scholarly journals Fast radio bursts and cosmological tests

2019 ◽  
Vol 484 (2) ◽  
pp. 1637-1644 ◽  
Author(s):  
M Jaroszynski
1994 ◽  
Vol 144 ◽  
pp. 283-284
Author(s):  
G. Maris ◽  
E. Tifrea

The type II solar radio bursts produced by a shock wave passing through the solar corona are one of the most frequently studied solar activity phenomena. The scientific interest in this type of phenomenon is due to the fact that the presence of this radio event in a solar flare is an almost certain indicator of a future geophysical effect. The origin of the shock waves which produce these bursts is not at all simple; besides the shocks which are generated as a result of a strong energy release during the impulsive phase of a flare, there are also the shocks generated by a coronal mass ejection or the shocks which appear in the interplanetary space due to the supplementary acceleration of the solar particles.


2020 ◽  
Vol 248 (3309) ◽  
pp. 18
Author(s):  
Jonathan O'Callaghan
Keyword(s):  

Author(s):  
Sergei B. Popov ◽  
Konstantin A. Postnov ◽  
Maxim S. Pshirkov
Keyword(s):  

2012 ◽  
Vol 2 (10) ◽  
pp. 1-3 ◽  
Author(s):  
Praveen Kumar Gupta ◽  
◽  
Puspraj Singh Puspraj Singh ◽  
Puspraj Singh Puspraj Singh ◽  
P. K. Chamadia P. K. Chamadia

2021 ◽  
Vol 64 (4) ◽  
Author(s):  
Di Xiao ◽  
FaYin Wang ◽  
ZiGao Dai
Keyword(s):  

GPS Solutions ◽  
2021 ◽  
Vol 25 (2) ◽  
Author(s):  
Yu. V. Yasyukevich ◽  
A. S. Yasyukevich ◽  
E. I. Astafyeva

Author(s):  
E. Petroff ◽  
J. W. T. Hessels ◽  
D. R. Lorimer
Keyword(s):  

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