The influence of doubly excited levels on the ionization formula for the solar corona Walter Van Rensbergen OriginalPaper Pages: 354 - 360
On the origin of spicules in the chromosphere-corona transition region Max KuperusR. Grant Athay OriginalPaper Pages: 361 - 370
On the dome formation in the corona around a prominence observed at the total eclipse of 15 February 1961 Ichiro Kawaguchi OriginalPaper Pages: 420 - 436
Solar source of the interplanetary sector structure John M. WilcoxNorman F. Ness OriginalPaper Pages: 437 - 445
Electrons > 40 ke V and protons > 500 ke V of solar origin R. P. LinK. A. Anderson OriginalPaper Pages: 446 - 464
A high-resolution 2800 MHz multi-element interferometer A. E. CovingtonT. H. LeggM. B. Bell OriginalPaper Pages: 465 - 473
Occultation of a noise storm source during the partial solar eclipse of May 20, 1966 V. LetfusA. TlamichaB. Valníček OriginalPaper Pages: 474 - 477
Small-scale solar magnetic fields and ‘invisible sunspots’ Cornelis Zwaan Research Note Pages: 478 - 480
On the physical meaning of the Freundlich-Forbes empirical constant A. G. Gasanalizade Research Note Pages: 481 - 483
The Crimean Astrophysical Observatory A. SevernyN. Stepanyan Report from Solar Institute Pages: 484 - 486
The solar work at the Göttingen Observatory G. BrücknerE. SchröterH. H. Voigt Report from Solar Institute Pages: 487 - 493
Solar physics at the ‘Observatoire de Paris-Meudon’ R. Michard Report from Solar Institute Pages: 498 - 503
