About: Kinetic instabilities in Mercury's magnetosphere: Three-dimensional simulation results

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rdf:type	skos:Concept http://linked.opendata.cz/ontology/domain/vavai/Vysledek
Description	A self-consistent global three-dimensional kinetic study of Mercury's magnetosphere is carried out examining waves and instabilities generated by ion temperature anisotropy and plasma flow. The overall structure of Mercury's upstream bow shock and magnetosheath are qualitatively very similar to those of Earth. Beam-generated long-wavelength oscillations are present upstream of Mercury's quasi-parallel bow shock, whereas large-amplitude mirror waves develop downstream of the quasi-parallel bow shock in the magnetosheath. A train of mirror waves forms also downstream of the quasi-perpendicular bow shock. A velocity shear near the magnetopause can lead to formation of vortex-like structures. The magnetospheric cavity close to the planet's equatorial plane is filled with ions much hotter than the solar wind protons. A drift-driven plasma belt close to the equator is present in the model and contains plasma with high-temperature anisotropy, and the loss cone for charged particles in this region is large. A self-consistent global three-dimensional kinetic study of Mercury's magnetosphere is carried out examining waves and instabilities generated by ion temperature anisotropy and plasma flow. The overall structure of Mercury's upstream bow shock and magnetosheath are qualitatively very similar to those of Earth. Beam-generated long-wavelength oscillations are present upstream of Mercury's quasi-parallel bow shock, whereas large-amplitude mirror waves develop downstream of the quasi-parallel bow shock in the magnetosheath. A train of mirror waves forms also downstream of the quasi-perpendicular bow shock. A velocity shear near the magnetopause can lead to formation of vortex-like structures. The magnetospheric cavity close to the planet's equatorial plane is filled with ions much hotter than the solar wind protons. A drift-driven plasma belt close to the equator is present in the model and contains plasma with high-temperature anisotropy, and the loss cone for charged particles in this region is large. (en)
Title	Kinetic instabilities in Mercury's magnetosphere: Three-dimensional simulation results Kinetic instabilities in Mercury's magnetosphere: Three-dimensional simulation results (en)
skos:prefLabel	Kinetic instabilities in Mercury's magnetosphere: Three-dimensional simulation results Kinetic instabilities in Mercury's magnetosphere: Three-dimensional simulation results (en)
skos:notation	RIV/68378289:_____/09:00337453!RIV10-AV0-68378289
http://linked.open...avai/riv/aktivita	P Z
http://linked.open...avai/riv/aktivity	P(IAA300030805), Z(AV0Z10030501), Z(AV0Z30420517)
http://linked.open...iv/cisloPeriodika	-
http://linked.open...vai/riv/dodaniDat	2010
http://linked.open...aciTvurceVysledku	Hellinger, Petr Herčík, David
http://linked.open.../riv/druhVysledku	J - Článek v odborném periodiku
http://linked.open...iv/duvernostUdaju	S - Úplné a pravdivé údaje nepodléhající ochraně podle zvláštních právních předpisů
http://linked.open...titaPredkladatele	Ústav fyziky atmosféry AV ČR, v. v. i.
http://linked.open...dnocenehoVysledku	321741
http://linked.open...ai/riv/idVysledku	RIV/68378289:_____/09:00337453
http://linked.open...riv/jazykVysledku	eng - angličtina
http://linked.open.../riv/klicovaSlova	Mercury; magnetosphere; instability; ion temperature anisotropy; plasma flow; magnetosheath (en)
http://linked.open.../riv/klicoveSlovo	ion temperature anisotropy Mercury instability magnetosphere plasma flow magnetosheath
http://linked.open...odStatuVydavatele	US - Spojené státy americké
http://linked.open...ontrolniKodProRIV	[71DD0369898E]
http://linked.open...i/riv/nazevZdroje	Geophysical Research Letters
http://linked.open...in/vavai/riv/obor	BL
http://linked.open...ichTvurcuVysledku	2 (xsd:int)
http://linked.open...cetTvurcuVysledku	6 (xsd:int)
http://linked.open...vavai/riv/projekt	Global Kinetic Simulations of the Mercurys magnetosphere
http://linked.open...UplatneniVysledku	2009
http://linked.open...v/svazekPeriodika	36
http://linked.open...iv/tvurceVysledku	Anderson, B. J. Hellinger, Petr Schriver, D. Slavin, J. A Trávníček, Pavel M. Herčík, David
http://linked.open...ain/vavai/riv/wos	000265101400001
http://linked.open...n/vavai/riv/zamer	Astronomie a astrofyzika Studium atmosférického obalu Země v interakci s pozemskými a kosmickými vlivy
issn	0094-8276
number of pages	5 (xsd:int)
is http://linked.open...avai/riv/vysledek of	Kinetic instabilities in Mercury's magnetosphere: Three-dimensional simulation results Kinetic instabilities in Mercury's magnetosphere: Three-dimensional simulation results Kinetic instabilities in Mercury's magnetosphere: Three-dimensional simulation results Kinetic instabilities in Mercury's magnetosphere: Three-dimensional simulation results

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