About: Solar Wind Modification Upstream of the Bow Shock

Facets (new session)
Description
Metadata
Settings
- owl:sameAs
- Inference Rule:

About: Solar Wind Modification Upstream of the Bow Shock Goto Sponge NotDistinct Permalink

An Entity of Type : http://linked.opendata.cz/ontology/domain/vavai/Vysledek, within Data Space : linked.opendata.cz associated with source document(s)

Attributes	Values
rdf:type	skos:Concept http://linked.opendata.cz/ontology/domain/vavai/Vysledek
rdfs:seeAlso	http://dx.doi.org/10.1063/1.4811079
Description	A spacecraft configuration with two monitors near L1 and a fleet of the spacecraft orbiting in front of the bow shock brings a great opportunity to test the propagation techniques for the solar wind and the assumption on a negligible solar wind parameter evolution. We use multi-point observations of the THEMIS-ARTEMIS mission and compare them with data from the Wind solar wind monitor in order to estimate different factors influencing solar wind speed evolution. We have found a significant deceleration (up to 6%) of the solar wind close to the bow shock and the effect extends up to 30 RE from the Earth. It is controlled by the level of magnetic field fluctuations and by the flux of reflected and accelerated particles. We can conclude that the reflected particles not only excite waves of large amplitudes but also modify mean values of the solar wind speed measured in an unperturbed solar wind. A spacecraft configuration with two monitors near L1 and a fleet of the spacecraft orbiting in front of the bow shock brings a great opportunity to test the propagation techniques for the solar wind and the assumption on a negligible solar wind parameter evolution. We use multi-point observations of the THEMIS-ARTEMIS mission and compare them with data from the Wind solar wind monitor in order to estimate different factors influencing solar wind speed evolution. We have found a significant deceleration (up to 6%) of the solar wind close to the bow shock and the effect extends up to 30 RE from the Earth. It is controlled by the level of magnetic field fluctuations and by the flux of reflected and accelerated particles. We can conclude that the reflected particles not only excite waves of large amplitudes but also modify mean values of the solar wind speed measured in an unperturbed solar wind. (en)
Title	Solar Wind Modification Upstream of the Bow Shock Solar Wind Modification Upstream of the Bow Shock (en)
skos:prefLabel	Solar Wind Modification Upstream of the Bow Shock Solar Wind Modification Upstream of the Bow Shock (en)
skos:notation	RIV/00216208:11320/13:10191871!RIV14-GA0-11320___
http://linked.open...avai/predkladatel	Matematicko-fyzikální fakulta
http://linked.open...avai/riv/aktivita	I P S Z
http://linked.open...avai/riv/aktivity	I, P(GA205/09/0170), P(GAP209/12/1774), S, Z(MSM0021620860)
http://linked.open...vai/riv/dodaniDat	2014
http://linked.open...aciTvurceVysledku	Přech, Lubomír Jelínek, Karel Šafránková, Jana Němeček, Zdeněk Urbář, Jaroslav
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	106226
http://linked.open...ai/riv/idVysledku	RIV/00216208:11320/13:10191871
http://linked.open...riv/jazykVysledku	eng - angličtina
http://linked.open.../riv/klicovaSlova	Foreshock; Reflected particles; Interplanetary magnetic field; Solar wind velocity (en)
http://linked.open.../riv/klicoveSlovo	Interplanetary magnetic field Foreshock Reflected particles Solar wind velocity
http://linked.open...ontrolniKodProRIV	[FFCD624B3AB6]
http://linked.open...v/mistoKonaniAkce	HI
http://linked.open...i/riv/mistoVydani	MELVILLE
http://linked.open...i/riv/nazevZdroje	AIP Conference Proceedings
http://linked.open...in/vavai/riv/obor	BL
http://linked.open...ichTvurcuVysledku	5 (xsd:int)
http://linked.open...cetTvurcuVysledku	5 (xsd:int)
http://linked.open...vavai/riv/projekt	The role of solar wind disturbances in Space Weather Solar wind control of the processes at the magnetospheric boundaries
http://linked.open...UplatneniVysledku	2013
http://linked.open...iv/tvurceVysledku	Němeček, Zdeněk Přech, Lubomír Šafránková, Jana Jelínek, Karel Urbář, Jaroslav
http://linked.open...vavai/riv/typAkce	WRD - Světová
http://linked.open...ain/vavai/riv/wos	000320997100104
http://linked.open.../riv/zahajeniAkce	2012-05-17 (xsd:date)
http://linked.open...n/vavai/riv/zamer	Fyzikální studium objektů a procesů ve sluneční soustavě a v astrofyzikálních systémech
issn	0094-243X
number of pages	4 (xsd:int)
http://bibframe.org/vocab/doi	10.1063/1.4811079
http://purl.org/ne...btex#hasPublisher	AMER INST PHYSICS
https://schema.org/isbn	978-0-7354-1163-0
http://localhost/t...ganizacniJednotka	11320

Faceted Search & Find service v1.16.118 as of Jun 21 2024

Alternative Linked Data Documents: ODE Content Formats:

RDF

ODATA

Microdata

About

OpenLink Virtuoso version 07.20.3240 as of Jun 21 2024, on Linux (x86_64-pc-linux-gnu), Single-Server Edition (126 GB total memory, 47 GB memory in use)
Data on this page belongs to its respective rights holders.
Virtuoso Faceted Browser Copyright © 2009-2024 OpenLink Software