@article{oai:nifs-repository.repo.nii.ac.jp:00011649,
 author = {WARMER, Felix and TANAKA,  Kenji and XANTHOPOULOS, P. and NUNAMI,  Masanori and NAKATA, Motoki and BEIDLER, Craig and BOZHENKOV, Sergey and BEURSKENS, Marc and BRUNNER, K. J. and FORD, O. P. and FUCHERT, Golo and FUNABA,  Hisamichi and GEIGER, J. and GRADIC, D. and IDA,  Katsumi and IGAMI,  Hiroe and KUBO,  Shin and LANGENBERG, Andreas and LAQUA, Heinrich and LAZERSON, Samuel and MORISAKI,  Tomohiro and OSAKABE,  Masaki and PABLANT, Novimir and PASCH, E. and PETERSON,  Byron and PETERSON,  Byron J. and SATAKE,  Shinsuke and SEKI,  Ryosuke and SHIMOZUMA,  Takashi and SMITH, H. M. and STANGE, Torsten and STECHOW, A. von and SUGAMA,  Hideo and SUZUKI,  Yasuhiro and TAKAHASHI,  Hiromi and TOKUZAWA,  Tokihiko and TSUJIMURA, Toru and TURKIN,  Yuri and WOLF, Robert and YAMADA,  Ichihiro and YANAI, Ryoma and YANAI, Ryohma and YASUHARA,  Ryo and YOKOYAMA,  Masayuki and YOSHIMURA,  Yasuo and YOSHINUMA,  Mikirou and ZHANG, Daihong and W7-X Team and LHD Experimental Group},
 issue = {22},
 journal = {Physical Review Letters},
 month = {Nov},
 note = {0000-0001-9585-5201, We assess the magnetic field configuration in modern fusion devices by comparing experiments with the same heating power, between a stellarator and a heliotron. The key role of turbulence is evident in the optimized stellarator, while neoclassical processes largely determine the transport in the heliotron device. Gyrokinetic simulations elucidate the underlying mechanisms promoting stronger ion scale turbulence in the stellarator. Similar plasma performances in these experiments suggests that neoclassical and turbulent transport should both be optimized in next step reactor designs.},
 title = {Impact of Magnetic Field Configuration on Heat Transport in Stellarators and Heliotrons},
 volume = {127},
 year = {2021}
}