Zobrazeno 1 - 10
of 49
pro vyhledávání: '"D.E. Rees"'
Publikováno v:
IEEE Transactions on Electron Devices. 42:780-784
Some accelerator designs require that the amount of RF power supplied to the accelerating cavities be varied along the accelerator length. In order to minimize operating expense for a high-power, CW system, it is also desirable to maximize RF-generat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a275da2bf7728110247dce135911fe71
https://doi.org/10.1109/16.372084
https://doi.org/10.1109/16.372084
Publikováno v:
Journal of Microwave Power and Electromagnetic Energy. 30:158-164
This paper presents the characterization of a high-power klystrode amplifier as a RF source for particle accelerator applications. The klystrode is a relatively new type [Preist and Shrader, 1991; Preist and Shrader, 1982; Loring and Shrader, 1993; S
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ac4e0003ef306d2111c5538ae851ae92
https://doi.org/10.1080/08327823.1995.11688272
https://doi.org/10.1080/08327823.1995.11688272
Publikováno v:
IEEE Transactions on Electron Devices. 40:1543-1548
A method for calculating the loaded Q and beam detuning of a passive (gain or idler) cavity in an electron device is presented. It is based on the determination of induced current by a technique often referred to as Ramo's theorem. The induced curren
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::848ca6809f6f08920fd2ed2c0966f4fa
https://doi.org/10.1109/16.223717
https://doi.org/10.1109/16.223717
Autor:
D.C. Nguyen, P.L. Colestock, S.S. Kurennoy, D.E. Rees, A.H. Regan, S. Russell, D.L. Schrage, R.L. Wood, L.M. Young, T. Schultheiss, V. Christina, M. Cole, J. Rathke, J. Shaw, C. Eddy, R. Holm, R. Henry, J. Yater
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ad340a0610d5ab12b070ec8fd335f840
https://doi.org/10.1016/b978-0-444-51727-2.50023-7
https://doi.org/10.1016/b978-0-444-51727-2.50023-7
Publikováno v:
Proceedings of International Conference on Particle Accelerators.
This paper describes an automated procedure for testing the high-power klystron amplifiers used in the Ground Test Accelerator (GTA). To verify klystron performance, we have developed an automated test system using data-acquisition and control progra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::82831294c43ada736def94416d1301d3
https://doi.org/10.1109/pac.1993.308643
https://doi.org/10.1109/pac.1993.308643
Publikováno v:
Proceedings of International Conference on Particle Accelerators.
The magnicon is a new type of high-efficiency deflection-modulated amplifier developed at the Institute of Nuclear Physics in Novosibirsk, Russia. The prototype pulsed magnicon achieved an output power of 2.4 MW and an efficiency of 73% at 915 MHz. T
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::63c97e4281dbcf567a76903a03533064
https://doi.org/10.1109/pac.1993.308645
https://doi.org/10.1109/pac.1993.308645
Contaminant plumes are significant waste problems that require remediation in both the government and private sectors. The authors are developing an in situ process that uses RF/microwave stimulation to remove pollutants from contaminated soils. This
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::74b47f760bfad952a77d4ef1281b0116
https://doi.org/10.2172/102158
https://doi.org/10.2172/102158
Publikováno v:
Biological Psychology. 37:48
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c48356a1ad5dbeef24a33f467fb39a16
https://doi.org/10.1016/0301-0511(93)90034-6
https://doi.org/10.1016/0301-0511(93)90034-6
Publikováno v:
The Astrophysical Journal. 296:268
Dynamic models of flux tubes were used to interpret the presence of mass motions with large velocity gradients associated with spatially unresolved magnetic elements in the solar photosphere. A downflow was necessary in order to concentrate the magne
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1353ff706b1c0be3c3ff39b6b8990878
https://doi.org/10.1086/163444
https://doi.org/10.1086/163444
Publikováno v:
The Astrophysical Journal. 339:1093
Two numerical methods for formal integration of the Stokes transfer equations for line formation in a strong magnetic field were tested by computing Stokes profiles for a Zeeman triplet in a Milne-Eddington model atmosphere, and for the anomalously s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::edc1f357965a32b7ee2dc8ca6b9b143d
https://doi.org/10.1086/167364
https://doi.org/10.1086/167364