1. Performance and Early Results from the GOLF Instrument Flown on the SOHO Mission; A.
Gabriel, et al. 2. First Results on P-Modes from GOLF Experiment; M. Lazrek, et al. 3. First View of the Solar Core from GOLF Acoustic Modes; S.
Turck-Chieze, et al. 4. In-Flight Performance of the VIRGO Solar Irradiance Instruments on SOHO; C. Froehlich, et al. 5. Measurements of Frequencies of Solar Oscillations from the MDI Medium-1 Program; E.J.
Rhodes, et al. 6. Tri-Phonic Helioseismology: Comparison of Solar P-Modes Observed by the Helioseismology Instruments aboard SOHO; T. Toutain, et al. 7. Modeling the Distribution of Magnetic Fluxes in Field Concentrations in a Solar Active Region; C.J. Schrijver, et al. 8. Bursts of Explosive Events in the Solar Network; D.E.
Innes, et al. 9. Doppler Shifts in the Quiet Sun Transition Region and Corona Observed with SUMER on SOHO; P. Brekke, et al. 10. Observations of Polar plumes with the SUMER Instrument on SOHO; D.K.
Hassler, et al. 11. A Coordinated Observation of Polar Plumes; C. DeForest, et al. 12. Eruptive Prominence and Associated CME Observed with SUMER, CDS, and LASCO; J.E.
Wiik. 13. First Observations of Coronal Hole Structure and Evolution Using SOHO-CDS; J.E.
Insley, et al. 14. EUV Observations of a Macrospicule: Evidence for Solar Wind Acceleration?
C.D. Pike, R.A. Harrison. 15. EUV Blinkers: The Significance of Fast Variations in the Extreme Ultraviolet Quiet Sun; R.A.
Harrison. 16. Active Regions Observed in EUV Light by the CDS on SOHO; A.
Fludra, et al. 17.High-Velocity Flows in an Active Region Loop System Observed with the CDS on SOHO; P.
Brekke, et al. 18. The Mg/Ne Relative Abundance in a Recently Emerged Flux Region Observed by CDS; P.R.
Young, H.E. Mason. 19. The Relationship Between UV and X-Ray Brightenings; S.A.
Matthews, L.K. Harra-Murnion. 20. SOHO CDS-NIS In-Flight Intensity Calibration with a Plasma Diagnostic Method; E.
Landi, et al. 21. EIT Observations of the Extreme Ultraviolet Sun; D.
Moses, et al. 22. EIT and LASCO Observations of the Initiation of a Coronal Mass Ejection; K.P.
Dere, et al. 23. First Results from the SOHO Ultraviolet Coronagraph Spectrometer; J.L.
Kohl, et al. 24. Composition of Coronal Streamers from the Solar Ultraviolet Coronagraph Spectrometer; J.C.
Raymond, et al. 25. First View of the Extended Green-Line Emission Corona at Solar Activity Minimum Using the LASCO-C1 Coronagraph on SOHO; R.
Schwenn, et al. 26. LASCO Observations of Disconnected Magnetic Structures Out to Beyond 28 Solar Radii During Coronal Mass Ejections; G.M.
Simnett, et al. 27. The Relationship of Green-Line Transients to White-Light Coronal Mass Ejections; S.P.
Plunkett, et al. 28. MHD Interpretation of LASCO Observations of a Coronal Mass Ejection as a Disconnected Magnetic Structure; S.T.
Wu, et al. 29. First Results from Swan/SOHO Lyman Alpha Sky/Solar Wing Mapper; J.L.
Bertaux, et al. 30. Recurrence of Energetic Particle Flux Anisotropy as Observed by ERNE on July 9, 1996; J.
Torsti, et al. 31. Implications of Proton Anisotropy Development Observed by ERNE Instrument During the 9 July 1996 Solar Particle Event; L.G.
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