scholarly journals A GW-level Ku-band oversized coaxial relativistic Cerenkov generator with low guiding magnetic field

AIP Advances ◽  
2019 ◽  
Vol 9 (6) ◽  
pp. 065006 ◽  
Author(s):  
Xiaoling Wu ◽  
Changhua Chen ◽  
Yan Teng ◽  
Ping Wu ◽  
Renzhen Xiao ◽  
...  
Keyword(s):  
IEEE Access ◽  
2021 ◽  
pp. 1-1
Author(s):  
Fangchao Dang ◽  
Fuxiang Yang ◽  
Xingjun Ge ◽  
Xinhe Wu ◽  
Xiaoping Zhang

2014 ◽  
Vol 85 (8) ◽  
pp. 084702 ◽  
Author(s):  
Junpu Ling ◽  
Jiande Zhang ◽  
Juntao He ◽  
Lei Wang ◽  
Bingfang Deng
Keyword(s):  

2014 ◽  
Vol 32 (2) ◽  
pp. 295-303 ◽  
Author(s):  
Jun-Pu Ling ◽  
Jun-Tao He ◽  
Jian-De Zhang ◽  
Tao Jiang ◽  
Li-Li Song

AbstractA novel coaxial relativistic transit-time oscillator with low guiding magnetic field is proposed and investigated to generate high power microwave at Ku-band. With the coaxial structure and a quasi body wave adopted as the operating mode, the device has a larger space-charge limiting current, higher power handling capacity, and lower guiding magnetic field. Moreover, for further improving the output power, a coaxial TM02mode resonant reflector is well designed. Main structure parameters of the device are optimized by particle in cell simulations. A typical simulation result is that, with a 358 keV, 7.25 kA beam guided by a magnetic field of about 0.7 T, an 810 MW microwave pulse at 14.25 GHz is generated, yielding a conversion efficiency of about 31%. The primary experiments are also carried out. At a low guiding magnetic field of 0.7 T, a microwave pulse with power of 400 MW, pulse duration of 30 ns, frequency of 14.3 GHz close to the simulation one, and efficiency of 15.4% is generated.


1967 ◽  
Vol 31 ◽  
pp. 381-383
Author(s):  
J. M. Greenberg

Van de Hulst (Paper 64, Table 1) has marked optical polarization as a questionable or marginal source of information concerning magnetic field strengths. Rather than arguing about this–I should rate this method asq+-, or quarrelling about the term ‘model-sensitive results’, I wish to stress the historical point that as recently as two years ago there were still some who questioned that optical polarization was definitely due to magnetically-oriented interstellar particles.


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