This HTML5 document contains 48 embedded RDF statements represented using HTML+Microdata notation.

The embedded RDF content will be recognized by any processor of HTML5 Microdata.

Namespace Prefixes

PrefixIRI
n9http://linked.opendata.cz/ontology/domain/vavai/riv/typAkce/
dctermshttp://purl.org/dc/terms/
n16http://purl.org/net/nknouf/ns/bibtex#
n15http://localhost/temp/predkladatel/
n12http://linked.opendata.cz/resource/domain/vavai/projekt/
n11http://linked.opendata.cz/resource/domain/vavai/riv/tvurce/
n23http://linked.opendata.cz/resource/domain/vavai/subjekt/
n14http://linked.opendata.cz/ontology/domain/vavai/
n20https://schema.org/
n18http://linked.opendata.cz/resource/domain/vavai/vysledek/RIV%2F00216208%3A11320%2F13%3A10192206%21RIV14-GA0-11320___/
shttp://schema.org/
skoshttp://www.w3.org/2004/02/skos/core#
rdfshttp://www.w3.org/2000/01/rdf-schema#
n3http://linked.opendata.cz/ontology/domain/vavai/riv/
n2http://linked.opendata.cz/resource/domain/vavai/vysledek/
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
n7http://linked.opendata.cz/ontology/domain/vavai/riv/klicoveSlovo/
n8http://linked.opendata.cz/ontology/domain/vavai/riv/duvernostUdaju/
xsdhhttp://www.w3.org/2001/XMLSchema#
n21http://linked.opendata.cz/ontology/domain/vavai/riv/jazykVysledku/
n6http://linked.opendata.cz/ontology/domain/vavai/riv/aktivita/
n22http://linked.opendata.cz/ontology/domain/vavai/riv/obor/
n17http://linked.opendata.cz/ontology/domain/vavai/riv/druhVysledku/
n4http://reference.data.gov.uk/id/gregorian-year/

Statements

Subject Item
n2:RIV%2F00216208%3A11320%2F13%3A10192206%21RIV14-GA0-11320___
rdf:type
skos:Concept n14:Vysledek
rdfs:seeAlso
http://www.mff.cuni.cz/veda/konference/wds/proc/pdf13/WDS13_203_f2_Grygorov.pdf
dcterms:description
We present a study of the impact of the interplanetary (IP) shock on December 7, 2003 in the distant tail of the Earth's magnetosphere. Using the data from the several spacecraft located in the solar wind in front of the Earth, we monitor the propagation of the IP shock from the L1 point to the magnetosphere and to magnetotail. Taking into account its velocity and beginning of the substorm onset from the ground, we considered the plasma parameters on the Wind spacecraft located downstream at XGSM MINUS SIGN 230 RE. Shortly after the shock arrival, Wind crossed consequentially southern and northern lobes in between which observed a flux rope and the tailward fast plasma flow ( 780 km/s) in the plasmasheet. We found that a orientation of the nominal tail axis is affected by VY components of the solar wind. Also, according to Wind data, we present a sketch how the distant tail moves with respect to the IP shock passage. We present a study of the impact of the interplanetary (IP) shock on December 7, 2003 in the distant tail of the Earth's magnetosphere. Using the data from the several spacecraft located in the solar wind in front of the Earth, we monitor the propagation of the IP shock from the L1 point to the magnetosphere and to magnetotail. Taking into account its velocity and beginning of the substorm onset from the ground, we considered the plasma parameters on the Wind spacecraft located downstream at XGSM MINUS SIGN 230 RE. Shortly after the shock arrival, Wind crossed consequentially southern and northern lobes in between which observed a flux rope and the tailward fast plasma flow ( 780 km/s) in the plasmasheet. We found that a orientation of the nominal tail axis is affected by VY components of the solar wind. Also, according to Wind data, we present a sketch how the distant tail moves with respect to the IP shock passage.
dcterms:title
Far Magnetotail Observations of an Interplanetary Shock Far Magnetotail Observations of an Interplanetary Shock
skos:prefLabel
Far Magnetotail Observations of an Interplanetary Shock Far Magnetotail Observations of an Interplanetary Shock
skos:notation
RIV/00216208:11320/13:10192206!RIV14-GA0-11320___
n14:predkladatel
n23:orjk%3A11320
n3:aktivita
n6:S n6:P n6:I
n3:aktivity
I, P(GA205/09/0170), S
n3:dodaniDat
n4:2014
n3:domaciTvurceVysledku
n11:1504126 Grygorov, Kostiantyn n11:5876265 n11:3178129
n3:druhVysledku
n17:D
n3:duvernostUdaju
n8:S
n3:entitaPredkladatele
n18:predkladatel
n3:idSjednocenehoVysledku
74651
n3:idVysledku
RIV/00216208:11320/13:10192206
n3:jazykVysledku
n21:eng
n3:klicovaSlova
Interplanetary shock; Magnetotail
n3:klicoveSlovo
n7:Interplanetary%20shock n7:Magnetotail
n3:kontrolniKodProRIV
[59DF51AD862A]
n3:mistoKonaniAkce
Praha
n3:mistoVydani
Praha
n3:nazevZdroje
WDS'13 Proceedings of Contributed Papers: Part II - Physics of Plasmas and Ionized Media
n3:obor
n22:BL
n3:pocetDomacichTvurcuVysledku
4
n3:pocetTvurcuVysledku
4
n3:projekt
n12:GA205%2F09%2F0170
n3:rokUplatneniVysledku
n4:2013
n3:tvurceVysledku
Němeček, Zdeněk Šafránková, Jana Přech, Lubomír Grygorov, Kostiantyn
n3:typAkce
n9:EUR
n3:zahajeniAkce
2013-06-04+02:00
s:numberOfPages
10
n16:hasPublisher
Matfyzpress
n20:isbn
978-80-7378-251-1
n15:organizacniJednotka
11320