Peculiar Features in the Solar Coronal Hole Occurrence Mirjam Y. HoferMarisa Storini OriginalPaper Pages: 1 - 10
Dependence of Supergranular Length-Scales on Network Magnetic Fields K.P. RajuJagdev Singh OriginalPaper Pages: 11 - 16
Interpretation of Localized Deficits in Coronal Emission Z. ZhangR.N. SmarttD.A. Landman OriginalPaper Pages: 63 - 71
Flux Cancellation Rates and Converging Speeds of Canceling Magnetic Features Jongchul ChaeYong-Jae MoonH.S. Yun OriginalPaper Pages: 73 - 85
The Magnetic Helicity Injected by Shearing Motions P. DémoulinC.H. MandriniG. Aulanier OriginalPaper Pages: 87 - 110
The Temperature and Density Structure of an Hα Flaring Loop M.D. DingY. LiuP.F. Chen OriginalPaper Pages: 125 - 135
An Improved Method to Derive the Lower Energy Cutoff of non-Thermal Electrons From Hard x-Rays of Solar Flares W.Q. GanY.P. LiJames M. Tiernan OriginalPaper Pages: 137 - 147
Hybrid Solar Energetic Particle Events Observed on Board Soho L. KocharovJ. Torsti OriginalPaper Pages: 149 - 157
The Solar Origin of the 6 January 1997 Coronal Mass Ejection Y.Q. WuY.H. TangG.P. Wu OriginalPaper Pages: 159 - 171
Solar Wind Speed and Expansion Rate of the Coronal Magnetic Field in Solar Maximum and Minimum Phases Kazuyuki HakamadaMasayoshi KojimaKen'ichi Fujiki OriginalPaper Pages: 173 - 185
Plasma and Magnetic Field Inside Magnetic Clouds: a Global Study C. CidM.A. HidalgoA.F. Viñas OriginalPaper Pages: 187 - 198