scholarly journals Low-Energy Enhancement of Magnetic Dipole Radiation

2013 ◽  
Vol 111 (23) ◽  
Author(s):  
R. Schwengner ◽  
S. Frauendorf ◽  
A. C. Larsen
2017 ◽  
Vol 118 (9) ◽  
Author(s):  
R. Schwengner ◽  
S. Frauendorf ◽  
B. A. Brown

2014 ◽  
Vol 22 (9) ◽  
pp. 10693 ◽  
Author(s):  
D. L. Markovich ◽  
P. Ginzburg ◽  
A. K. Samusev ◽  
P. A. Belov ◽  
A. V. Zayats

1983 ◽  
Vol 101 ◽  
pp. 505-507
Author(s):  
A. I. Tsygan

It is shown that pulsars that have ceased to generate electron-positron pairs (switched-off radiopulsars) may be the sources of X-ray and γ-ray radiation. The magnetic dipole radiation from these rotating neutron stars is transformed near the “light radius” into hard radiation by the plasma that is created due to ionization of interstellar neutral hydrogen.


Nature ◽  
1969 ◽  
Vol 221 (5179) ◽  
pp. 454-456 ◽  
Author(s):  
JAMES E. GUNN ◽  
JEREMIAH P. OSTRIKER

2011 ◽  
Author(s):  
J. Li ◽  
T. Higuchi ◽  
N. Kanda ◽  
K. Konishi ◽  
M. Kuwata-Gonokami

Low energy electrons have been used as an excitation source to reinvestigate the visible luminescence spectrum of pure solid nitrogen. Particular attention has been given to the interpretation of the α( 2 D– 4 S) emission within the ground state configuration of trapped nitrogen atoms. The spectral intensity distribution within α was photoelectrically recorded with a variety of excitation energies and at a number of different temperatures between that of liquid helium and liquid hydrogen. Decay curves for these features and the results of flow experiments are discussed. The components that comprise the α emission are shown to arise as dipole radiation from N atoms in at least five sites within the N 2 lattice, one of which is a surface site.


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