scholarly journals Development of LB film taste sensor for beer degradation evaluation and its physical properties

2019 ◽  
Vol 102 (11) ◽  
pp. 47-54 ◽  
Author(s):  
Masayoshi Yazawa ◽  
Kazunari Takahashi ◽  
Hidekazu Uchida ◽  
Yuki Hasegawa
Keyword(s):  
Physical Properties ◽  
Lb Film ◽  
Degradation Evaluation ◽  
Taste Sensor

Development of LB Film Taste Sensor for Beer Degradation Evaluation and its Physical Properties

2019 ◽  
Vol 139 (9) ◽  
pp. 289-295
Author(s):  
Masayoshi Yazawa ◽  
Kazunari Takahashi ◽  
Hidekazu Uchida ◽  
Yuki Hasegawa
Keyword(s):  
Physical Properties ◽  
Lb Film ◽  
Degradation Evaluation ◽  
Taste Sensor

scholarly journals Mixed Taste Material Identification with LB Film Taste Sensor

2009 ◽  
Vol 129 (2) ◽  
pp. 47-52 ◽  
Author(s):  
Satoshi Hasebe ◽  
Takamichi Hirata ◽  
Masahiro Akiya
Keyword(s):  
Material Identification ◽  
Lb Film ◽  
Taste Sensor

Optical Taste Sensor Using Dye-Doped Hetero-Structured LB film

2007 ◽  
Author(s):  
Masayuki Morisawa ◽  
Koji Miyazawa ◽  
Shinzo Muto
Keyword(s):  
Lb Film ◽  
Taste Sensor

scholarly journals Mono-channel taste sensor using LB film

2000 ◽  
Vol 120 (12) ◽  
pp. 588-592 ◽  
Author(s):  
Jun Matsuzaki ◽  
Hitoshi Takano ◽  
Masahiro Akiya
Keyword(s):  
Lb Film ◽  
Taste Sensor

Optrode-Type POF Taste Sensor Using Dye Doped Hetero-Structured LB Film

2006 ◽  
Author(s):  
Masayuki Morisawa ◽  
Koji Miyazawa ◽  
Shinzo Muto
Keyword(s):  
Lb Film ◽  
Taste Sensor

Study for Electrode Metals on Taste Sensor with LB film

2009 ◽  
Vol 129 (10) ◽  
pp. 338-343
Author(s):  
Takahiro Yokoya ◽  
Takamichi Hirata ◽  
Masahiro Akiya
Keyword(s):  
Lb Film ◽  
Taste Sensor

The Photometric Properties of the Ap Stars

1976 ◽  
Vol 32 ◽  
pp. 365-377 ◽  
Author(s):  
B. Hauck
Keyword(s):  
Physical Properties ◽  
Ap Stars

The Ap stars are numerous - the photometric systems tool It would be very tedious to review in detail all that which is in the literature concerning the photometry of the Ap stars. In my opinion it is necessary to examine the problem of the photometric properties of the Ap stars by considering first of all the possibility of deriving some physical properties for the Ap stars, or of detecting new ones. My talk today is prepared in this spirit. The classification by means of photoelectric photometric systems is at the present time very well established for many systems, such as UBV, uvbyβ, Vilnius, Geneva and DDO systems. Details and methods of classification can be found in Golay (1974) or in the proceedings of the Albany Colloquium edited by Philip and Hayes (1975).

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