The SOHO-7 Proceedings have been published in Space Science Reviews, volume 87, no. 1-2. The stand-alone hardcover volume has also been published in 1999 by Kluwer Academic Publishers (ISBN 0-7923-5828-7).
| PAGES | AUTHOR(S), TITLE |
| -- - -- | Foreword |
| 001 - 024 | E. Marsch, Solar wind models from the Sun to 1 AU: Constraints by in situ and remote sensing measurements |
| 025 - 041 | W. Ian Axford, et al., Acceleration of the high speed solar wind in coronal holes |
| 043 - 054 | L. A. Fisk, et al., Coronal Hole Boundaries and their Interactions with Adjacent Regions |
| 055 - 066 | J. C. Raymond, Composition variations in the solar corona and solar wind |
| 067 - 077 | E. Leer and E. Marsch, Working Group 1 Report: Solar wind models from the Sun to 1 AU: Constraints by ``in situ'' and remote sensing measurements |
| 079 - 092 | A. W. Hood, Working Group 2 Report: Energy Input, Heating, and Solar Wind Acceleration in Coronal Holes |
| 093 - 104 | R. Esser, Working Group 3 Report: Coronal hole boundaries and interactions with adjacent regions |
| 105 - 121 | H. E. Mason and P. Bochsler, Working Group 4 Report: Composition and Elemental Abundance Variations in the Solar Atmosphere and Solar Wind |
| 123 - 128 | A. H. Gabriel, SOHO after 30 months: a personal view |
| 129 - 132 | J.-L. Bertaux, et al., SWAN observations of the Solar Wind Latitude Distribution and its Evolution Since Launch |
| 133 - 136 | R. Betta, et al., On the stability of siphon flows confined in coronal loops |
| 137 - 140 | L. F. Burlaga and A. Szabo, Fast and slow flows in the solar wind near the ecliptic at 1 AU? |
| 141 - 144 | F. Chiuderi-Drago, et al., EUV and Radio Observations of an equatorial coronal hole |
| 145 - 148 | J. R. Clegg, et al., The solar magnetic field as a coronal hole extension forms: effects of magnetic helicity and boundary conditions |
| 149 - 152 | S. R. Cranmer, et al., Spectroscopic Constraints on Models of Ion-Cyclotron Resonance Heating in the Polar Solar Corona |
| 153 - 156 | I. Cuseri, et al., Coronal heating: a comparison of ion-cyclotron and gravity damping models |
| 157 - 160 | R. B. Dahlburg and G. Einaudi, Compressible aspects of slow solar wind formation |
| 161 - 164 | I. E. Dammasch, et al., Statistical Analysis of EUV and UV Lines Inside and Outside of Solar Coronal Holes |
| 165 - 168 | J. M. Davila and L. Ofman, Two-fluid 2.5D MHD Simulations of the Fast Solar Wind in Coronal Holes and the Relation to UVCS Observations |
| 169 - 172 | G. Del Zanna and B. J. I. Bromage, Characterization of solar coronal holes and plumes using spectroscopic diagnostic techniques applied to SOHO/CDS observations |
| 173 - 176 | D. Dobrzycka, et al., Comparison of Polar and Equatorial Coronal Holes observed by UVCS/SOHO: Geometry and Physical Properties |
| 177 - 180 | D. Dobrzycka, et al., Variation of Polar Coronal Hole Profiles with Solar Cycle |
| 181 - 184 | D. A. Falconer, et al., Large-Scale Coronal Heating, Clustering of Coronal Bright Points, and Concentration of Magnetic Flux |
| 185 - 188 | A. Fludra, et al., EUV Observations Above Polar Coronal Holes |
| 189 - 192 | R. A. Frazin, et al., UVCS/SOHO Ion Kinetics in Coronal Streamers |
| 193 - 198 | C. P. T. Groth, et al., A Parallel Adaptive 3D MHD Scheme for Modeling Coronal and Solar Wind Plasma Flows |
| 199 - 206 | M. Guhathakurta, et al., Semi-empirical MHD Model of the Solar Wind and Its Comparison with Ulysses |
| 207 - 210 | P. Hackenberg, et al., Plasma properties in coronal funnels |
| 211 - 214 | B. Inhester, et al., The rotation of the Fe XIV solar corona during the recent solar activity minimum |
