On the influence of gradients in the angular velocity on the solar meridional motions Bernard R. Durney OriginalPaper Pages: 1 - 32
Validity of the isobaric assumption to the solar corona R. W. WalshG. E. BellA. W. Hood OriginalPaper Pages: 33 - 45
Fe XXI emission line ratios as electron temperature diagnostics for the coronae of cool stars F. P. KeenanV. J. FosterK. G. Widing OriginalPaper Pages: 47 - 53
Modulational instability of self-generated magnetic fields X. Q. LiZ. D. Zhang OriginalPaper Pages: 69 - 77
Gradients of the line-of-sight magnetic fields in active region NOAA 6659 Yang LiuJingxiu WangGuoxiang Ai OriginalPaper Pages: 79 - 89
Topology and current ribbons: A model for current, reconnection and flaring in a complex, evolving corona D. W. Longcope OriginalPaper Pages: 91 - 121
A filament eruption and accompanying coronal field changes on November 5, 1992 A. H. McAllisterH. KurokawaN. Nitta OriginalPaper Pages: 123 - 149
MHD shock interactions in coronal structures S. A. GribS. KoutchmyV. N. Sazonova OriginalPaper Pages: 151 - 166
A large arcade along the inversion line, observed on May 19, 1992 by Yohkoh, and enhancement of interplanetary energetic particles Shinichi WatariT. DetmanJ. A. Joselyn OriginalPaper Pages: 167 - 179
A joint analysis of high-energy neutrons and neutron-decay protons from a flare L. G. KocharovJ. TorstiI. G. Usoskin OriginalPaper Pages: 181 - 207
Radial dependence of solar wind parameters in the ecliptic (1.1 R ⊙−61 AU) W. Köhnlein OriginalPaper Pages: 209 - 213
Rescaled range analysis of the asymmetry of solar activity R. OliverJ. L. Ballester OriginalPaper Pages: 215 - 224
