Microbunch Instability Observations from a THz Detector at Diamond Light Source

被引：13
|
作者：
Shields, W. [1 ]
Bartolini, R. [2 ,3 ]
Boorman, G. [1 ]
Karataev, P. [1 ]
Lyapin, A. [1 ]
Puntree, J. [3 ]
Rehm, G. [2 ]
机构：
[1] Univ London, John Adams Inst, Egham TW20 0EX, Surrey, England
[2] Diamond Light Source, Oxford, England
[3] Univ Oxford, John Adams Inst, Oxford OX1 3RH, England
来源：
IX INTERNATIONAL SYMPOSIUM ON RADIATION FROM RELATIVISTIC ELECTRONS IN PERIODIC STRUCTURES (RREPS-2011) | 2012年 / 357卷
关键词：
D O I：
10.1088/1742-6596/357/1/012037
中图分类号：
TH7 [仪器、仪表];
学科分类号：
0804 ; 080401 ; 081102 ;
摘要：
Diamond Light source is a third generation synchrotron facility dedicated to producing radiation of outstanding brightness, ranging from infra-red to x-rays. The short electron bunches that are accelerated around the storage ring are susceptible to the phenomenon of microbunching instabilities when the bunch charge exceeds a threshold. The primary feature of the microbunch instabilities is the onset of bursts of radiation in the THz range. The high frequencies involved in the emissions make detection and analysis challenging. A 60-90 GHz Schottky Barrier Diode detector was installed to investigate turn by turn evolution of the instabilities.
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页数：8
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