論文

査読有り
2015年2月

The criteria of flushing phenomena under microwave heating

JOURNAL OF NUCLEAR SCIENCE AND TECHNOLOGY
  • Tatsunori Yamaki
  • ,
  • Yutaka Abe
  • ,
  • Akiko Kaneko
  • ,
  • Tomoomi Segawa
  • ,
  • Koichi Kawaguchi
  • ,
  • Yoshikazu Yamada
  • ,
  • Kan-ichi Fujii

52
2
開始ページ
241
終了ページ
250
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1080/00223131.2014.946567
出版者・発行元
TAYLOR & FRANCIS LTD

In the microwave heating (MH) de-nitration method developed in Japan, a mixed solution of uranyl nitrate and plutonium nitrate recovered from the spent fuel in the reprocessing plant is converted directly to mixed oxide (MH-MOX) powder. This MH-MOX powder is utilized to fabricate MOX fuel with UO2 powder for FBR. The MH method is accompanied with transient boiling phenomena such as overflow and flushing. Toward high-speed and high-capacity conversion by MH-method in the future, it is required to avoid overflow and flushing and to understand optimal conditions for design and operation. At the first step for these objectives, basic knowledge of transient boiling phenomena by the MH-method has been acquired with using distilled water. It is observed that generation of singular bubble triggers flushing and distilled water just before flushing is superheated by a temperature 10 degrees C higher than boiling temperature. Based on these results, it is clarified that the occurrence criteria of flushing correlate with absorbed power in the water and released power from the water surface.

リンク情報
DOI
https://doi.org/10.1080/00223131.2014.946567
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000347532500010&DestApp=WOS_CPL
Scopus
https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84920784157&origin=inward 本文へのリンクあり
Scopus Citedby
https://www.scopus.com/inward/citedby.uri?partnerID=HzOxMe3b&scp=84920784157&origin=inward
ID情報
  • DOI : 10.1080/00223131.2014.946567
  • ISSN : 0022-3131
  • eISSN : 1881-1248
  • SCOPUS ID : 84920784157
  • Web of Science ID : WOS:000347532500010

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