Extremely High Peak Power Obtained at 29 GHZ Microwave Pulse Generation

التفاصيل البيبلوغرافية
العنوان: Extremely High Peak Power Obtained at 29 GHZ Microwave Pulse Generation
المؤلفون: M. I. Yalandin, M. S. Pedos, Ilya V. Romanchenko, Marat R. Ul'maskulov, S. N. Rukin, Konstantin A. Sharypov, Vladislav V. Rostov, A. V. Gunin, S. A. Shunailov
المصدر: Russian Physics Journal. 60:1325-1331
بيانات النشر: Springer Science and Business Media LLC, 2017.
سنة النشر: 2017
مصطلحات موضوعية: 010302 applied physics, Materials science, business.industry, Phase (waves), General Physics and Astronomy, Pulse duration, Particle accelerator, Nanosecond, 01 natural sciences, 010305 fluids & plasmas, law.invention, Pulse (physics), Full width at half maximum, Optics, law, 0103 physical sciences, Backward-wave oscillator, business, Microwave
الوصف: The paper presents research results on enhancing the peak power of microwave pulses with sub- and nanosecond length using a backward-wave oscillator (BWO) operating at 29 GHz frequency and possessing a reproducible phase structure. Experiments are conducted in two modes on a high-current electron accelerator with the required electron beam power. In the first (superradiation) mode, which utilizes the elongated slow-wave structure, the BWO peak power is 3 GW at 180 ns pulse duration (full width at halfmaximum, FWHM). In the second (quasi-stationary) mode, the BWO peak power reaches 600 MW at ~2 ns pulse duration (FWHM). The phase spread from pulse to pulse can vary from units to several tens of percent in a nanosecond pulse mode. The experiments do not show any influence of microwave breakdown on the BWO power generation and radiation pulse duration.
تدمد: 1573-9228
1064-8887
DOI: 10.1007/s11182-017-1216-2
URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_________::faa0a0ea44798b8bdef697b971b85767
https://doi.org/10.1007/s11182-017-1216-2
Rights: CLOSED
رقم الانضمام: edsair.doi...........faa0a0ea44798b8bdef697b971b85767
قاعدة البيانات: OpenAIRE
الوصف
تدمد:15739228
10648887
DOI:10.1007/s11182-017-1216-2