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@INPROCEEDINGS{Soltwisch:201100,
      author       = {Soltwisch, H. and Kempkes, P. and Mackel, F. and Stein, H.
                      and Tenfelde, J. and Arnold, L. and Dreher, J. and Grauer,
                      R.},
      title        = {{F}lare{L}ab: early results},
      journal      = {Plasma physics and controlled fusion},
      volume       = {52},
      number       = {12},
      issn         = {1361-6587},
      address      = {Bristol},
      publisher    = {IOP Publ.},
      reportid     = {FZJ-2015-03405},
      pages        = {124030 -},
      year         = {2010},
      abstract     = {The FlareLab experiment at Bochum University has been
                      constructed to generate and investigate plasma-filled
                      magnetic flux tubes similar to arch-shaped solar
                      prominences, which often result in coronal mass ejections
                      (CMEs). In its first version, the device has been used to
                      reproduce and extend previous studies of Bellan et al (1998
                      Phys. Plasmas 5 1991). Here the plasma source consists of
                      two electrodes, which can be connected to a 1.0 kJ
                      capacitor bank, and of a horseshoe magnet, which provides an
                      arch-shaped guiding field. The discharge is ignited in a
                      cloud of hydrogen gas that has been puffed into the space
                      above the electrodes. In the first few microseconds the
                      plasma current rises at a rate of several kA µs−1,
                      causing the plasma column to pinch along the guiding B-field
                      and to form an expanding loop structure. The observed
                      dynamics of the magnetic flux tubes is analysed by means of
                      three-dimensional MHD simulations in order to determine the
                      influence of parameters like the initial magnetic field
                      geometry on magnetic stability. At present, FlareLab is
                      redesigned to mimic a model that was proposed by Titov and
                      Démoulin (1999 Astron. Astrophys. 351 707) to investigate
                      twisted magnetic configurations in solar flares.},
      month         = {Jun},
      date          = {2010-06-21},
      organization  = {37th European Physical Society
                       Conference on Plasma Physics, Dublin
                       (Ireland), 21 Jun 2010 - 25 Jun 2010},
      cin          = {JSC},
      ddc          = {530},
      cid          = {I:(DE-Juel1)JSC-20090406},
      pnm          = {411 - Computational Science and Mathematical Methods
                      (POF2-411)},
      pid          = {G:(DE-HGF)POF2-411},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)16},
      UT           = {WOS:000286181100031},
      doi          = {10.1088/0741-3335/52/12/124030},
      url          = {https://juser.fz-juelich.de/record/201100},
}