Solar rotation measurements at Mount Wilson Barry J. LabonteRobert Howard OriginalPaper Pages: 3 - 12
A mechanism for solar ultraviolet flux variability Kenneth H. SchattenDonald F. Heath OriginalPaper Pages: 13 - 23
On the temporal variation of the solar continuous brightness fluctuations B. Hadjebi OriginalPaper Pages: 25 - 35
Preliminary observation of missing energy flux of sunspot Tadashi HirayamaTomizo Okamoto OriginalPaper Pages: 37 - 43
The He i 10 830 Å chromosphere and filament associated structures Marie K. McCabeD. L. Mickey OriginalPaper Pages: 59 - 66
Role of plasma flow in determining structure of the chromosphere-corona transition zone of the sun W. M. Glencross OriginalPaper Pages: 67 - 79
Measuring electron density in coronal active regions J. -C. NoensJ. -L. Leroy OriginalPaper Pages: 81 - 87
Current confinement in solar coronal loops Claudio ChiuderiGiorgio Einaudi OriginalPaper Pages: 89 - 103
Analysis of the high-resolution x-ray spectra obtained aboard the intercosmos 16 satellite V. V. KrutovV. V. KorneevS. Vasha OriginalPaper Pages: 105 - 119
Height structure of thermal hard x-ray sources on the sun John C. BrownJohn Hayward OriginalPaper Pages: 121 - 132
Forerunners: Early coronal manifestations of solar mass ejection events Bernard V. Jackson OriginalPaper Pages: 133 - 144
Hydrodynamic response of the solar chromosphere to an elementary flare burst B. V. SomovS. I. SyrovatskiiA. R. Spektor OriginalPaper Pages: 145 - 155
Internal structure of reconnecting current sheets and the emerging flux model for solar flares A. M. MilneE. R. Priest OriginalPaper Pages: 157 - 181
A comparison of type III metric radio bursts and global solar potential field models Bernard V. JacksonRandolph H. Levine OriginalPaper Pages: 183 - 190
Langmuir-wave conversion as the explanation of moving type IV solar meter-wave radio outbursts R. A. Duncan OriginalPaper Pages: 191 - 204
Comment on ‘first phase acceleration mechanisms and implications for hard x-ray burst models in solar flares’ Gerard Van Hoven Research Note Pages: 205 - 205