About: Magnetic Reconnection in ICME Sheath

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rdf:type	skos:Concept http://linked.opendata.cz/ontology/domain/vavai/Vysledek
rdfs:seeAlso	http://www.mff.cuni.cz/veda/konference/wds/proc/pdf11/WDS11_202_f2_Enzl.pdf
Description	Magnetic reconnection is a phenomenon where the energy stored in magnetic field dissipates into heating and particle acceleration. It can occur on boundaries connecting plasma with different magnetic field topology. We can frequently find magnetic reconnection in ICME sheaths, where plasma is compressed and different plasma topologies encounter each other. In these regions we can recognize magnetic reconnection by number of plasma signatures such as temperature enhancement, or changes in magnetic field and bulk flow direction. A brief introduction into Interplanetary Coronal Mass Ejection (ICME), magnetic reconnection and its properties are presented and short statistics on shear angle dependence are provided. We have found dependence of temperature enhancement inside reconnection exhaust on shear angle. We have also obtained dependence of reconnection outflow speed on shear angle. Magnetic reconnection is a phenomenon where the energy stored in magnetic field dissipates into heating and particle acceleration. It can occur on boundaries connecting plasma with different magnetic field topology. We can frequently find magnetic reconnection in ICME sheaths, where plasma is compressed and different plasma topologies encounter each other. In these regions we can recognize magnetic reconnection by number of plasma signatures such as temperature enhancement, or changes in magnetic field and bulk flow direction. A brief introduction into Interplanetary Coronal Mass Ejection (ICME), magnetic reconnection and its properties are presented and short statistics on shear angle dependence are provided. We have found dependence of temperature enhancement inside reconnection exhaust on shear angle. We have also obtained dependence of reconnection outflow speed on shear angle. (en)
Title	Magnetic Reconnection in ICME Sheath Magnetic Reconnection in ICME Sheath (en)
skos:prefLabel	Magnetic Reconnection in ICME Sheath Magnetic Reconnection in ICME Sheath (en)
skos:notation	RIV/00216208:11320/11:10109844!RIV12-GA0-11320___
http://linked.open...avai/riv/aktivita	P S
http://linked.open...avai/riv/aktivity	P(GA205/07/0694), S
http://linked.open...vai/riv/dodaniDat	2012
http://linked.open...aciTvurceVysledku	Přech, Lubomír Lynnyk, Andrii Enžl, Jakub Grygorov, Kostiantyn
http://linked.open.../riv/druhVysledku	D - Článek ve sborníku
http://linked.open...iv/duvernostUdaju	S - Úplné a pravdivé údaje nepodléhající ochraně podle zvláštních právních předpisů
http://linked.open...titaPredkladatele	Univerzita Karlova v Praze / Matematicko-fyzikální fakulta
http://linked.open...dnocenehoVysledku	210230
http://linked.open...ai/riv/idVysledku	RIV/00216208:11320/11:10109844
http://linked.open...riv/jazykVysledku	eng - angličtina
http://linked.open.../riv/klicovaSlova	ICME sheath; Magnetic reconnection (en)
http://linked.open.../riv/klicoveSlovo	ICME sheath Magnetic reconnection
http://linked.open...ontrolniKodProRIV	[D093E635F046]
http://linked.open...v/mistoKonaniAkce	Praha
http://linked.open...i/riv/mistoVydani	Praha
http://linked.open...i/riv/nazevZdroje	WDS'11 Proceedings of Contributed Papers: Part II – Physics of Plasmas and Ionized Media
http://linked.open...in/vavai/riv/obor	BL
http://linked.open...ichTvurcuVysledku	4 (xsd:int)
http://linked.open...cetTvurcuVysledku	4 (xsd:int)
http://linked.open...vavai/riv/projekt	Application of fast monitors for the study of instabilities in the solar wind and foreshock region
http://linked.open...UplatneniVysledku	2011
http://linked.open...iv/tvurceVysledku	Přech, Lubomír Lynnyk, Andrii Grygorov, Kostiantyn Enžl, Jakub
http://linked.open...vavai/riv/typAkce	EUR - Evropská
http://linked.open.../riv/zahajeniAkce	2011-05-31 (xsd:date)
number of pages	5 (xsd:int)
http://purl.org/ne...btex#hasPublisher	Matfyzpress
https://schema.org/isbn	978-80-7378-185-9
http://localhost/t...ganizacniJednotka	11320

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