Home > Publications database > Simulation of Orbit Correction and Synchrotron Radiation Aspects in the Upgraded HERA Interaction Regions > print

001     301896
005     20211110134753.0
024 7 _ |a 10.3204/PUBDB-2016-02955
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037 _ _ |a PUBDB-2016-02955
041 _ _ |a English
088 1 _ |a DESY-M-00-04ZK
088 _ _ |a DESY-M-00-04ZK
|2 DESY
100 1 _ |a Montag, C.
|0 P:(DE-HGF)0
|b 0
|e Corresponding author
111 2 _ |a The 7th European Particle Accelerator Conference EPAC 2000
|g EPAC 2000
|c Vienna
|d 2000-06-26 - 2000-06-30
|w Austria
245 _ _ |a Simulation of Orbit Correction and Synchrotron Radiation Aspects in the Upgraded HERA Interaction Regions
260 _ _ |a Hamburg
|c 2000
|b DESY
300 _ _ |a 370-372
336 7 _ |a CONFERENCE_PAPER
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336 7 _ |a Conference Paper
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336 7 _ |a INPROCEEDINGS
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336 7 _ |a Contribution to a conference proceedings
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520 _ _ |a In the upgraded HERA interaction regions, about 30kW of synchrotron radiation have to be passed safely through the high energy physics detectors. At a distance of about 11m from the interaction point a fraction of this synchrotron radiation is absorbed, while the remaining part is passed further on through the separated beam pipes. To protect the vacuum chamber between the IP and the 11m absorber against accidential mis-steering of the synchrotron radiation fan, four emergency absorbers are installed. On the other hand the HERA detectors are very sensitive to backgrounds from backscattered synchrotron radiation photons. The aperture of absorbers and other elements in the downstrem beamline have to be chosen such as to guarantee acceptable background conditions even with moderately missteered electron beams. To investigate the feasibility of this scheme, extensive simulations have been carried out taking into account realistic machine errors, such as magnet misalignments, monitor errors, optics distortions, etc. It is shown that under realistic conditions the synchrotron radiationfan can be safely controlled.
536 _ _ |a No facility / HGF program None (POF1-890)
|0 G:(DE-H253)POF1-HGF-No-Prog-20130405
|c POF1-890
|x 0
588 _ _ |a Dataset connected to INSPIRE
650 _ 7 |a talk: Vienna 2000/06/26
|2 INSPIRE
650 _ 7 |a electron p: storage ring
|2 INSPIRE
650 _ 7 |a luminosity: upgrade
|2 INSPIRE
650 _ 7 |a synchrotron radiation
|2 INSPIRE
650 _ 7 |a radiation protection
|2 INSPIRE
650 _ 7 |a shielding
|2 INSPIRE
650 _ 7 |a alignment: error
|2 INSPIRE
650 _ 7 |a numerical calculations
|2 INSPIRE
650 _ 7 |a DESY HERA Stor
|2 INSPIRE
693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
|5 EXP:(DE-MLZ)NOSPEC-20140101
|e No specific instrument
|x 0
700 1 _ |a Stulle, F.
|0 P:(DE-HGF)0
|b 1
787 0 _ |a Decking, Winfried
|d Hamburg : DESY, 2000
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|0 PUBDB-2016-02907
|r DESY-M-00-04; C00-06-26.2
|t Contributions to the 7th European Particle Accelerator Conference EPAC 2000
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913 2 _ |a DE-HGF
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913 1 _ |b Programmorientierte Förderung
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