scholarly journals Complex Type III-like radio emissions observed from 1 to 14 MHz

1999 ◽  
Vol 26 (3) ◽  
pp. 397-400 ◽  
Author(s):  
M. J. Reiner ◽  
M. L. Kaiser
1980 ◽  
Vol 86 ◽  
pp. 299-302
Author(s):  
T. Takakura

By the use of semi-analytical method, modeling of three kinds of type III solar radio bursts have been made. Many basic problems about the type III bursts and associated solar electrons have been solved showing some striking or unexpected results. If the fundamental radio emissions should be really observed as the normal type III bursts, the emission mechanism would not be the currently accepted one, i.e. the scattering of plasma waves by ions.


2011 ◽  
Vol 60 (4) ◽  
pp. 645-648
Author(s):  
Katsunori Yazawa ◽  
Junji Ide ◽  
Hiroshi Mizuta

Solar Physics ◽  
2008 ◽  
Vol 249 (2) ◽  
pp. 337-354 ◽  
Author(s):  
M. J. Reiner ◽  
K.-L. Klein ◽  
M. Karlický ◽  
K. Jiřička ◽  
A. Klassen ◽  
...  
Keyword(s):  
Type Iii ◽  

Author(s):  
Zety Sharizat Hamidi ◽  
N.N.M. Shariff

Variation of solar bursts due to solar flares such as type an isolated type III , a complex type III, U is being highlighted. These bursts occurred on 9th March 2012 at the National Space Centre, Sg. Lang, Selangor, Malaysia Here, we study a unique case with a combination of two types burst associated with solar flare and CMEs. Our observation is focused on the low frequency region starting from 150 MHz till 400 MHz. We found that a solar flare type solar flare type M 6.3 which occurred in active region AR 1429 starting from 3:32 UT and ending at 05:00 UT. The flare has been confirmed to be the largest flare since 2005. Some physical parameters will be measured. We then compared our results with X-ray data from NOAA Space Weather Prediction Centre (SWPC).


2000 ◽  
Vol 530 (2) ◽  
pp. 1049-1060 ◽  
Author(s):  
M. J. Reiner ◽  
M. Karlicky ◽  
K. Jiřička ◽  
H. Aurass ◽  
G. Mann ◽  
...  

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