Heliophysics with radio scintillation and occultation

Heliophysics ◽  
2016 ◽  
pp. 289-326 ◽  
Author(s):  
Mario M. Bisi
Keyword(s):  
Icarus ◽  
2015 ◽  
Vol 252 ◽  
pp. 301-310 ◽  
Author(s):  
Tomoya Iju ◽  
Shinsuke Abe ◽  
Munetoshi Tokumaru ◽  
Ken’ichi Fujiki

1992 ◽  
Vol 128 ◽  
pp. 287-289
Author(s):  
O. A. Kuz'min

AbstractRegular structure with 10 to 50kHz-scale was detected in the radio scintillation spectrum of PSR 1919+21. This regular structure may be a simple interferometric pattern formed by refractive multi-ray propagation between the pulsar and observer. It was found that the pulsar PSR 1919+21 radio emission scintillation spectrum phase changes significantly across the average profile. Within the refractive scattering scenario this phase-longitude dependence corresponds to a transversal shift of the magnetosphere emitting region of about 6 x 108 cm. The radio emission altitude is estimated to be near the light cylinder.


2000 ◽  
Vol 105 (A5) ◽  
pp. 10435-10453 ◽  
Author(s):  
Munetoshi Tokumaru ◽  
Masayoshi Kojima ◽  
Ken'ichi Fujiki ◽  
Atsushi Yokobe

1989 ◽  
Vol 94 (A2) ◽  
pp. 1473 ◽  
Author(s):  
Richard Woo ◽  
William L. Sjogren ◽  
Janet G. Luhmann ◽  
Arvydas J. Kliore ◽  
Larry H. Brace

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