ATF2 Optics for the Commissioning Toshiyuki Okugi, KEK 2008 / 10/ 22 ATF2 commissioning meeting.

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Presentation transcript:

ATF2 Optics for the Commissioning Toshiyuki Okugi, KEK 2008 / 10/ 22 ATF2 commissioning meeting

Quadrupole definition of ATF2 beamline User Program K 1 =k 1 ×L eff /2 SaveATF2Optics K = K 1 ×2 LoadATF2Optics K 1 = K /2 K = k 1 ×L eff ATF2 Optics File Storage SaveATF2Optics and LoadATF2Optics Command Vsystem GUI SAD computer TCP-IP Quadrupole definition of old extraction line

! --- ATF2 optics deck read "/users/atfopr/sad/atf2daihonnew.sad"; FFS USE=ATF2; ! --- Library for “Load” and “Save” command Get["/users/atfopr/sad/atf2lib.n"]; ! --- Ver4.0 Design Optics LoadATF2Optics[“ATF2V40design”]; ! --- Optics for Radiation Inspection ! LoadATF2Optics[“ATF2Radiation”]; ! --- High Beta Optics ! LoadATF2Optics["ATF2HighBeta"]; cal; end; Example of the ATF2 optics calculation for SAD

Directory of optics file storage; /users/atfopr/sad/ringoptics/ Format of the file; qvatf2={{"QM6R", },{"QM7R", },{"QS1X",0},{"QF1X", },{"QD2X", }, {"QF3X", },{"QF4X", },{"QD5X", },{"QF6X", },{"QS2X",0}, {"QF7X", }, {"QD8X", },{"QF9X", },{"QK1X",0},{"QD10X", }, {"QF11X", },{"QK2X",0}, {"QD12X", },{"QF13X", },{"QD14X", }, {"QF15X", },{"QK3X",0}, {"QD16X", },{"QF17X", },{"QK4X",0}, {"QD18X", },{"QF19X", }, {"QD20X", },{"QF21X", }, {"QM16FF", },{"QM15FF", },{"QM14FF", }, {"QM13FF", }, {"QM12FF", },{"QM11FF",0},{"QD10BFF", },{"QD10AFF", }, {"QF9BFF", },{"QF9AFF", },{"QD8FF", },{"QF7FF", }, {"QD6FF", }, {"QF5BFF", },{"QF5AFF", },{"QD4BFF", }, {"QD4AFF", },{"QF3FF", }, {"QD2BFF", },{"QD2AFF", }, {"QF1FF", },{"QD0FF", } }; svatf2={ {"SF6FF", },{"SF5FF", },{"SD4FF", },{"SF1FF", }, {"SD0FF", } }; zvatf2={ {"ZH1X",0},{"ZH2X",0},{"ZH3X",0},{"ZH4X",0},{"ZH5X",0},{"ZH6X",0},{"ZH7X",0},{"ZH8X",0},{"ZH9X",0},{"ZH10X",0},{"ZV1X",0}, {"ZV2X",0},{"ZV3X",0},{"ZV4X",0},{"ZV5X",0},{"ZV6X",0},{"ZV7X",0},{"ZV8X",0},{"ZV9X",0},{"ZV10X",0},{"ZV11X",0},{"ZX1X",0}, {"ZX2X",0},{"ZX3X",0}}; If you prepare the same format of the file, you can easily apply the magnet setting with Vsystem control. Format of the optics file

Comment for SAD deck Since the definitions of SAD and MAD are different for the fringe field of the bending magnet, the differences of the fringe fields are compensated by the quadrupole strength in matching section (QM11FF to QM16FF) for SAD deck. ATF2 Ver4.0 Optics for SAD

QF1X QD2X QF3X QF4X QD5X QF6X QF7X QD8X QF9X QD10X 0 QF11X 0 QD12X 0 QF13X QD14X QF15X QD16X 0 QF17X 0 QD18X 0 QF19X 0 QD20X QF21X QM16FF 0 QM15FF 0 QM14FF 0 QM13FF 0 QM12FF 0 QM11FF 0 QD10BFF 0 QF9BFF 0 QF9AFF QD8FF QF7FF QD6FF 0 QF5BFF 0 QF5AFF 0 QD4BFF 0 QD4AFF 0 QF3FF QD2BFF QD2AFF QF1FF 0 QD0FF 0 O Optics for Radiation Inspection -Only 6 QEA magnets -Turned off the QEA magnets in extraction -No Laser Wire and Coupling Study

High Beta Optics Purpose of High Beta Optics -Turn on all magnets. - Orbit tuning with all magnet movers. - Make the small beam size for IP-BSM measurement

 y = 1e-11m  y = 0.08m Chromatic Effect of the High Beta Optics Simulation results for beam size enhancement for all sextupoles off Sextupole ? When the sextupoles turn on, we can make the nonlinear effect small after the tuning of the beam orbit correction at sextupoles. But, it make some possibility to make beam size growth by the sextupole fields.