On the relation between the Sun's (geocentric) angular diameter and the observed (topocentric) ‘drift time’ Axel D. WittmannHeinz Neckel OriginalPaper Pages: 1 - 5
Using scintillation measurements to achieve high spatial resolution in photometric solar observations R. CoulterJ. R. KuhnT. Rimmele OriginalPaper Pages: 7 - 19
Meridional motions of magnetic features in the solar photosphere Herschel B. SnodgrassSara B. Dailey OriginalPaper Pages: 21 - 42
Potential field extrapolation using three components of a solar vector magnetogram with a finite field of view G. Allen Gary OriginalPaper Pages: 43 - 64
Calculated profiles of H I lines of interest for solar plasma electric field measurements Roberto CasiniPeter Foukal OriginalPaper Pages: 65 - 77
Ca II K line profile of the truly quiet Sun K. R. SivaramanS. S. GuptaR. Kariyappa OriginalPaper Pages: 93 - 97
Joint radio and soft x-ray imaging of an ‘anemone’ active region A. VourlidasT. S. BastianM. J. Aschwanden OriginalPaper Pages: 99 - 120
Hβ Doppler-velocity fields within sites of flares in a solar active region Wei LiGuoxiang AiHongqi Zhang OriginalPaper Pages: 121 - 131
The 4 February, 1986 flare and flare-filament current model Tang Yu-HuaYin Chun-LinQiu Jiong OriginalPaper Pages: 133 - 144
X-ray bright point flares due to magnetic reconnection L. Van Driel-GesztelyiB. SchmiederJ. Staiger OriginalPaper Pages: 145 - 170
1–4 GHz type II-like radio bursts and pinch processes near the transition region Marian KarlickýKarel Jiřička OriginalPaper Pages: 171 - 181
Confirmation of the 25.5-day fundamental period of the Sun using the north-south asymmetry of the flare index Atila ÖzgüçTamer Ataç OriginalPaper Pages: 183 - 191
A nonlinear RLC solar cycle model J. M. PolygiannakisX. MoussasC. P. Sonett OriginalPaper Pages: 193 - 203