On the solar type III radio burst emission process

1982 ◽  
Vol 256 ◽  
pp. 271 ◽  
Author(s):  
D. G. Wentzel



2013 ◽  
Vol 118 (7) ◽  
pp. 4039-4052 ◽  
Author(s):  
G. Thejappa ◽  
R. J. MacDowall ◽  
M. Bergamo


2012 ◽  
Vol 747 (1) ◽  
pp. L1 ◽  
Author(s):  
G. Thejappa ◽  
R. J. MacDowall ◽  
M. Bergamo ◽  
K. Papadopoulos




2010 ◽  
Author(s):  
Urs Ganse ◽  
Thomas Burkart ◽  
Felix Spanier ◽  
Rami Vainio ◽  
M. Maksimovic ◽  
...  


2019 ◽  
Vol 875 (2) ◽  
pp. 98 ◽  
Author(s):  
Atul Mohan ◽  
Surajit Mondal ◽  
Divya Oberoi ◽  
Colin J. Lonsdale
Keyword(s):  
Type Iii ◽  


Solar Physics ◽  
1972 ◽  
Vol 26 (2) ◽  
pp. 468-473 ◽  
Author(s):  
H. Alvarez ◽  
F. Haddock ◽  
R. P. Lin


1980 ◽  
Vol 4 (1) ◽  
pp. 62-64 ◽  
Author(s):  
C. S. Wright

Solar type III radio bursts often occur for prolonged periods (≳ 1 hour) with small time intervals (≲ 1 minute) between bursts. Such phenomena usually are confined to decametre wavelengths (frequency ≲ 100 MHz) and are called ‘type III storms’ (e.g. Stewart and Labrum 1972).



2005 ◽  
Vol 431 (1) ◽  
pp. 353-357 ◽  
Author(s):  
R. Ramesh ◽  
A. Satya Narayanan ◽  
C. Kathiravan ◽  
Ch. V. Sastry ◽  
N. Udaya Shankar


1981 ◽  
Vol 251 ◽  
pp. 364 ◽  
Author(s):  
R. P. Lin ◽  
D. W. Potter ◽  
D. A. Gurnett ◽  
F. L. Scarf


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