scholarly journals Magnetic-field symmetry of dynamic capacitances

1997 ◽  
Vol 55 (4) ◽  
pp. R1946-R1949 ◽  
Author(s):  
T. Christen ◽  
M. Büttiker
Keyword(s):  
Magnetic Field ◽  
Field Symmetry

Molecular Rovibronic Symmetries in Electric and Magnetic Fields

1975 ◽  
Vol 53 (19) ◽  
pp. 2210-2220 ◽  
Author(s):  
James K. G. Watson
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Electric Field ◽  
Symmetry Groups ◽  
Nuclear Spins ◽  
Symmetry Classification ◽  
Electric And Magnetic Fields ◽  
Field Symmetry ◽  
Point Groups

The structures of the symmetry groups for the rovibronic levels of a molecule in a homogeneous electric or magnetic field are derived, and the symmetry classification of the levels in terms of the representations and corepresentations of these groups is discussed. Specific results are given for molecules of the point groups C3, C2v, C3v, D2d, and Td in an electric field. Symmetry in combined electric and magnetic fields and the inclusion of nuclear spins are considered briefly.

scholarly journals Magnetic Field Symmetry and Phase Rigidity of the Nonlinear Conductance in a Ring

2006 ◽  
Vol 96 (12) ◽  
Author(s):  
R. Leturcq ◽  
D. Sánchez ◽  
G. Götz ◽  
T. Ihn ◽  
K. Ensslin ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Field Symmetry ◽  
Nonlinear Conductance

scholarly journals Magnetic field symmetry and phase rigidity of the nonlinear conductance in a ring

2007 ◽  
Author(s):  
R. Leturcq ◽  
R. Bianchetti ◽  
G. Götz ◽  
T. Ihn ◽  
K. Ensslin ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Field Symmetry ◽  
Nonlinear Conductance

scholarly journals Inductive lenses for improved magnetic field symmetry in a corrugated theta-pinch coil

1969 ◽  
Vol 9 (3) ◽  
pp. 233-238
Author(s):  
F. Hartz ◽  
J. Junker ◽  
F. Pohl ◽  
G.H. Wolf
Keyword(s):  
Magnetic Field ◽  
Theta Pinch ◽  
Field Symmetry

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.

Observing the galactic magnetic field

1967 ◽  
Vol 31 ◽  
pp. 375-380
Author(s):  
H. C. van de Hulst
Keyword(s):  
Magnetic Field ◽  
Fair Agreement ◽  
Solar Neighbourhood ◽  
Galactic Magnetic Field ◽  
The Magnetic Field

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.

Sign in / Sign up

Export Citation Format

Share Document