<?xml version="1.0" encoding="utf-8" standalone="no"?>
<!DOCTYPE article SYSTEM "http://www.astrophys-space-sci-trans.net/inc/astra/copernicus.dtd">
<article language="en">
	<journal>
		<journal_title>Astrophysics and Space Sciences Transactions</journal_title>
		<journal_url>www.astrophys-space-sci-trans.net</journal_url>
		<issn>1810-6528</issn>
		<eissn>1810-6536</eissn>
		<volume_number>5</volume_number>
		<issue_number>1</issue_number>
		<publication_year>2009</publication_year>
	</journal>
	<doi>10.5194/astra-5-39-2009</doi>
	<article_url>http://www.astrophys-space-sci-trans.net/5/39/2009/</article_url>
	<abstract_html>http://www.astrophys-space-sci-trans.net/5/39/2009/astra-5-39-2009.html</abstract_html>
	<fulltext_pdf>http://www.astrophys-space-sci-trans.net/5/39/2009/astra-5-39-2009.pdf</fulltext_pdf>
	<start_page>39</start_page>
	<end_page>42</end_page>
	<publication_date>2009-09-11</publication_date>
	<article_title content_type="html">Shear driven waves in the induced magnetosphere of Mars: parameter dependence</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>U. V. Amerstorfer</name>
			<email>ute.amerstorfer@oeaw.ac.at</email>
		</author>
		<author numeration="2" affiliations="2">
			<name>H. Gunell</name>
		</author>
		<author numeration="3" affiliations="3">
			<name>N. V. Erkaev</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>H. K. Biernat</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Space Research Institute, Austrian Academy of Sciences,  Schmiedlstr. 6, 8042 Graz, Austria</affiliation>
		<affiliation numeration="2" content_type="html">Department of Physics, West Virginia University,  Morgantown, WV 26506-6315, USA</affiliation>
		<affiliation numeration="3" content_type="html">Institute of Computational Modelling, Russian Academy of Sciences, 660036 Krasnoyarsk-36, Russia</affiliation>
	</affiliations>
	<abstract content_type="html">Low frequency oscillations in the plasma in the induced magnetosphere
of Mars were recently measured by the Mars Express spacecraft. Velocity
shear was observed, and the plasma was shown to be Kelvin-Helmholtz
unstable. In this paper we examine the effects on the frequency and
growth rate of the instability when the parameters are varied around
the observed values. It is found that if the velocity shear is increased
by decreasing the velocity on the low velocity side, i.e. close to
the planet, the growth rate increases, while a frequency consistent
with the observations can be maintained. When finite Larmor radius
effects are included, the growth rate depends on the direction of the
vorticity and in the maximum case it is seen to increase substantially,
up to a factor of 50, for narrow shear layers. This does also increase
the frequency of the oscillations to a large extent.</abstract>
	<references>
		<reference numeration="1" content_type="text"> Amerstorfer, U V., Erkaev, N V., Langmayr, D., and Biernat,~H K.: On Kelvin Helmholtz instability due to the solar wind interaction with unmagnetized planets, Planet. Space Sci., 55, 1811–1816, \doi10.1016/j.pss.2007.01.015, 2007. </reference>
		<reference numeration="2" content_type="text"> Arshukova, I L., Erkaev, N V., Biernat, H K., and Vogl, D F.: Interchange instability of the Venusian ionopause, Adv. Space Res., 33, 182–186, \doi10.1016/j.asr.2003.04.015, 2004. </reference>
		<reference numeration="3" content_type="text"> Baranov, V B., Fahr, H J., and Ruderman, M S.: Investigation of macroscopic instabilities at the heliopause boundary surface, Astron. Astrophys., 261, 341–347, 1992. </reference>
		<reference numeration="4" content_type="text"> Biernat, H., Erkaev, N., Amerstorfer, U., Penz, T., and Lichtenegger, H.: Solar wind flow past Venus and its implications for the occurrence of the Kelvin-Helmholtz instability, Planet. Space Sci., 55, 1793–1803, \doi10.1016/j.pss.2007.01.006, 2007. </reference>
		<reference numeration="5" content_type="text"> Brace, L H., Theis, R F., and Hoegy, W R.: Plasma clouds above the ionopause of Venus and their implications, Planet. Space Sci., 30, 29–37, \doi10.1016/0032-0633(82)90069-1, 1982. </reference>
