For the HERA luminosity upgrade the horizontal emit-tance of the electron beam was reduced from 41 nm to 22 nm firstly by an increased quadrupole focusing in the arcs’ FODO structures and secondly by a change of the damp-ing partition numbers by means of an rf frequency shift. The stronger focusing alone, which increases the phase ad-vance per FODO cell from 60 to 72 degrees, would only reduce the emittance to 35 nm. It was therefore critical for the luminosity upgrade to make sure that there is sufficient room in the damping window for increasing the frequency of HERA’s 500 MHz system by the required 300 Hz. For this purpose HERA’s rf frequency had to be compared to the central frequency of the ring, for which the design or-bit goes throug...
The Hydrogen Epoch of Reionization Array (HERA) is a radio interferometer aiming to detect the power...
After the design luminosity has been exceeded in the electron–proton collider HERA, the interaction ...
© 2020. The American Astronomical Society. All rights reserved. The central challenge in 21 cm cosmo...
For the HERA luminosity upgrade the horizontal emittance of the electron beam was reduced from 41 nm...
The HERA accelerator study periods during 2000 were mainly concerned with issues of the luminosity u...
DESY is currently working on decreasing the size of the proton beam and of the electron beam in HERA...
DESY is currently working on decreasing the size of the proton beam and of the electron beam in HERA...
After the luminosity upgrade of the electron proton collider HERA, the proton bunch length will beco...
The HERA luminosity upgrade, scheduled to take place in 2001, presents a major modifica-tion of the ...
EPAC 2000, Vienna DESY is currently working on decreasing the size of the proton beam and of the ele...
The collision of both beams in the HERA storage ring is performed by the guidance of the electron be...
The linear optics of both HERA electron and proton ring have been measured with several methods, inc...
Ground motion and impcrfcct filtering of the power sup-plies result in micrometer level transverse o...
As demonstrated in many accelerators, luminosity scans can be used to measure the beam overlap integ...
After the design luminosity had been exceeded in the electron–proton collider HERA, the interaction ...
The Hydrogen Epoch of Reionization Array (HERA) is a radio interferometer aiming to detect the power...
After the design luminosity has been exceeded in the electron–proton collider HERA, the interaction ...
© 2020. The American Astronomical Society. All rights reserved. The central challenge in 21 cm cosmo...
For the HERA luminosity upgrade the horizontal emittance of the electron beam was reduced from 41 nm...
The HERA accelerator study periods during 2000 were mainly concerned with issues of the luminosity u...
DESY is currently working on decreasing the size of the proton beam and of the electron beam in HERA...
DESY is currently working on decreasing the size of the proton beam and of the electron beam in HERA...
After the luminosity upgrade of the electron proton collider HERA, the proton bunch length will beco...
The HERA luminosity upgrade, scheduled to take place in 2001, presents a major modifica-tion of the ...
EPAC 2000, Vienna DESY is currently working on decreasing the size of the proton beam and of the ele...
The collision of both beams in the HERA storage ring is performed by the guidance of the electron be...
The linear optics of both HERA electron and proton ring have been measured with several methods, inc...
Ground motion and impcrfcct filtering of the power sup-plies result in micrometer level transverse o...
As demonstrated in many accelerators, luminosity scans can be used to measure the beam overlap integ...
After the design luminosity had been exceeded in the electron–proton collider HERA, the interaction ...
The Hydrogen Epoch of Reionization Array (HERA) is a radio interferometer aiming to detect the power...
After the design luminosity has been exceeded in the electron–proton collider HERA, the interaction ...
© 2020. The American Astronomical Society. All rights reserved. The central challenge in 21 cm cosmo...