Partial reconstruction of the initial conditions for streams of energetic electrons associated with a solar type III burst

Solar Physics ◽  
1984 ◽  
Vol 94 (1) ◽  
pp. 165-170 ◽  
Author(s):  
R. J. -M. Grognard
Keyword(s):  
Initial Conditions ◽  
Energetic Electrons ◽  
Type Iii ◽  
Partial Reconstruction ◽  
Solar Type

Energetic electrons and plasma waves associated with a solar type III radio burst

1981 ◽  
Vol 251 ◽  
pp. 364 ◽  
Author(s):  
R. P. Lin ◽  
D. W. Potter ◽  
D. A. Gurnett ◽  
F. L. Scarf
Keyword(s):  
Radio Burst ◽  
Plasma Waves ◽  
Energetic Electrons ◽  
Type Iii ◽  
Solar Type

WindSpacecraft Observations of Solar Impulsive Electron Events Associated with Solar Type III Radio Bursts

1998 ◽  
Vol 503 (1) ◽  
pp. 435-445 ◽  
Author(s):  
R. E. Ergun ◽  
D. Larson ◽  
R. P. Lin ◽  
J. P. McFadden ◽  
C. W. Carlson ◽  
...  
Keyword(s):  
Radio Bursts ◽  
Type Iii ◽  
Solar Type

scholarly journals First Observation of the Solar Type III Burst Decay and Its Interpretation

2019 ◽  
Vol 885 (1) ◽  
pp. 78 ◽  
Author(s):  
V. N. Melnik ◽  
A. A. Konovalenko ◽  
S. M. Yerin ◽  
I. M. Bubnov ◽  
A. I. Brazhenko ◽  
...  
Keyword(s):  
Type Iii ◽  
Solar Type

Unusual Absorption of a Solar Type II Burst by ‘Shadow’ Type III Bursts

1974 ◽  
Vol 57 ◽  
pp. 245-248
Author(s):  
K. Kai
Keyword(s):  
Band Structure ◽  
Absorption Feature ◽  
Spectral Features ◽  
Type Ii ◽  
Type Iii ◽  
Solar Type ◽  
Split Band

(Proc. Astron. Soc. Australia). The Hα-flare on 1968 August 23d23h45m was followed by a short-lived type II burst. The radio spectrograph record obtained at Culgoora is shown in Figure 1. The type II burst was of split-band structure with unusual spectral features in each component of the split band. The most remarkable one is an absorption feature between 23h52m02s and 23h52m10s: suppression of the bright type II emission along an ‘inverted U’ (between 120 and 85 MHz).

Sign in / Sign up

Export Citation Format

Share Document