		<reference numeration="6" content_type="text"> Braginskii, S I.: Transport Processes in a Plasma, in: Reviews of\vadjust Plasma Physics, edited by Leontovich, M A., 1, 205–311, Consultants Bureau, New York, 1965. </reference>
		<reference numeration="7" content_type="text"> Espley, J R., Cloutier, P A., Brain, D A., Crider, D H., and Acuña,~ M H.: Observations of low-frequency magnetic oscillations in the Martian magnetosheath, magnetic pileup region, and tail, J. Geophys. Res., 109, A07 213, \doi10.1029/2003JA010193, 2004. </reference>
		<reference numeration="8" content_type="text"> Gunell, H., Amerstorfer, U V., Nilsson, H., Grima, C., Koepke,~M., Fränz,~ M., Winningham,~J D., Frahm,~R A., Sauvaud,~J.-A., Fedorov,~A., Erkaev,~N V., Biernat,~H K., Holmström,~M., Lundin,~R., and Barabash,~S.: Shear driven waves in the induced magnetosphere of Mars, Plasma Phys. Contr. F., 50, 074 018, \doi10.1088/0741-3335/50/7/074018, 2008. </reference>
		<reference numeration="9" content_type="text"> Huba, J D.: The Kelvin–Helmholtz instability: Finite Larmor radius magnetohydrodynamics, Geophys. Res. Lett., 23, 2907–2910, 1996. </reference>
		<reference numeration="10" content_type="text"> Lundin, R., Barabash, S., Andersson, H., Holmström, M., Grigoriev, A., Yamauchi, M., Sauvaud, J.-A., Fedorov, A., Budnik, E., Thocaven, J.-J., Winningham, D., Frahm, R., Scherrer,~J., Sharber,~J., Asamura,~K., Hayakawa,~H., Coates,~A., Linder,~D R., Curtis,~C., Hsieh,~K C., Sandel,~B R., Grande,~M., Carter,~M., Reading,~D H., Koskinen,~H., Kallio,~E., Riihela,~P., Schmidt,~W., Säles,~T., Kozyra,~J., Krupp,~N., Woch,~J., Luhmann,~J., McKenna-Lawler,~S., Cerulli-Irelli,~R., Orsini,~S., Maggi,~M., Mura,~A., Milillo,~A., Roelof,~E., Williams,~D., Livi,~S., Brandt,~P., Wurz,~P., and Bochsler,~P.: Solar Wind-Induced Atmospheric Erosion atMars: First Results from ASPERA-3 on Mars Express, Science, 305, 1933–1936, \doi10.1126/science.1101860, 2004. </reference>
		<reference numeration="11" content_type="text"> Penz, T., Erkaev, N V., Biernat, H K., Lammer, H., Amerstorfer,~U V., Gunell,~H., Kallio,~E., Barabash,~S., Orsini,~S., Milillo,~A., and Baumjohann,~W.: Ion loss on Mars caused by the Kelvin–Helmholtz instability, Planet. Space Sci., 52, 1157–1167, \doi10.1016/j.pss.2004.06.001, 2004. </reference>
		<reference numeration="12" content_type="text"> Penz, T., Arshukova, I L., Terada, N., Shinagawa, H., Erkaev, N V., Biernat, H K., and Lammer, H.: A comparison of magnetohydrodynamic instabilities at the Martian ionopause, Adv. Space Res., 36, 2049–2056, \doi10.1016/j.asr.2004.11.039, 2005. </reference>
		<reference numeration="13" content_type="text"> Russell, C T., Luhmann, J G., Elphic, R C., Scarf, F L., and Brace,~L H.: Magnetic field and plasma wave observations in a plasma cloud at Venus, Geophys. Res. Lett., 9, 45–48, 1982. </reference>
		<reference numeration="14" content_type="text"> Winningham,~J D., Frahm,~R A., Sharber,~J R., Coates,~A J., Linder,~D R., Soobiah,~Y., Kallio,~E., Espley,~J R., Lundin,~R., Barabash,~S., Holmström,~M., Andersson,~H., Yamauchi,~M., Grigoriev,~A., Scherrer,~J R., Jeffers,~S J., Kataria,~D O., Kozyra,~J U., Luhmann,~J G., Roelof,~E C., Williams,~D J., Livi,~S., Curtis,~C C., Hsieh,~K C., Sandel,~B R., Koskinen,~H., Säles,~T., Riihelä,~P., Schmidt,~W., Grande,~M., Carter,~M., Sauvaud,~J.-A., Fedorov,~A., Thocaven,~J.-J., McKenna-Lawler,~S., Orsini,~S., Cerulli-Irelli,~R., Maggi,~M., Wurz,~P., Bochsler,~P., Krupp,~N., Woch,~J., Fränz,~M., Asamura,~K., and Dierker,~C.: Electron oscillations in the induced martian magnetosphere, Icarus, 182, 360–370, \doi10.1016/j.icarus.2005.10.033, 2006. </reference>
		<reference numeration="15" content_type="text"> Wolff, R S., Goldstein, B E., and Yeates, C M.: The onset and development of Kelvin-Helmholtz instability at the Venus ionopause, J.\ Geophys. Res., 85, 7697–7707, 1980. </reference>
	</references>
</article>
