Počet záznamů: 1
Current sheet structure and associated small-scale flux ropes in the heliospheric magnetic field observed by Solar Orbiter
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SYSNO ASEP 0538733 Druh ASEP A - Abstrakt Zařazení RIV Záznam nebyl označen do RIV Zařazení RIV Není vybrán druh dokumentu Název Current sheet structure and associated small-scale flux ropes in the heliospheric magnetic field observed by Solar Orbiter Tvůrce(i) Eastwood, J. P. (GB)
Stawarz, J. E. (GB)
Souček, Jan (UFA-U) RID, ORCID
Štverák, Štěpán (ASU-R) RID, ORCID
Trávníček, P. M. (US)Celkový počet autorů 35 Zdroj.dok. AGU Fall Meeting. - : American Geophysical Union, 2020
SH035-08Poč.str. 1 s. Akce AGU Fall Meeting 2020 Datum konání 01.12.2020 - 17.12.2020 Místo konání online everywhere Země US - Spojené státy americké Typ akce WRD Jazyk dok. eng - angličtina Země vyd. US - Spojené státy americké Klíč. slova heliosphere ; solar orbiter ; solar wind ; heliospheric magnetic field ; magnetic flux rope structures Vědní obor RIV BN - Astronomie a nebeská mechanika, astrofyzika Obor OECD Astronomy (including astrophysics,space science) Vědní obor RIV – spolupráce Astronomický ústav - Astronomie a nebeská mechanika, astrofyzika Institucionální podpora UFA-U - RVO:68378289 ; ASU-R - RVO:67985815 Anotace A notable feature of current sheets in the magnetosphere of Earth and other planets is the formation of flux ropes, helical magnetic field structures which are thought to play a key role in the dynamics of the current sheet and in particle acceleration models. Flux ropes are commonly produced by magnetic reconnection, and so provide insight into the time-dependent nature of the reconnection process. Reconnection is also an important target for studies of solar wind physics as it controls the topology of the heliospheric magnetic field and may also enable particle heating and acceleration. In contrast to the Earth’s magnetosphere, current sheets in the solar wind extend to very large scales, reconnection is typically large scale and relatively steady-state, and observations of flux ropes contained within solar wind current sheets are very rare, even though they are a potentially important component of many particle acceleration models. The general properties of such flux ropes are therefore poorly understood, including their prevalence and size distribution. 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 2021
Počet záznamů: 1