Počet záznamů: 1
Cluster Observations of Particle Injections in the Exterior Cusp
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SYSNO ASEP 0442503 Druh ASEP A - Abstrakt Zařazení RIV Záznam nebyl označen do RIV Zařazení RIV Není vybrán druh dokumentu Název Cluster Observations of Particle Injections in the Exterior Cusp Tvůrce(i) Escoubet, C. P. (NL)
Grison, Benjamin (UFA-U) RID, ORCID
Berchem, J. (US)
Trattner, K. (US)
Lavraud, B. (FR)
Pitout, F. (FR)
Souček, Jan (UFA-U) RID, ORCID
Richard, R. (US)
Laakso, H. (NL)
Masson, A. (ES)
Dandouras, I. (FR)
Reme, H. (FR)
Fazakerley, A. (GB)
Daly, P. (DE)Zdroj.dok. AGU Fall Meeting. - s. l : American Geophysical Union, 2014
SM13F-4219Akce AGU Fall Meeting Datum konání 15.12.2014-19.12.2014 Místo konání San Francisco Země US - Spojené státy americké Typ akce WRD Jazyk dok. eng - angličtina Země vyd. US - Spojené státy americké Institucionální podpora UFA-U - RVO:68378289 Anotace The main process that injects solar wind plasma into the polar cusp is now generally accepted to be magnetic reconnection. Depending on the IMF direction, this process takes place equatorward (for IMF southward), poleward (for IMF northward) or on the dusk or dawn sides (for IMF azimuthal) of the cusp. We report a Cluster crossing on 5 January 2002 near the exterior cusp on the southern dusk side. The IMF was mainly azimuthal (IMF-By around -5 nT), the solar wind speed lower than usual around 280 km/s with the density of order 5 cm-3. The four Cluster spacecraft had an elongated configuration near the magnetopause. C4 was the first spacecraft to enter the cusp around 19:52:04 UT, followed by C2 at 19:52:35 UT, C1 at 19:54:24 UT and C3 at 20:13:15 UT. C4 and C1 observed two ion energy dispersions at 20:10 UT and 20:40 UT and C3 at 20:35 UT and 21:15 UT. Using the time of flight technique on the upgoing and downgoing ions, which leads to energy dispersions, we obtain distances of the ion sources between 14 and 20 RE from the spacecraft. Using Tsyganenko model, we find that these sources are located on the dusk flank, past the terminator. The first injection by C3 is seen at approximately the same time as the 2nd injection on C1 but their sources at the magnetopause were separated by more than 7 RE. This would imply that two distinct sources were active at the same time on the dusk flank of the magnetosphere. In addition, a flow reversal was observed at the magnetopause on C4 which would be an indication that reconnection is taking place near the exterior cusp. Pracoviště Ústav fyziky atmosféry Kontakt Kateřina Adamovičová, adamovicova@ufa.cas.cz, Tel.: 272 016 012 ; Kateřina Potužníková, kaca@ufa.cas.cz, Tel.: 272 016 019 Rok sběru 2015
Počet záznamů: 1