<?xml version="1.0" encoding="utf-8" standalone="no"?>
<!DOCTYPE article SYSTEM "http://www.adv-radio-sci.net/inc/ars/copernicus.dtd">
<article language="en">
	<journal>
		<journal_title>Advances in Radio Science</journal_title>
		<journal_url>www.adv-radio-sci.net</journal_url>
		<issn>1684-9965</issn>
		<eissn>1684-9973</eissn>
		<volume_number>1</volume_number>
		<volume_title>Kleinheubacher Berichte 2002</volume_title>
		<publication_year>2003</publication_year>
	</journal>
	<doi>10.5194/ars-1-329-2003</doi>
	<article_url>http://www.adv-radio-sci.net/1/329/2003/</article_url>
	<abstract_html>http://www.adv-radio-sci.net/1/329/2003/ars-1-329-2003.html</abstract_html>
	<fulltext_pdf>http://www.adv-radio-sci.net/1/329/2003/ars-1-329-2003.pdf</fulltext_pdf>
	<start_page>329</start_page>
	<end_page>333</end_page>
	<publication_date>2003-05-05</publication_date>
	<article_title content_type="html">Response of the Effelsberg 100m radio telescope to signals in the near-field at 24 GHz</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>K. Ruf</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>E. Fürst</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>K. Grypstra</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>J. Neidhöfer</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>M. Schumacher</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53111 Bonn</affiliation>
	</affiliations>
	<abstract content_type="html">Short range radar (SRR) for cars has been proposed
to operate over 5 GHz of bandwidth at the 24 GHz
ISM band. To estimate the level of interference from these
devices on radio telescopes, the near-field antenna pattern has
to be known. We report on new measurements with the Effelsberg
100 m radio telescope. These measurements were
performed with a transmitter set up at a distance of 1.7 km
from the telescope. The strength of the signal picked up by
the telescope sidelobes shows that the proposed SRR would
interfere with sensitive radio astronomical observations.</abstract>
	<references>
	</references>
</article>

