<?xml version="1.0" encoding="utf-8" standalone="no"?>
<!DOCTYPE article SYSTEM "http://www.ocean-sci.net/inc/os/copernicus.dtd">
<article language="en">
	<journal>
		<journal_title>Ocean Science</journal_title>
		<journal_url>www.ocean-sci.net</journal_url>
		<issn>1812-0784</issn>
		<eissn>1812-0792</eissn>
		<volume_number>1</volume_number>
		<issue_number>1</issue_number>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/os-1-17-2005</doi>
	<article_url>http://www.ocean-sci.net/1/17/2005/</article_url>
	<abstract_html>http://www.ocean-sci.net/1/17/2005/os-1-17-2005.html</abstract_html>
	<fulltext_pdf>http://www.ocean-sci.net/1/17/2005/os-1-17-2005.pdf</fulltext_pdf>
	<start_page>17</start_page>
	<end_page>28</end_page>
	<publication_date>2005-05-10</publication_date>
	<article_title content_type="html">High sampling rate thermistor string observations at the slope of Great Meteor Seamount</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>H. van Haren</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>R. Groenewegen</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>M. Laan</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>B. Koster</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Royal Netherlands Institute for Sea Research (NIOZ), P.O. Box 59, 1790 AB Den Burg, The Netherlands</affiliation>
	</affiliations>
	<abstract content_type="html">A high sampling rate (1 Hz) thermistor string has been built to accommodate
the scientific need to accurately monitor high-frequency and vigorous
internal wave and overturning processes in the ocean. The thermistors and
their custom designed electronics can register temperature at an estimated
precision of about 0.001&amp;deg; C with a response time faster than 0.25 s
down to depths of 6000 m. With a quick in situ calibration using SBE 911 CTD
an absolute accuracy of 0.005&amp;deg; C is obtained. The present string
holds 128 sensors at 0.5 m intervals, which are all read-out within 0.5 s.
When sampling at 1 Hz, the batteries and the memory capacity of the recorder
allow for deployments of up to 2 weeks. In this paper, the instrument is
described in some detail. Its performance is illustrated with examples from
the first moored observations, which show Kelvin-Helmholtz overturning and
very high-frequency (Doppler-shifted) internal waves besides occasionally
large turbulent bores moving up the sloping side of Great Meteor Seamount,
Canary Basin, North-Atlantic Ocean.</abstract>
	<references>
	</references>
</article>

