isbn><isbn>9781108423373</isbn><eisbn>110852592X</eisbn><eisbn>9781108525923</eisbn><abstract>AbstractAs the world’s lowest and flattest continent, Australia exhibits numerous gently inclined topographic basins that have generated a large number of megafans. One of the most extensive contiguous arrays occurs on the western flank of Cape York Peninsula. These megafans are derived from a complex network of modern and ancient distributary channels that have debouched into the epicontinental seaway of the Gulf of Carpentaria since at least Pliocene times. The Mitchell megafan-delta represents the largest of these fans. In this case study we examine the modern processes and resulting sedimentary facies and architecture of a type example. Mapping, field exploration and chronologic investigations were used to characterise these channel-belt facies and to link them to specific forcing conditions. These Holocene surficial deposits are associated with a network of modern streams and recent palaeochannels overlying, and sometimes incised into, older, fine-grained, partially indurated Quaternary alluvium. Where present, the partially indurated alluvium restricts channel migration, thereby promoting anabranching as a means of channel adjustment. Additionally, channel-belt distribution, morphology and sediment infilling are strongly affected by marine backwater dynamics operating in the downstream reaches. This has had an overriding influence on the position of avulsion nodes and channel-belt distribution in this zone.</abstract><doi>10.1017/9781108525923.015</doi><tpages>23</tpages></addata></record> |
fulltext | fulltext |
identifier | ISBN: 110842337X |
ispartof | Fluvial Megafans on Earth and Mars, 2023, p.219-241 |
issn | |
language | eng |
recordid | cdi_cambridge_corebooks_9781108525923_CN_bp_12 |
source | Ebook Central Perpetual and DDA |
title | The Holocene Mitchell Megafan, Gulf of Carpentaria, Australia |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-04T10%3A57%3A34IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-cambridge&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=bookitem&rft.atitle=The%20Holocene%20Mitchell%20Megafan,%20Gulf%20of%20Carpentaria,%20Australia&rft.btitle=Fluvial%20Megafans%20on%20Earth%20and%20Mars&rft.au=Lane,%20Tessa%20I.&rft.date=2023-04-30&rft.spage=219&rft.epage=241&rft.pages=219-241&rft.isbn=110842337X&rft.isbn_list=9781108423373&rft_id=info:doi/10.1017/9781108525923.015&rft_dat=%3Ccambridge%3E9781108525923_CN_bp_12%3C/cambridge%3E%3Curl%3E%3C/url%3E&rft.eisbn=110852592X&rft.eisbn_list=9781108525923&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rft_cupid=9781108525923_CN_bp_12&rfr_iscdi=true |