Implications of a strongly peaked polar magnetic field N. R. Sheeley Jr.Y. -M. WangC. R. DeVore OriginalPaper Pages: 1 - 13
Wave behavior in the solar photosphere: A comparison of theory and observation Ciro MarmolinoRobin T. Stebbins OriginalPaper Pages: 23 - 36
Spectroscopic observations and models of umbral light bridges M. Sobotka OriginalPaper Pages: 37 - 52
Coronal holes as indicators of large-scale magnetic fields in the corona V. N. ObridkoB. D. Shelting OriginalPaper Pages: 73 - 80
Average properties of bipolar magnetic regions during sunspot cycle 21 Y. -M. WangN. R. Sheeley Jr. OriginalPaper Pages: 81 - 100
Magnetic and boundary effects on thermal instabilities in solar magnetic fields: Localized modes in a slab geometry P. J. CargillA. W. Hood OriginalPaper Pages: 101 - 127
Anomalous resistivity as the possible cause of fast reconnection in the solar corona S. I. Vainshtein OriginalPaper Pages: 129 - 144
The spectrum of coronal sources at millimetre and centimetre waves V. N. BorovikG. B. GelfreikhS. Urpo OriginalPaper Pages: 157 - 166
Solar wind observations with the ion composition instrument aboard the ISEE-3/ICE spacecraft K. W. OgilvieM. A. CoplanJ. Geiss OriginalPaper Pages: 167 - 183
Densities in the quiet sun and coronal holes using EUV emission lines Bhola N. Dwivedi Solar Physics Letters Pages: 185 - 188
Changes of the chromosphere model during “umbral flashes” S. A. GrigoryevaI. P. TurovaR. B. Teplitskaya Solar Physics Letters Pages: 189 - 192
