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.

引用

页数：8

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