Bandwidths and amplitudes of chorus-like banded emissions measured by the TC-1 Double Star spacecraft

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F15%3A10319424" target="_blank" >RIV/00216208:11320/15:10319424 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/68378289:_____/15:00441082

Výsledek na webu

<a href="http://dx.doi.org/10.1002/2014JA020440" target="_blank" >http://dx.doi.org/10.1002/2014JA020440</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1002/2014JA020440" target="_blank" >10.1002/2014JA020440</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Bandwidths and amplitudes of chorus-like banded emissions measured by the TC-1 Double Star spacecraft

Popis výsledku v původním jazyce

Characteristics of banded whistler-mode emissions are derived from a database of chorus-like events obtained from the complete data set of the wave measurements provided by the Spatio-Temporal Analysis of Field Fluctuation-Digital Wave Processing (STAFF-DWP) wave instrument on board the TC-1 Double Star spacecraft. Our study covers the full operational period of this spacecraft (almost 4 years). Our entire data set has been collected within 30 degrees of geomagnetic latitude at L shells between 2 and 12and below 4 kHz. All events have been processed automatically to accurately determine their power spectral density (PSD), bandwidth, and amplitude. We found most cases of chorus-like banded emissions at L10 on the dawnside and dayside. The upper band emissions (above one half of the equatorial electron cyclotron frequency) occur almost 20 times less often than the lower band, and their average amplitude is almost 3 times smaller than for the lower band. Intense upper band emissions cove

Název v anglickém jazyce

Bandwidths and amplitudes of chorus-like banded emissions measured by the TC-1 Double Star spacecraft

Popis výsledku anglicky

Characteristics of banded whistler-mode emissions are derived from a database of chorus-like events obtained from the complete data set of the wave measurements provided by the Spatio-Temporal Analysis of Field Fluctuation-Digital Wave Processing (STAFF-DWP) wave instrument on board the TC-1 Double Star spacecraft. Our study covers the full operational period of this spacecraft (almost 4 years). Our entire data set has been collected within 30 degrees of geomagnetic latitude at L shells between 2 and 12and below 4 kHz. All events have been processed automatically to accurately determine their power spectral density (PSD), bandwidth, and amplitude. We found most cases of chorus-like banded emissions at L10 on the dawnside and dayside. The upper band emissions (above one half of the equatorial electron cyclotron frequency) occur almost 20 times less often than the lower band, and their average amplitude is almost 3 times smaller than for the lower band. Intense upper band emissions cove

Druh

J_x - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)

CEP obor

BL - Fyzika plasmatu a výboje v plynech

OECD FORD obor

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Projekt

Výsledek vznikl pri realizaci vícero projektů. Více informací v záložce Projekty.

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2015

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Journal of Geophysical Research - Space Physics

ISSN

2169-9380

e-ISSN

—

Svazek periodika

120

Číslo periodika v rámci svazku

2

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

15

Strana od-do

1057-1071

Kód UT WoS článku

000351360800015

EID výsledku v databázi Scopus

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