| 215 - 218 | J. E. Insley, A CDS observation of the relationship between a coronal hole and chromospheric structure |
| 219 - 222 | M. Karovska, et al., Study of Dynamical Properties of Coronal Structures in the Polar Regions |
| 223 - 226 | R. Keppens and J. P. Goedbloed, Numerical simulations of stellar winds |
| 227 - 231 | Y.-K. Ko and C. P. T. Groth, On the Electron Temperature and Coronal Heating in the Fast Solar Wind Constrained by In-Situ Observations |
| 233 - 236 | J. L. Kohl, et al., UVCS/SOHO Observations of Spectral Line Profiles in Polar Coronal Holes |
| 237 - 239 | M. Kojima, et al., The highest solar wind velocity in a polar region estimated from IPS tomography analysis |
| 241 - 244 | E. Landi, et al., Observation of transition region fine structures with SOHO/SUMER |
| 245 - 248 | M. Landini, et al., Loop models from SOHO observations |
| 249 - 252 | P. Lemaire, et al., Search for signatures of a coronal hole in transition region lines near disk center |
| 253 - 256 | X. Li, A 16-Moment Fast Solar Wind Model |
| 257 - 260 | P. Liewer, et al., Hybrid Simulations of Wave Propagation and Ion Cyclotron Heating in the Expanding Solar Wind |
| 261 - 264 | Y.-Q. Lou, Magneto-Gravity Waves Trapped in the Lower Solar Corona |
| 265 - 268 | L. Maccari, et al., Ly-alpha observation of a coronal streamer with UVCS/SOHO |
| 269 - 275 | W. H. Matthaeus, et al., Fluctuations, dissipation and heating in the corona |
| 277 - 281 | M. P. Miralles, et al., Properties of Coronal Hole/Streamer boundaries and adjacent regions as observed by Spartan 201 |
| 283 - 286 | R. L. Moore, et al., Coronal Heating by Magnetic Explosions |
| 287 - 290 | L. Ofman, et al., SOHO Observations of Density Fluctuations in Coronal Holes |
| 291 - 294 | S. Patsourakos, et al., Outflow velocities at the base of a polar coronal hole during the 1998 total eclipse |
| 295 - 298 | S. Poedts, et al., Velocity Shear Induced Phenomena in Solar Atmosphere |
| 299 - 302 | U. Schuehle, et al., Signatures of coronal hole spectra between 660 Angstroms and 1460 Angstroms measured with SUMER on SOHO |
| 303 - 306 | N. Srivastava, et al., Acceleration Profile Of the Slow Solar Wind as inferred from gradual mass ejections observed by LASCO |
| 307 - 310 | G. Stenborg, et al., MICA: The Mirror Coronagraph For Argentina |
| 311 - 314 | L. Strachan, et al., Constraints on Coronal Outflow Velocities derived from UVCS Doppler Dimming Measurements and In-Situ Charge State Data |
| 315 - 318 | K. Stucki, et al., Coronal hole properties observed with SUMER |
| 319 - 322 | S. T. Suess, et al., Ulysses-UVCS Coordinated Observations |
| 323 - 326 | S. T. Suess, et al., Streamer Evaporation |
| 327 - 330 | R. M. Suleiman, et al., UVCS/SOHO Observations of H I Lyman Alpha Line Profiles in Coronal Holes at Heliocentric Heights above 3.0 solar radii |
| 331 - 334 | C.-Y. Tu, et al., Ion temperatures as observed in a solar coronal hole |
| 335 - 338 | A. M. Vasquez, et al., UVCS observations and modeling of streamers |
| 339 - 343 | M. Velli and P. Liewer, Alfven Wave Generation in Photospheric Vortex Filaments, Macrospicules, and ``Solar Tornadoes'' |
| 345 - 348 | P. R. Young and R. Esser, Comparing quiet Sun and coronal hole regions with CDS/SOHO |
| 349 - 352 | L. Zangrilli, et al., On the Lyman alpha and O VI line profiles in streamers and coronal holes |
| 353 - 356 | T. H. Zurbuchen, et al., The transition between fast and slow solar wind from composition data |
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