scholarly journals The origin of the frequency-dependent behaviour of pulsar radio profiles

2014 ◽  
Vol 446 (3) ◽  
pp. 2505-2522 ◽  
Author(s):  
J. Dyks ◽  
B. Rudak
2000 ◽  
Vol 177 ◽  
pp. 535-536
Author(s):  
D. Khechinashvili ◽  
G. Melikidze ◽  
J. Gil

AbstractWe suggest that companions of two binary eclipsing pulsars, B1957+20 and J2051-0827, are degenerate magnetic dwarfs. The magnetospheres of the white dwarfs are infused with relativistic particles supplied by the pulsar wind. We demonstrate that the radio waves emitted by the pulsars are strongly damped due to cyclotron resonance with the plasma particles, in the magnetospheres of companions. Large stable continuos and frequency-dependent radio eclipses should occur as a result of this process. This agrees well with observations.


1992 ◽  
Vol 29 (4) ◽  
pp. 321-328
Author(s):  
J. Rohan Lucas

Inclusion of frequency dependent losses in transformer flux-current excursions This paper presents a model for the frequency dependent losses in the transformer core for transient studies. The non-integer power series approach is extended to include the frequency dependent behaviour of the losses. The results obtained are compared with manufacturer's data and are found to give a very good fit.


1972 ◽  
Vol 8 (4) ◽  
pp. 81 ◽  
Author(s):  
J.D. Maines ◽  
F.G. Marshall ◽  
J.F.C. Oliver ◽  
E.G.S. Paige

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