RF technology workshop, Amsterdam, October 4 - PowerPoint PPT Presentation

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RF technology workshop, Amsterdam, October 4

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All current activity revolves ... Main design challenge is reduction of heat load through: ... Increasing Din Spot size increases which lowers power density ... – PowerPoint PPT presentation

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Title: RF technology workshop, Amsterdam, October 4


1
  • All current activity revolves around 6 lines per
    port
  • Initial 6-beamline option still had too high a
    heat load on front mirror
  • Main design challenge is reduction of heat load
    through
  • Wider waveguides ? Resulting beams lead to lower
    power density
  • ? This will help all options since 6 lines per
    port leave more room for this
  • Increasing Din ? Spot size increases which
    lowers power density
  • ? Only possible in combination with measures to
    limit front mirror size
  • Decreasing angle of incidence ? this decreases
    loss factor on mirror
  • Only possible with higher launching position
    (not desirable)
  • or second front mirror per line

Result 2 options
1 end mirror for 3 beam lines 2 x 3 on 1 option
2 end mirrors per beam line Dogleg option
2
2 x 3 on 1 option
3
2 x 3 on 1 option
  • Pros
  • Smaller end mirror surface when wider waveguides
    are used. This leads to a lower heat load on the
    end mirror.
  • Cons
  • Since each end mirror controls three beams,
    there is less freedom in aiming the beams slight
    variation in Alpha / Beta angle.
  • Mirrors most likely grow larger in length than
    earlier options with 1 line per mirror.
  • Hole in front shield needs to be higher then
    earlier 6-beamline option. However, it can be
    more narrow.
  • Placing the components at rear end of the port
    plug will prove to be difficult.

4
Dogleg option
5
Dogleg option
  • Pros
  • Launching positions can be placed lower and
    closer to the front shield
  • Dog leg drastically reduces neutron streaming
    towards rear end of the plug, since waveguides do
    not face the plasma
  • Front shield penetration is much smaller
  • Mirrors are a lot smaller and are therefore
    easier to handle
  • Less problems with placing components in the
    launcher interspace in the rear.
  • Cut in lower blanket module is not required
  • First mirror after waveguide can be used for
    both upper and lower row
  • More flexible design due to increased number of
    parameters
  • Scanning range through waveguide can be lower
    (/- 10 deg) for at least three beamlines
  • Cons
  • 9 Mirrors are required in the front shield,
    which leads to a higher amount of total power
    that needs to be cooled away
  • Scanning range measured in degrees is larger
    then with any other option this requires a
    higher degree of accuracy in the steering
    mechanism and mirror surfaces.
  • Less shielding can be realised for area above
    the port plug, as compared to previous options.
  • ? There is still some room for further
    optimisation

6
Qualitative comparison
Blue 6 beamline option Purple 2 x 3 on 1
option Green Dogleg option
Conclusion When comparing nominal spot sizes on
the absorption plane, it appears that the dogleg
option outperforms all recent launcher options! ?
More time is needed to do exact calculations to
determine the overall performance
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