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Database of Whistler-mode Chorus in the Equatorial Plane
Macúšová, E. ; Santolík, Ondřej
Chorus emission is one of the most intense electromagnetic waves. Its source region is localised close to the geomagnetic equatorial plane within a few degrees. We present a unique database of whistler-mode chorus/hiss events obtained from the complete data set of wave measurements provided by the STAFF/DWP wave instrument on board TC-1 spacecraft. The TC-1 is one of two Earth orbiting satellites from the Double Star mission and it orbits close to the equatorial plane. Some instruments onboard both spacecraft are identical to those currently flying on the four Cluster spacecraft. The data base covers the full operational period of the spacecraft, between January 2004 and October 2007. All the events have been visually selected from the onboard-analyzed time-frequency spectrograms of magnetic search-coil measurements below 4 kHz.
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Calibration of the STEREO/WAVES Instrument in the Solar Wind
Krupař, Vratislav ; Maksimovic, M. ; Cecconi, B. ; Santolík, Ondřej
The S/WAVES instrument onboard the STEREO spacecraft measures electromagnetic waves in the solar wind. This unique project allows us to investigate properties of type II and type III radio bursts related with solar flares and propagation of coronal mass ejections (CMEs) in the interplanetary medium, respectively. In this paper we present properties of the High Frequency Receiver (HFR) receiver which covers the frequency range 125 kHz–16.025 MHz. We have compared the gains from the two HFR channels and we have found significant variations of these gains with time. We have proposed a solution for correcting these gain variations and improving the S/WAVES HFR calibrations in order to get as accurate goniopolarimetric measurements as possible.
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Analýza nestacionárního proudění uvnitř ulice a dvoru
Kellnerová, Radka ; Jaňour, Zbyněk
Jedno-bodovým měřením jsme získali prostorové rozložení strředního toku hybnosti a momentů třetího řádu (šikmost) složek rychlosti. Zkoumaná oblast pokrývala vnitřní část uličního kaňonu a přilehlé křižovatky. Střední hodnoty toku hybnosti byly rozděleny do jednotlivých kvadrantů podle kavadrantové analýzy. Srovnáním mezi těmito kvadranty a šikmostí jsme získali náhled na prostorové rozložení silných intermitentních dějů v kaňonu a pomohli vysvětlit lokální dominanci událostí "sweep" nebo "ejection".
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