Retrieving information from digital solar radio spectrograms

2008 ◽  
pp. 83-92 ◽  
Author(s):  
Andre Csillaghy
Keyword(s):  
Solar Radio

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.

The Heights of Solar Radio Sources at 1424 MHz and 696 MHz

1969 ◽  
Vol 1 (5) ◽  
pp. 192-194 ◽  
Author(s):  
D. G. Cole ◽  
R. F. Mullaly
Keyword(s):  
Solar Activity ◽  
High Resolution ◽  
Solar Disk ◽  
Previous Investigation ◽  
Solar Radio ◽  
Radio Sources ◽  
Grating Interferometer ◽  
Maximum Solar Activity

The heights of solar radio sources at 1424 MHz and 696 MHz have been measured during the years 1965 and 1966. Solar activity at this time was near minimum. The number of radio sources appearing on the solar disk rarely exceeded three at any time and it thus was possible to resolve the majority of these with a high resolution grating interferometer. Many of the previous height measurements at these frequencies have been made near times of maximum solar activity and the confusion of sources within the beam has limited their accuracy. The number of sources studied here is quite considerably higher than in any previous investigation at these frequencies, and the period of observation has been continuous.

Mid-term Periodicities in Solar Radio Emission Corresponding to Sunspot Number During Solar Cycle 23

Solar Physics ◽  
2021 ◽  
Vol 296 (3) ◽  
Author(s):  
Mahender Aroori ◽  
Panditi Vemareddy ◽  
Partha Chowdhury ◽  
Ganji Yellaiah
Keyword(s):  
Solar Cycle ◽  
Radio Emission ◽  
Sunspot Number ◽  
Solar Radio ◽  
Solar Radio Emission ◽  
Solar Cycle 23

scholarly journals A statistical study of solar radio Type III bursts and space weather implication

2020 ◽  
Author(s):  
Theogene Ndacyayisenga ◽  
Jean Uwamahoro ◽  
K. Sasikumar Raja ◽  
Christian Monstein
Keyword(s):  
Space Weather ◽  
Solar Radio ◽  
Statistical Study ◽  
Type Iii

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

Flare-plasma diagnostics from millisecond pulsations of the solar radio emission

2002 ◽  
Vol 46 (6) ◽  
pp. 497-514 ◽  
Author(s):  
V. F. Melnikov ◽  
G. D. Fleishman ◽  
Q. J. Fu ◽  
G.-L. Huang
Keyword(s):  
Radio Emission ◽  
Plasma Diagnostics ◽  
Solar Radio ◽  
Solar Radio Emission ◽  
Flare Plasma

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
Sign in / Sign up

Export Citation Format

Share Document