Abstract
Diamond Light Source is a third generation synchrotron facility dedicated to producingradiation of outstanding brightness. Above a threshold current, the electron bunches aresusceptible to the phenomenon known as the microbunching instability. This instability ischaracterised by the onset of radiation bursts, the wavelength of which is shorter than thebunch length. Near threshold, the bursting occurs quasi-periodically, however at highercurrents, the bursting appears randomly. The high frequencies involved in these emissionsmake detection and analysis challenging. A port specifically for the investigation of mmwave emissions has recently been built at Diamond. Ultra fast Schottky Barrier Diodedetectors have been installed to observe the instability on a turn by turn basis. The onsetand evolution of the bunches have been investigated.
| Original language | English |
|---|---|
| Title of host publication | IPAC 2012 - International Particle Accelerator Conference 2012 |
| Pages | 3114-3116 |
| Number of pages | 3 |
| Publication status | Published - 2012 |
| Externally published | Yes |
| Event | 3rd International Particle Accelerator Conference 2012, IPAC 2012 - New Orleans, LA, United States Duration: 20 May 2012 → 25 May 2012 |
Conference
| Conference | 3rd International Particle Accelerator Conference 2012, IPAC 2012 |
|---|---|
| Country | United States |
| City | New Orleans, LA |
| Period | 20.5.12 → 25.5.12 |
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ASJC Scopus subject areas
- Nuclear and High Energy Physics
Cite this
Observations of microbunching instabilities from a THz port at diamond light source. / Shields, W.; Boorman, G.; Karataev, P.; Lyapin, A.; Bartolini, R.; Morgan, A.; Rehm, G.
IPAC 2012 - International Particle Accelerator Conference 2012. 2012. p. 3114-3116.Research output: Chapter in Book/Report/Conference proceeding › Conference contribution
}
TY - GEN
T1 - Observations of microbunching instabilities from a THz port at diamond light source
AU - Shields, W.
AU - Boorman, G.
AU - Karataev, P.
AU - Lyapin, A.
AU - Bartolini, R.
AU - Morgan, A.
AU - Rehm, G.
PY - 2012
Y1 - 2012
N2 - Diamond Light Source is a third generation synchrotron facility dedicated to producingradiation of outstanding brightness. Above a threshold current, the electron bunches aresusceptible to the phenomenon known as the microbunching instability. This instability ischaracterised by the onset of radiation bursts, the wavelength of which is shorter than thebunch length. Near threshold, the bursting occurs quasi-periodically, however at highercurrents, the bursting appears randomly. The high frequencies involved in these emissionsmake detection and analysis challenging. A port specifically for the investigation of mmwave emissions has recently been built at Diamond. Ultra fast Schottky Barrier Diodedetectors have been installed to observe the instability on a turn by turn basis. The onsetand evolution of the bunches have been investigated.
AB - Diamond Light Source is a third generation synchrotron facility dedicated to producingradiation of outstanding brightness. Above a threshold current, the electron bunches aresusceptible to the phenomenon known as the microbunching instability. This instability ischaracterised by the onset of radiation bursts, the wavelength of which is shorter than thebunch length. Near threshold, the bursting occurs quasi-periodically, however at highercurrents, the bursting appears randomly. The high frequencies involved in these emissionsmake detection and analysis challenging. A port specifically for the investigation of mmwave emissions has recently been built at Diamond. Ultra fast Schottky Barrier Diodedetectors have been installed to observe the instability on a turn by turn basis. The onsetand evolution of the bunches have been investigated.
UR - http://www.scopus.com/inward/record.url?scp=84885654740&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84885654740&partnerID=8YFLogxK
M3 - Conference contribution
AN - SCOPUS:84885654740
SN - 9783954501151
SP - 3114
EP - 3116
BT - IPAC 2012 - International Particle Accelerator Conference 2012
ER -