Reversed-polarity structures of chromospheric magnetic field Wei LiGuoxiang AiHongqi Zhang OriginalPaper Pages: 1 - 14
The covariance of latitudinal and longitudinal motions of small magnetic features R. W. KommR. F. HowardJ. W. Harvey OriginalPaper Pages: 15 - 28
Solar line identifications in the calcium isoelectronic sequence S. O. Kastner OriginalPaper Pages: 41 - 49
How bright is the [Si X] 1431 nm coronal emission line? M. J. PennJ. R. Kuhn OriginalPaper Pages: 51 - 56
The three-dimensional structures of X-ray bright points C. E. ParnellE. R. PriestL. Golub OriginalPaper Pages: 57 - 74
Dynamical fine structure of a quiescent filament N. MeinP. MeinJ. E. Wiik OriginalPaper Pages: 75 - 89
A coronal magnetic field model with horizontal volume and sheet currents Xuepu ZhaoJ. Todd Hoeksema OriginalPaper Pages: 91 - 105
The dynamics of driven magnetic reconnection in coronal arcades G. J. RickardE. R. Priest OriginalPaper Pages: 107 - 127
Vertical current and a 3B/X12 flare in a highly sheared active region (NOAA 6659) on June 9, 1991 Hongqi ZhangTongjiang Wang OriginalPaper Pages: 129 - 136
Formation of fast magnetosonic shock waves during a two-current-loop collision in solar flares Shinji KoideJun-Ichi Sakai OriginalPaper Pages: 137 - 145
High-energy gamma-ray emission from solar flares: Constraining the accelerated proton spectrum David AlexanderPhilip P. DunphyAlexander L. MacKinnon OriginalPaper Pages: 147 - 167
The shape of the sunspot cycle David H. HathawayRobert M. WilsonEdwin J. Reichmann OriginalPaper Pages: 177 - 190
Dissipation of fast magnetoacoustic waves in a cold plasma G. B. LaingP. M. Edwin Solar physics letters Pages: 191 - 194
An explanation for the flare frequency - energy dependence Yu. E. Litvinenko Solar physics letters Pages: 195 - 198