About: Type III Radio Bursts at Long Wavelengths: Statistical Survey

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

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rdf:type	skos:Concept http://linked.opendata.cz/ontology/domain/vavai/Vysledek
Description	We present statistical results of 156 type III radio bursts observed by S/Waves instruments on- board two STEREO spacecraft between May 2007 and September 2011. We have used data from the High Frequency Receiver (HFR, a part of the STEREO/Waves instrument) which provides us with the goniopolarimetric (GP, also referred to as direction-nding) measurements between 125 kHz and 2 MHz, while flux density is recorded up to 16 MHz. We have investigated both ux density and GP properties of type III radio bursts. We have found that maximum of flux density occurs at 1 MHz. The apparent source size during peak uxes is very extended (approximately 40 degrees) for low frequencies (below 500 kHz), while remaining almost constant between 500 kHz and 2 MHz (25 degrees). Deviation of the wave vector from the Sun-spacecraft line has a maximum of 40 degrees for lowest frequency decreasing to 10 degrees for 2 MHz. We present statistical results of 156 type III radio bursts observed by S/Waves instruments on- board two STEREO spacecraft between May 2007 and September 2011. We have used data from the High Frequency Receiver (HFR, a part of the STEREO/Waves instrument) which provides us with the goniopolarimetric (GP, also referred to as direction-nding) measurements between 125 kHz and 2 MHz, while flux density is recorded up to 16 MHz. We have investigated both ux density and GP properties of type III radio bursts. We have found that maximum of flux density occurs at 1 MHz. The apparent source size during peak uxes is very extended (approximately 40 degrees) for low frequencies (below 500 kHz), while remaining almost constant between 500 kHz and 2 MHz (25 degrees). Deviation of the wave vector from the Sun-spacecraft line has a maximum of 40 degrees for lowest frequency decreasing to 10 degrees for 2 MHz. (en)
Title	Type III Radio Bursts at Long Wavelengths: Statistical Survey Type III Radio Bursts at Long Wavelengths: Statistical Survey (en)
skos:prefLabel	Type III Radio Bursts at Long Wavelengths: Statistical Survey Type III Radio Bursts at Long Wavelengths: Statistical Survey (en)
skos:notation	RIV/68378289:_____/12:00426542!RIV14-MSM-68378289
http://linked.open...avai/riv/aktivita	I P
http://linked.open...avai/riv/aktivity	I, P(LG11032)
http://linked.open...vai/riv/dodaniDat	2014
http://linked.open...aciTvurceVysledku	Santolík, Ondřej Krupař, Vratislav
http://linked.open.../riv/druhVysledku	O - Ostatní výsledky nezařaditelné do žádného z výše uvedených druhů výsledku
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	175531
http://linked.open...ai/riv/idVysledku	RIV/68378289:_____/12:00426542
http://linked.open...riv/jazykVysledku	eng - angličtina
http://linked.open.../riv/klicovaSlova	flux density; long wavelengths; type III radio bursts (en)
http://linked.open.../riv/klicoveSlovo	long wavelengths type III radio bursts flux density
http://linked.open...ontrolniKodProRIV	[CC5C61294F72]
http://linked.open...in/vavai/riv/obor	DG
http://linked.open...ichTvurcuVysledku	2 (xsd:int)
http://linked.open...cetTvurcuVysledku	4 (xsd:int)
http://linked.open...vavai/riv/projekt	COSPAR 2011-2013
http://linked.open...UplatneniVysledku	2012
http://linked.open...iv/tvurceVysledku	Santolík, Ondřej Cecconi, B. Krupař, Vratislav Maksimovic, M.

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