On the directional dependence of the emission of acoustic noise by convective turbulence in a gravitational atmosphere M. Kuperus OriginalPaper Pages: 257 - 262
Some properties of velocity fields in the solar photosphere Franz-Ludwig Deubner OriginalPaper Pages: 263 - 275
Spectral analyses of solar photospheric fluctuations Frank N. Edmonds Jr.Carol J. Webb OriginalPaper Pages: 276 - 296
Turbulent velocity in undisturbed and active photosphere O. G. BadalyanM. A. Livshits OriginalPaper Pages: 297 - 306
The interpretation of total line intensities from optically thin gases J. T. JefferiesF. Q. OrrallJ. B. Zirker OriginalPaper Pages: 307 - 316
The interpretation of total line intensities from optically thin gases J. T. JefferiesF. Q. OrrallJ. B. Zirker OriginalPaper Pages: 317 - 326
The interpretation of total line intensities from optically thin gases J. T. JefferiesF. Q. OrrallJ. B. Zirker OriginalPaper Pages: 327 - 343
Inhomogeneous structure of the solar chromosphere from Lyman-continuum data J. E. VernazzaR. W. Noyes OriginalPaper Pages: 358 - 374
Multi-component models for the formation of the chromospheric Caii K line L. E. Cram OriginalPaper Pages: 375 - 386
A model for the chromosphere-corona transition region based on radio observations and on hydrodynamical conservation equations P. Lantos OriginalPaper Pages: 387 - 401
On the filamentary nature of solar magnetic fields Robert HowardJ. O. Stenflo OriginalPaper Pages: 402 - 417
The mean photospheric magnetic field from solar magnetograms: Comparisons with the interplanetary magnetic field Philip H. ScherrerJohn M. WilcoxRobert Howard OriginalPaper Pages: 418 - 424
Suppression of the kink instability for magnetic flux ropes in the chromosphere M. A. Raadu OriginalPaper Pages: 425 - 433
Differential rotation and the structure and energy content of coronal magnetic fields M. A. Raadu OriginalPaper Pages: 443 - 449
Observed heights of EUV lines formed in the transition zone and corona George W. SimonRobert W. Noyes OriginalPaper Pages: 450 - 458
The normalization of solar X-ray data from many experiments Charles D. Wende OriginalPaper Pages: 492 - 502