The relation between flare-related metric continuum bursts and coronal mass ejections R. D. Robinson OriginalPaper Pages: 33 - 39
Discussion on the classification of fine structures in continua Ø. Elgarøy OriginalPaper Pages: 41 - 42
Exponential decay and exciter profile of fast pulses in type IV events Alberto AbramiMauro MesserottiPaolo Zlobec OriginalPaper Pages: 51 - 55
Electron-cyclotron maser emission from the sun and stars: Variations with plasma temperature and density R. M. WingleeG. A. Dulk OriginalPaper Pages: 93 - 97
The characteristics of type IV-associated spikes at metric wavelengths M. NoninoA. AbramiP. Zlobec OriginalPaper Pages: 111 - 116
Occurrence of solar decimetric spike bursts over a period of 4 years during the 21st cycle H. W. Urbarz OriginalPaper Pages: 125 - 129
Hollow beam distribution of energetic electrons and higher harmonics of electron cyclotron maser Hong Wei Li OriginalPaper Pages: 131 - 136
A model of ultra-fast fine structures of microwave bursts Ren-Yang ZhaoJian-Kui Shi OriginalPaper Pages: 137 - 144
Relative timing of hard X-rays and radio emissions during the different phases of solar flares: Consequences for the electron acceleration G. Trottet ReviewPaper Pages: 145 - 163
Radio observations of the solar neutron flare of 3 June, 1982 M. KarlickýH. AurassG. Mann OriginalPaper Pages: 165 - 168
Behaviour of the polarization at dm-m wavelengths during the evolution of five two-ribbon flares V. RuždjakB. VršnakA. Schroll OriginalPaper Pages: 169 - 174
Electron acceleration in flares inferred from radio and hard X-ray emissions A. O. BenzS. R. Kane OriginalPaper Pages: 179 - 185
Images of post-flare coronal structures in X-rays Zdeněk ŠvestkaPaul Hick OriginalPaper Pages: 187 - 190
Interpretation of temporal features in an unusual X-ray and microwave burst A. L. MackinnonJ. E. R. CostaB. R. Dennis OriginalPaper Pages: 191 - 198
Flare stars and solar bursts: High resolution in time and frequency Kenneth R. Lang OriginalPaper Pages: 227 - 233
Can observed hard X-ray and microwave flux from solar flares be explained by a single electron population? K. Kai OriginalPaper Pages: 235 - 241
Microwave diagnostics of energetic electrons in flares K.-L. KleinG. TrottetA. Magun OriginalPaper Pages: 243 - 252