Do Photospheric Brightness Structures Outside Magnetic Flux Tubes Contribute to Solar Luminosity Variation? Peter FoukalPietro N. Bernasconi OriginalPaper 22 February 2008 Pages: 1 - 15
Current Helicity and Twist as Two Indicators of the Mirror Asymmetry of Solar Magnetic Fields D. SokoloffH. ZhangV. N. Tutubalin OriginalPaper 03 February 2008 Pages: 17 - 28
Topological Departures from Translational Invariance along a Filament Observed by THEMIS J. DudíkG. AulanierT. Roudier OriginalPaper 19 March 2008 Pages: 29 - 50
Where Do Solar Filaments Form?: Consequences for Theoretical Models Duncan H. MackayVictor GaizauskasAnthony R. Yeates OriginalPaper 03 February 2008 Pages: 51 - 65
Relationship between Powerful Flares and Dynamic Evolution of the Magnetic Field at the Solar Surface Jihong LiuYin ZhangHongqi Zhang OriginalPaper 06 March 2008 Pages: 67 - 84
Statistical Models for the Solar Flare Interval Distribution in Individual Active Regions Yūki Kubo OriginalPaper 22 February 2008 Pages: 85 - 98
RHESSI Observations of the Neupert Effect in Three Solar Flares Zongjun Ning OriginalPaper 03 February 2008 Pages: 99 - 111
Space Weather Application Using Projected Velocity Asymmetry of Halo CMEs G. MichalekN. GopalswamyS. Yashiro OriginalPaper 03 February 2008 Pages: 113 - 123
Average Thickness of Magnetosheath Upstream of Magnetic Clouds at 1 AU versus Solar Longitude of Source R. P. LeppingC.-C. WuD. B. Berdichevsky OriginalPaper Open access 01 March 2008 Pages: 125 - 139
The Behavior of Sunspot Contrast during Cycle 23 M. J. WesolowskiS. R. WaltonG. A. Chapman OriginalPaper 06 February 2008 Pages: 141 - 154
Short-Period Fluctuations in Coronal Mass Ejection Activity during Solar Cycle 23 Alejandro LaraAndrea BorgazziMargarete Oliveira Domingues OriginalPaper 20 March 2008 Pages: 155 - 166
Coronal Mass Ejections, Magnetic Fields, and the Green Corona in Cycle 23 M. MinarovjechV. RušinM. Saniga OriginalPaper 03 March 2008 Pages: 167 - 176
Similarities and Dissimilarities between the Variations of CME and Other Solar Parameters at Different Heliographic Latitudes and Time Scales R. P. Kane OriginalPaper 07 March 2008 Pages: 177 - 190
On Prediction of the Strength of the 11-Year Solar Cycle No. 24 V. N. ObridkoB. D. Shelting OriginalPaper 03 March 2008 Pages: 191 - 202
Prediction of Solar Cycle Maximum Using Solar Cycle Lengths R. P. Kane OriginalPaper 03 February 2008 Pages: 203 - 209