Comments on forbidden sulphur I lines in the solar spectrum J. W. Swensson Research Note Pages: 31 - 34
Analysis of the chromospheric hydrogen spectrum at the 1962 eclipse William Henze Jr. OriginalPaper Pages: 65 - 76
Periodic structures in quiescent prominences Y. NakagawaJ. McKim Malville OriginalPaper Pages: 102 - 115
Interferometric investigation of the red and green coronal lines during the total solar eclipse of May 30, 1965 A. B. DeloneE. A. Makarova OriginalPaper Pages: 116 - 130
Magnetic fields and the structure of the solar corona Martin D. AltschulerGordon Newkirk Jr. OriginalPaper Pages: 131 - 149
On the localization, size and structure of the regions of the X-ray flares on the Sun I. L. BeigmanYu. I. GrinevaI. A. Žitnik OriginalPaper Pages: 160 - 165
A magnetohydrodynamic approach for interpreting solar polarization bursts at 7 GHz O. T. Matsuura OriginalPaper Pages: 173 - 182
Coronal densities and magnetic fields from K-coronameter and type IV radio burst data J. David BohlinM. Simon OriginalPaper Pages: 183 - 193
On the origin of type II and IV radio sources during flares observed by a radioheliograph on 80 MHz L. Křivský Research Note Pages: 194 - 197
Flare-time sudden enhancements of low frequency field strength and associated meter wave solar radio bursts S. K. AlurkarR. V. Bhonsle OriginalPaper Pages: 198 - 204
On astronomical seeing: The single Schlieren model Ulrich Grossmann-Doerth OriginalPaper Pages: 210 - 224
Absolute calibration method and technique of the daily patrol of the solar flux density at 1470 MHz J. Priese OriginalPaper Pages: 235 - 240
Algonquin radio observatory, Lake Traverse, Ont., Canada Arthur E. Covington Report from Solar Institute Pages: 241 - 245
Solar research at the Catania Astrophysical Observatory G. Godoli Report from Solar Institute Pages: 246 - 249