Title of article
Generation of powerful ultrashort electromagnetic pulses based on superradiance
Author/Authors
Ginzburg، نويسنده , , N.S and Zotova، نويسنده , , I.V and Novozhilova، نويسنده , , Yu.V. and Sergeev، نويسنده , , A.S. and Phelps، نويسنده , , A.D.R and Cross، نويسنده , , A.W. and Wiggins، نويسنده , , S.M. and Ronald، نويسنده , , K. and Shpak، نويسنده , , V.G and Yalandin، نويسنده , , M.I and Shunailov، نويسنده , , S.A and Ulmaskulov، نويسنده , , M.R.، نويسنده ,
Pages
6
From page
385
To page
390
Abstract
Experimental results of the observation of superradiation from intense, subnanosecond electron bunches moving through a periodic waveguide and interacting with a backward propagating TM01 wave are presented. The ultra-short microwave pulses in Ka, W, and G band were generated with repetition frequencies of up to 25 Hz. Observation of RF breakdown of ambient air, as well as direct measurements by hot-carrier germanium detectors, leads to an estimate of the peak power as high as 60–120 MW for the 300–400 ps pulses at 38 GHz. The initial observation of 75 GHz 10–15 MW radiation pulses with duration less than 150 ps, and of 150 GHz microwave spikes with a risetime of 75ps are also reported. Comparison with simulations is discussed as well.
Keywords
Cherenkov emission , Electron bunch , COHERENCE
Journal title
Astroparticle Physics
Record number
2017911
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