% IMPORTANT: The following is UTF-8 encoded. This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.
@ARTICLE{Klinger:836047,
author = {Klinger, T. and Alonso, A. and Bozhenkov, S. and Burhenn,
R. and Dinklage, A. and Fuchert, G. and Geiger, J. and
Grulke, O. and Langenberg, A. and Hirsch, M. and Kocsis, G.
and Knauer, J. and Krämer-Flecken, A. and Laqua, H. and
Lazerson, S. and Landreman, M. and Maaßberg, H. and Marsen,
S. and Otte, M. and Pablant, N. and Pasch, E. and Rahbarnia,
K. and Stange, T. and Szepesi, T. and Thomsen, H. and
Traverso, P. and Velasco, J. L. and Wauters, T. and Weir, G.
and Windisch, T.},
title = {{P}erformance and properties of the first plasmas of
{W}endelstein 7-{X}},
journal = {Plasma physics and controlled fusion},
volume = {59},
number = {1},
issn = {1361-6587},
address = {Bristol},
publisher = {IOP Publ.},
reportid = {FZJ-2017-05172},
pages = {014018 -},
year = {2017},
abstract = {The 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.},
cin = {IEK-4},
ddc = {530},
cid = {I:(DE-Juel1)IEK-4-20101013},
pnm = {171 - Stellarator Research (POF3-171)},
pid = {G:(DE-HGF)POF3-171},
typ = {PUB:(DE-HGF)16},
UT = {WOS:000386799100001},
doi = {10.1088/0741-3335/59/1/014018},
url = {https://juser.fz-juelich.de/record/836047},
}