Počet záznamů: 1

THOR Fluxgate Magnetometer (MAG)

SYSNO ASEP	0459692
Druh ASEP	A - Abstrakt
Zařazení RIV	Záznam nebyl označen do RIV
Zařazení RIV	Není vybrán druh dokumentu
Název	THOR Fluxgate Magnetometer (MAG)
Tvůrce(i)	Nakamura, R. (AT) Eastwood, J. (GB) Magnes, W. (AT) Valavanoglou, A. (AT) Carr, C. M. (GB) O’Brien, H. L. (GB) Narita, Y. (AT) Delva, M. (AT) Chen, Ch. H. K. (GB) Plaschke, F. (GB) Souček, Jan (UFA-U)_{RID, ORCID}
Celkový počet autorů	11
Zdroj.dok.	Geophysical Research Abstracts. - Göttingen : European Geosciences Union, 2016 - ISSN 1607-7962 EGu2016-12336
Poč.str.	1 s.
Forma vydání	Tištěná - P
Akce	EGU General Assembly 2016
Datum konání	17.04.2016-22.04.2016
Místo konání	Vienna
Země	AT - Rakousko
Typ akce	WRD
Jazyk dok.	eng - angličtina
Země vyd.	DE - Německo
Klíč. slova	Fluxgate Magnetometer (MAG) ; THOR ; plasma turbulence
Vědní obor RIV	BL - Fyzika plazmatu a výboje v plynech
Institucionální podpora	UFA-U - RVO:68378289
Anotace	Turbulence Heating ObserveR (THOR) is the first mission ever flown in space dedicated to plasma turbulence. The/ngoal of the Fluxgate Magnetometer (MAG) is to measure the DC to low frequency ambient magnetic field. The/ndesign of the magnetometer consists of two tri-axial sensors and the related magnetometer electronics; the electronics/nare hosted on printed circuit boards in the common electronics box of the fields and wave processor (FWP). A/nfully redundant two sensor system mounted on a common boom and the new miniaturized low noise design based/non MMS and Solar Orbiter instruments enable accurate measurement throughout the region of interest for THOR/nscience. The usage of the common electronics hosted by FWP guarantees to fulfill the required timing accuracy/nwith other fields measurements. These improvements are important to obtain precise measurements of magnetic/nfield, which is essential to estimate basic plasma parameters and correctly identify the spatial and temporal scales/nof the turbulence. Furthermore, THOR MAG provides high quality data with sufficient overlap with the Search/nCoil Magnetometer (SCM) in frequency space to obtain full coverage of the wave forms over all the frequencies/nnecessary to obtain the full solar wind turbulence spectrum from MHD to kinetic range with sufficient accuracy
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	2017

Počet záznamů: 1