000836047 001__ 836047
000836047 005__ 20240711113524.0
000836047 0247_ $$2doi$$a10.1088/0741-3335/59/1/014018
000836047 0247_ $$2ISSN$$a0032-1028
000836047 0247_ $$2ISSN$$a0368-3281
000836047 0247_ $$2ISSN$$a0741-3335
000836047 0247_ $$2ISSN$$a1361-6587
000836047 0247_ $$2ISSN$$a1879-2979
000836047 0247_ $$2Handle$$a2128/15006
000836047 0247_ $$2WOS$$aWOS:000386799100001
000836047 037__ $$aFZJ-2017-05172
000836047 041__ $$aEnglish
000836047 082__ $$a530
000836047 1001_ $$0P:(DE-HGF)0$$aKlinger, T.$$b0$$eCorresponding author
000836047 245__ $$aPerformance and properties of the first plasmas of Wendelstein 7-X
000836047 260__ $$aBristol$$bIOP Publ.$$c2017
000836047 3367_ $$2DRIVER$$aarticle
000836047 3367_ $$2DataCite$$aOutput Types/Journal article
000836047 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1501503753_31600
000836047 3367_ $$2BibTeX$$aARTICLE
000836047 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000836047 3367_ $$00$$2EndNote$$aJournal Article
000836047 520__ $$aThe optimized, superconducting stellarator Wendelstein 7-X went into operation and delivered first measurement data after 15 years of construction and one year commissioning. Errors in the magnet assembly were confirmend to be small. Plasma operation was started with 5 MW electron cyclotron resonance heating (ECRH) power and five inboard limiters. Core plasma values of ${{T}_{\text{e}}}>8$ keV, ${{T}_{\text{i}}}>2$ keV at line-integrated densities $n\approx 3\centerdot {{10}^{19}}~{{\text{m}}^{-2}}$ were achieved, exceeding the original expectations by about a factor of two. Indications for a core-electron-root were found. The energy confinement times are in line with the international stellarator scaling, despite unfavourable wall conditions, i.e. large areas of metal surfaces and particle sources from the limiter close to the plasma volume. Well controlled shorter hydrogen discharges at higher power (4 MW ECRH power for 1 s) and longer discharges at lower power (0.7 MW ECRH power for 6 s) could be routinely established after proper wall conditioning. The fairly large set of diagnostic systems running in the end of the 10 weeks operation campaign provided first insights into expected and unexpected physics of optimized stellarators.
000836047 536__ $$0G:(DE-HGF)POF3-171$$a171 - Stellarator Research (POF3-171)$$cPOF3-171$$fPOF III$$x0
000836047 588__ $$aDataset connected to CrossRef
000836047 7001_ $$0P:(DE-HGF)0$$aAlonso, A.$$b1
000836047 7001_ $$0P:(DE-HGF)0$$aBozhenkov, S.$$b2
000836047 7001_ $$0P:(DE-HGF)0$$aBurhenn, R.$$b3
000836047 7001_ $$0P:(DE-HGF)0$$aDinklage, A.$$b4
000836047 7001_ $$0P:(DE-HGF)0$$aFuchert, G.$$b5
000836047 7001_ $$0P:(DE-HGF)0$$aGeiger, J.$$b6
000836047 7001_ $$0P:(DE-HGF)0$$aGrulke, O.$$b7
000836047 7001_ $$0P:(DE-HGF)0$$aLangenberg, A.$$b8
000836047 7001_ $$0P:(DE-HGF)0$$aHirsch, M.$$b9
000836047 7001_ $$0P:(DE-HGF)0$$aKocsis, G.$$b10
000836047 7001_ $$0P:(DE-HGF)0$$aKnauer, J.$$b11
000836047 7001_ $$0P:(DE-Juel1)130075$$aKrämer-Flecken, A.$$b12$$ufzj
000836047 7001_ $$0P:(DE-HGF)0$$aLaqua, H.$$b13
000836047 7001_ $$0P:(DE-HGF)0$$aLazerson, S.$$b14
