The determination of the velocity amplitude of the total photospheric motion field N. N. KondrashovaE. A. Gurtovenko OriginalPaper Pages: 291 - 298
Determination of electron temperature of quiescent prominences by hydrogen lines N. N. Morozhenko OriginalPaper Pages: 303 - 308
Non-thermal line broadening in the solar chromosphere R. A. E. Fosbury Research Note Pages: 309 - 311
On intensity ratios of helium and hydrogen lines in quiescent prominences N. N. Morozhenko OriginalPaper Pages: 313 - 322
Spatial distribution of soft X-ray and EUV emission associated with a chromospheric flare of importance 1B on August 2, 1972 W. M. NeupertR. J. ThomasR. D. Chapman OriginalPaper Pages: 349 - 375
A correlation between time-overlapping solar flares and the release of energetic particles G. M. Simnett OriginalPaper Pages: 377 - 391
Kilometer-wave type III burst: Harmonic emission revealed by direction and time of arrival Hector AlvarezFred T. HaddockWilliam H. Potter OriginalPaper Pages: 413 - 420
Comments on ‘neutralization and stabilization of particle streams in the corona and type III radio bursts’ by Dean F. Smith D. B. Melrose OriginalPaper Pages: 421 - 425
On a suggested explanation for fine structures observed in some wide-band bursts W. N.-C. Sy OriginalPaper Pages: 427 - 431
Decameter type IV bursts associated with coronal transients T. E. GergelyM. R. Kundu OriginalPaper Pages: 433 - 446
The coronal transient of 16 June 1972 Martin KoomenRussell HowardShirley Hansen OriginalPaper Pages: 447 - 452
Coronal magnetic structure at a solar sector boundary John M. WilcoxLeif Svalgaard OriginalPaper Pages: 461 - 470
Implications of the reported low energy electron gradients J. A. LezniakW. R. Webber OriginalPaper Pages: 477 - 489
