Techniques for Identifying and Measuring High Order Modes in RF Cavities Metadata

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Title

  • Main Title Techniques for Identifying and Measuring High Order Modes in RF Cavities

Creator

  • Author: Goldberg, D.A.
    Creator Type: Personal
  • Author: Rimmer, R.A.
    Creator Type: Personal

Contributor

  • Sponsor: Lawrence Berkeley Laboratory. Accelerator & Fusion Research Division.
    Contributor Type: Organization

Publisher

  • Name: Lawrence Berkeley National Laboratory
    Place of Publication: Berkeley, California
    Additional Info: Ernest Orlando Lawrence Berkeley National Laboratory, Berkeley, CA (United States)

Date

  • Creation: 1997-05-01

Language

  • English

Description

  • Content Description: We report on a number of techniques which can be used to unravel the higher-order-mode spectrum of an RF cavity. Most of these techniques involve the application of basic symmetry principles and require for their application only that the cavity exhibit some basic symmetry, possibly broken by the presence of couplers, apertures, etc., which permits a classification of these modes in terms of some property characterized by that symmetry, e.g., multipolarity for a cavity which is basically a figure of revolution. Several examples of the application of these techniques are given.
  • Physical Description: 17

Subject

  • Keyword: Classification
  • Keyword: Apertures
  • Keyword: Cavities
  • STI Subject Categories: 43
  • STI Subject Categories: 99
  • Keyword: Symmetry
  • Keyword: Multipolarity

Source

  • Journal Name: Nuclear Instruments and Methods in Physics Research A

Collection

  • Name: Office of Scientific & Technical Information Technical Reports
    Code: OSTI

Institution

  • Name: UNT Libraries Government Documents Department
    Code: UNTGD

Resource Type

  • Article

Format

  • Text

Identifier

  • Report No.: LBNL-40290
  • Grant Number: DE-AC02-05CH11231
  • Office of Scientific & Technical Information Report Number: 1004688
  • Archival Resource Key: ark:/67531/metadc839532
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