000836047 7001_ $$0P:(DE-HGF)0$$aLandreman, M.$$b15
000836047 7001_ $$0P:(DE-HGF)0$$aMaaßberg, H.$$b16
000836047 7001_ $$0P:(DE-HGF)0$$aMarsen, S.$$b17
000836047 7001_ $$0P:(DE-HGF)0$$aOtte, M.$$b18
000836047 7001_ $$0P:(DE-HGF)0$$aPablant, N.$$b19
000836047 7001_ $$0P:(DE-HGF)0$$aPasch, E.$$b20
000836047 7001_ $$0P:(DE-HGF)0$$aRahbarnia, K.$$b21
000836047 7001_ $$0P:(DE-HGF)0$$aStange, T.$$b22
000836047 7001_ $$0P:(DE-HGF)0$$aSzepesi, T.$$b23
000836047 7001_ $$0P:(DE-HGF)0$$aThomsen, H.$$b24
000836047 7001_ $$0P:(DE-HGF)0$$aTraverso, P.$$b25
000836047 7001_ $$0P:(DE-HGF)0$$aVelasco, J. L.$$b26
000836047 7001_ $$0P:(DE-Juel1)145890$$aWauters, T.$$b27$$ufzj
000836047 7001_ $$0P:(DE-HGF)0$$aWeir, G.$$b28
000836047 7001_ $$0P:(DE-HGF)0$$aWindisch, T.$$b29
000836047 773__ $$0PERI:(DE-600)1473144-7$$a10.1088/0741-3335/59/1/014018$$gVol. 59, no. 1, p. 014018 -$$n1$$p014018 -$$tPlasma physics and controlled fusion$$v59$$x1361-6587$$y2017
000836047 8564_ $$uhttps://juser.fz-juelich.de/record/836047/files/Klinger_2017_Plasma_Phys._Control._Fusion_59_014018.pdf$$yOpenAccess
000836047 8564_ $$uhttps://juser.fz-juelich.de/record/836047/files/Klinger_2017_Plasma_Phys._Control._Fusion_59_014018.pdf?subformat=pdfa$$xpdfa$$yOpenAccess
000836047 909CO $$ooai:juser.fz-juelich.de:836047$$pdnbdelivery$$pVDB$$pdriver$$popen_access$$popenaire
000836047 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)130075$$aForschungszentrum Jülich$$b12$$kFZJ
000836047 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)145890$$aForschungszentrum Jülich$$b27$$kFZJ
000836047 9131_ $$0G:(DE-HGF)POF3-171$$1G:(DE-HGF)POF3-170$$2G:(DE-HGF)POF3-100$$3G:(DE-HGF)POF3$$4G:(DE-HGF)POF$$aDE-HGF$$bEnergie$$lKernfusion$$vStellarator Research$$x0
000836047 9141_ $$y2017
000836047 915__ $$0LIC:(DE-HGF)CCBY3$$2HGFVOC$$aCreative Commons Attribution CC BY 3.0
000836047 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS
000836047 915__ $$0StatID:(DE-HGF)0600$$2StatID$$aDBCoverage$$bEbsco Academic Search
000836047 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bPLASMA PHYS CONTR F : 2015
000836047 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection
000836047 915__ $$0StatID:(DE-HGF)0110$$2StatID$$aWoS$$bScience Citation Index
000836047 915__ $$0StatID:(DE-HGF)0111$$2StatID$$aWoS$$bScience Citation Index Expanded
000836047 915__ $$0StatID:(DE-HGF)9900$$2StatID$$aIF < 5
000836047 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000836047 915__ $$0StatID:(DE-HGF)0030$$2StatID$$aPeer Review$$bASC
000836047 915__ $$0StatID:(DE-HGF)1150$$2StatID$$aDBCoverage$$bCurrent Contents - Physical, Chemical and Earth Sciences
000836047 915__ $$0StatID:(DE-HGF)0430$$2StatID$$aNational-Konsortium
000836047 915__ $$0StatID:(DE-HGF)0420$$2StatID$$aNationallizenz
000836047 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bThomson Reuters Master Journal List
000836047 9201_ $$0I:(DE-Juel1)IEK-4-20101013$$kIEK-4$$lPlasmaphysik$$x0
000836047 9801_ $$aFullTexts
000836047 980__ $$ajournal
000836047 980__ $$aVDB
000836047 980__ $$aUNRESTRICTED
000836047 980__ $$aI:(DE-Juel1)IEK-4-20101013
000836047 981__ $$aI:(DE-Juel1)IFN-1-20101013