scholarly journals Fretting wear under magnetic field

2010 ◽  
Author(s):  
Y. Nasu ◽  
K. Sato
Keyword(s):  
2000 ◽  
Vol 2000.1 (0) ◽  
pp. 539-540
Author(s):  
Kenkichi SATO ◽  
Jun HOMIZU ◽  
Hiroyuki FUJIMOTO ◽  
Yukio SATO
Keyword(s):  

Wear ◽  
2000 ◽  
Vol 241 (1) ◽  
pp. 99-108 ◽  
Author(s):  
K. Sato ◽  
T.A. Stolarski ◽  
Y. Iida
Keyword(s):  

2005 ◽  
Vol 2005.4 (0) ◽  
pp. 291-292
Author(s):  
Yusuke IIDA ◽  
Yuki NASU ◽  
Kenkichi SATO
Keyword(s):  

1967 ◽  
Vol 31 ◽  
pp. 381-383
Author(s):  
J. M. Greenberg

Van de Hulst (Paper 64, Table 1) has marked optical polarization as a questionable or marginal source of information concerning magnetic field strengths. Rather than arguing about this–I should rate this method asq+-, or quarrelling about the term ‘model-sensitive results’, I wish to stress the historical point that as recently as two years ago there were still some who questioned that optical polarization was definitely due to magnetically-oriented interstellar particles.


1967 ◽  
Vol 31 ◽  
pp. 375-380
Author(s):  
H. C. van de Hulst

Various methods of observing the galactic magnetic field are reviewed, and their results summarized. There is fair agreement about the direction of the magnetic field in the solar neighbourhood:l= 50° to 80°; the strength of the field in the disk is of the order of 10-5gauss.


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