Development of a second cyclotron harmonic gyrotron operating at submillimeter wavelengths

1992 ◽  
Vol 4 (1) ◽  
pp. 267-273 ◽  
Author(s):  
T. Idehara ◽  
T. Tatsukawa ◽  
I. Ogawa ◽  
H. Tanabe ◽  
T. Mori ◽  
...  
Keyword(s):  
Submillimeter Wavelengths ◽  
Harmonic Gyrotron ◽  
Cyclotron Harmonic

High‐frequency, step tunable, cyclotron harmonic gyrotron

1991 ◽  
Vol 3 (7) ◽  
pp. 1766-1772 ◽  
Author(s):  
Toshitaka Idehara ◽  
Toshiaki Tatsukawa ◽  
Hidehiko Tanabe ◽  
Satoru Matsumoto ◽  
Kohji Kunieda ◽  
...  
Keyword(s):  
High Frequency ◽  
Harmonic Gyrotron ◽  
Cyclotron Harmonic

Development of high frequency, cyclotron harmonic gyrotron oscillator

1988 ◽  
Vol 132 (6-7) ◽  
pp. 344-346 ◽  
Author(s):  
Toshitaka Idehara ◽  
Toshiaki Tatsukawa ◽  
Satoru Matsumoto ◽  
Kohji Kunieda ◽  
Kazuhisa Hemmi ◽  
...  
Keyword(s):  
High Frequency ◽  
Gyrotron Oscillator ◽  
Harmonic Gyrotron ◽  
Cyclotron Harmonic

Development of a second cyclotron harmonic gyrotron operating at 0.8 mm wavelength

1990 ◽  
Vol 56 (18) ◽  
pp. 1743-1745 ◽  
Author(s):  
T. Idehara ◽  
T. Tatsukawa ◽  
I. Ogawa ◽  
H. Tanabe ◽  
T. Mori ◽  
...  
Keyword(s):  
Harmonic Gyrotron ◽  
Cyclotron Harmonic

Automodulation instability in gyrotrons operating at the second cyclotron harmonic

2021 ◽  
Vol 28 (4) ◽  
pp. 043303
Author(s):  
A. P. Fokin ◽  
V. L. Bakunin ◽  
M. Yu. Glyavin ◽  
G. S. Nusinovich
Keyword(s):  
Cyclotron Harmonic

scholarly journals Excitation mechanism in the intracluster filaments surrounding the Brightest Cluster Galaxies

2019 ◽  
Vol 15 (S359) ◽  
pp. 185-187
Author(s):  
Fiorella L. Polles
Keyword(s):  
Active Galactic Nuclei ◽  
Galactic Nuclei ◽  
Elliptical Galaxies ◽  
Cluster Galaxies ◽  
Cooling Flow ◽  
Submillimeter Wavelengths ◽  
Hot Plasma ◽  
Brightest Cluster Galaxies ◽  
Multi Phase ◽  
The Impact

AbstractMulti-phase filamentary structures surrounding giant elliptical galaxies at the center of cool-core clusters, the Brightest Cluster Galaxies (BCGs), have been detected from optical to submillimeter wavelengths. The source of the ionisation in the filaments is still debated. Studying the excitation of these structures is key to our understanding of Active Galactic Nuclei (AGN) feedback in general, and more precisely of the impact of environmental and local effects on star formation. One possible contributor to the excitation of the filaments is the thermal radiation from the cooling of the hot plasma surrounding the BCGs, the so-called cooling flow.

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