Determination of the coronal magnetic field and the radio-emitting electron energy from a Type IV solar radio burst

Solar Physics ◽  
1968 ◽  
Vol 5 (4) ◽  
pp. 531-545 ◽  
Author(s):  
Reuven Ramaty ◽  
Richard E. Lingenfelter
Solar Physics ◽  
2013 ◽  
Vol 289 (1) ◽  
pp. 251-261 ◽  
Author(s):  
V. Vasanth ◽  
S. Umapathy ◽  
Bojan Vršnak ◽  
Tomislav Žic ◽  
O. Prakash

Solar Physics ◽  
1984 ◽  
Vol 90 (2) ◽  
Author(s):  
J.-L. Bougeret ◽  
J.H. King ◽  
R. Schwenn

Solar Physics ◽  
1971 ◽  
Vol 20 (2) ◽  
pp. 438-447 ◽  
Author(s):  
George A. Dulk ◽  
Martin D. Altschuler

1963 ◽  
Vol 16 (4) ◽  
pp. 526 ◽  
Author(s):  
AA Weiss

Properties of 24 sources of type IV emission at metre wavelengths (including the long-lived continuum storms) have been observed by interferometry in the frequency range 40-70 Mc/s and by dynamic spectroscopy in the frequency range 15-210 Mc/s. The characteristics investigated are the positions, movements, and angular sizes of the sources, and the spectrum and polarization of the emission.


2016 ◽  
Vol 121 (7) ◽  
pp. 6141-6156 ◽  
Author(s):  
B. Li ◽  
Iver H. Cairns ◽  
J. T. Gosling ◽  
D. M. Malaspina ◽  
D. Neudegg ◽  
...  

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