Powerful solar radio bursts as a global and free tool for testing satellite broadband radio systems, including GPS–GLONASS–GALILEO

2008 ◽  
Vol 70 (15) ◽  
pp. 1985-1994 ◽  
Author(s):  
E.L. Afraimovich ◽  
V.V. Demyanov ◽  
A.B. Ishin ◽  
G.Ya. Smolkov
Keyword(s):  
Solar Radio ◽  
Radio Bursts ◽  
Solar Radio Bursts ◽  
Broadband Radio ◽  
Radio Systems

Fine Spectral Structure of Solar Radio Storms

1980 ◽  
Vol 4 (1) ◽  
pp. 64-67 ◽  
Author(s):  
D. McConnell
Keyword(s):  
Radio Frequency ◽  
Radio Telescope ◽  
Solar Radio ◽  
High Time ◽  
Video Tape ◽  
Spectral Structure ◽  
Radio Bursts ◽  
Solar Radio Bursts ◽  
Broadband Radio ◽  
Radio Frequency Signals

As part of an investigation of solar radio bursts at high time (≈ 1 msec) and frequency (≈ 10 kHz) resolution, observations have been made between 30 MHz with the Llanherne broadband radio telescope (Ferris 1980). The radio frequency signals in the six frequency ranges 30-33, 33-36, 38-41, 54-57 and 79-82 MHz were recorded on six video tape recorders for about 10 minutes each day near solar transit.

Type II Solar Radio Bursts over Solar Cycle 21

1994 ◽  
Vol 144 ◽  
pp. 283-284
Author(s):  
G. Maris ◽  
E. Tifrea
Keyword(s):  
Solar Radio ◽  
Interplanetary Space ◽  
Impulsive Phase ◽  
Radio Bursts ◽  
Type Ii ◽  
Solar Radio Bursts ◽  
Strong Energy ◽  
Mass Ejection ◽  
Geophysical Effect ◽  
Radio Event

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.

scholarly journals How modernized and strengthened GPS signals enhance the system performance during solar radio bursts

GPS Solutions ◽  
2021 ◽  
Vol 25 (2) ◽  
Author(s):  
Yu. V. Yasyukevich ◽  
A. S. Yasyukevich ◽  
E. I. Astafyeva
Keyword(s):  
System Performance ◽  
Solar Radio ◽  
Radio Bursts ◽  
Solar Radio Bursts

An Observational Revisit of Stationary Type IV Solar Radio Bursts

Solar Physics ◽  
2021 ◽  
Vol 296 (2) ◽  
Author(s):  
Maoshui Lv ◽  
Yao Chen ◽  
V. Vasanth ◽  
Mohd Shazwan Radzi ◽  
Zamri Zainal Abidin ◽  
...  
Keyword(s):  
Solar Radio ◽  
Radio Bursts ◽  
Solar Radio Bursts ◽  
Type Iv ◽  
Stationary Type

Electron Exciter Speeds Associated with Interplanetary Type III Solar Radio Bursts

Solar Physics ◽  
2015 ◽  
Vol 290 (10) ◽  
pp. 2975-3004 ◽  
Author(s):  
M. J. Reiner ◽  
R. J. MacDowall
Keyword(s):  
Solar Radio ◽  
Radio Bursts ◽  
Solar Radio Bursts ◽  
Type Iii

Impacts of the December 2006 solar radio bursts on the performance of GPS

Radio Science ◽  
2009 ◽  
Vol 44 (1) ◽  
pp. n/a-n/a ◽  
Author(s):  
Charles S. Carrano ◽  
Christopher T. Bridgwood ◽  
Keith M. Groves
Keyword(s):  
Solar Radio ◽  
Radio Bursts ◽  
Solar Radio Bursts
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