The First Results from SOHO, 1997

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. Kocharov, et al. Viewing Instructions CD-ROM.,

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-Chièze, 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. K

The Solar and Heliospheric Observatory (SOHO) is a joint ESA/NASA mission to study the Sun, from its deep core to the outer corona, and the solar wind. SOHO was launched on 2 December 1995 and was inserted into a halo orbit around the L1 Lagrangian point on 14 February 1996. From this vantage point it is continuously monitoring the Sun, the heliosphere, and the solar wind particles that stream toward the Earth. Nominal operations of the SOHO mission started in April 1996 after commissioning of the spacecraft and the scientific payload. Detailed descriptions of the twelve instruments, which represent the most comprehensive set of solar and heliospheric instruments ever developed and placed on the same platform, can be found in The SOHO Mission (Solar Physics, Vol. 162, Nos. 1--2, 1995). Th