Effect of Large-Scale Magnetic Fields on Total Solar Irradiance A.V. MordvinovR.C. Willson OriginalPaper Pages: 5 - 16
A Consistent one-Dimensional Model for the Turbulent Tachocline K. Petrovay OriginalPaper Pages: 17 - 30
On the Connection Between Mean Field Dynamo Theory and Flux Tubes Arnab Rai Choudhuri OriginalPaper Pages: 31 - 55
Obliquely Propagating Shear Alfvén Waves Excited by Newborn Ions in the Chromosphere – Corona Transition Region Y.P. ChenG.C. Zhou OriginalPaper Pages: 57 - 68
Determination of coronal loop properties from trace observations I. De MoortelC.E. ParnellA.W. Hood OriginalPaper Pages: 69 - 86
Imaging Spectropolarimetry of Ti I 2231 nm in a Sunspot M.J. PennW.D. CaoW. Livingston OriginalPaper Pages: 87 - 97
On the Latitudinal Distribution of Sunspot Groups over a Solar Cycle K.J. LiJ.X. WangX.M. Gu OriginalPaper Pages: 99 - 109
Does solar flare activity lag behind sunspot activity? M. TemmerA. VeronigA. Hanslmeier OriginalPaper Pages: 111 - 126
Precise determination of cooling times of post-flare loops from the detailed comparison between Hα and soft X-ray images Suguru KamioHiroki KurokawaTakako T. Ishii OriginalPaper Pages: 127 - 146
Double Plasma Resonance for Decimetric dot-Emissions V. KrishanF.C.R. FernandesH.S. Sawant OriginalPaper Pages: 147 - 159
An Investigation of Solar Maximum Metric Type ii Radio Bursts: do two Kinds of Coronal Shock Sources Exist? A. ShanmugarajuY.-J. MoonS. Umapathy OriginalPaper Pages: 161 - 184
On the kinematic evolution of flare-associated cmes A. ShanmugarajuY.-J. MoonS. Umapathy OriginalPaper Pages: 185 - 201