Ion Drift Velocities in Gaseous Mixtures at Arbitrary Field Strengths

1972 ◽  
Vol 5 (1) ◽  
pp. 438-441 ◽  
Author(s):  
E. A. Mason ◽  
Hong-sup Hahn
Keyword(s):  
Arbitrary Field ◽  
Gaseous Mixtures ◽  
Ion Drift ◽  
Field Strengths

scholarly journals Nonlinear electrophoresis at arbitrary field strengths: small-Dukhin-number analysis

2014 ◽  
Vol 26 (12) ◽  
pp. 122002 ◽  
Author(s):  
Ory Schnitzer ◽  
Ehud Yariv
Keyword(s):  
Arbitrary Field ◽  
Field Strengths

Zeeman diamagnetism in hydrogen at arbitrary field strengths

1986 ◽  
Vol 19 (7) ◽  
pp. L215-L219 ◽  
Author(s):  
P C Rech ◽  
M R Gallas ◽  
J A C Gallas
Keyword(s):  
Arbitrary Field ◽  
Field Strengths

Harmonic mixing in a cosine potential for large damping and arbitrary field strengths

1982 ◽  
Vol 28 (4) ◽  
pp. 335-339 ◽  
Author(s):  
H. -J. Breymayer ◽  
H. Risken ◽  
H. D. Vollmer ◽  
W. Wonneberger
Keyword(s):  
Arbitrary Field ◽  
Harmonic Mixing ◽  
Field Strengths

Magnetic Resonance for Arbitrary Field Strengths

1955 ◽  
Vol 98 (4) ◽  
pp. 927-933 ◽  
Author(s):  
Roald K. Wangsness
Keyword(s):  
Magnetic Resonance ◽  
Arbitrary Field ◽  
Field Strengths

Magnetic-field strengths from optical polarization data

1967 ◽  
Vol 31 ◽  
pp. 381-383
Author(s):  
J. M. Greenberg
Keyword(s):  
Magnetic Field ◽  
Optical Polarization ◽  
Polarization Data ◽  
Term Model ◽  
Source Of Information ◽  
Field Strengths

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.

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