Section I: The Corona.- Coronal Magnetic Fields — a Mini Survey.- Origins of the Solar Wind in the Corona.- The Heliospheric Energy Source.- Coronal Spectroscopy and Imaging from Spartan during the Polar Passage of Ulysses.- The Structure and Rotation of the Solar Corona: Implications for the Heliosphere.- OVI Diagnostics of Solar Wind Generation.- Solar Wind Observations Near the Sun.- Three-Dimensional Reconnection after a Prominence Eruption.- Section II: Solar Hard X-Rays.- Stereoscopic Measurements of Hard Solar X-Rays and Related Topics.- Temporal Evolution of an Energetic Electron Population in an Inhomogeneous Medium. Application to X-Ray Bursts.- Influence of Solar Flares on the X-Ray Corona.- Section III: Coronal Transients and Mass Ejections.- Coronal Transients at High Heliographic Latitudes.- The Solar Cycle Dependence of Coronal Mass Ejections.- Helios Images of Coronal Mass Ejections.- Relationship of Coronal Transients to Interplanetary Shocks: 3-D Aspects.- 3-Dimensional Configurations of Interplanetary Disturbances Associated with Coronal Mass Ejections.- The 3-Dimensional Extent at 1 AU of Interplanetary Disturbances Associated with Disappearing Solar Filaments.- 3-Dimensional, Time-Dependent, MHD Model of a Solar Flare-Generated Interplanetary Shock Wave.- Section IV: Solar Wind.- Interplanetary Scintillation Observations of the Solar Wind at High Latitudes.- Exploration of Heliosphere by Interplanetary Scintillation.- Evolution of Turbulence and Waves in the Solar Wind in Radius and Latitude.- A Computer Simulation Study of the Microscopic Structure of a Typical Current Sheet in the Solar Wind.- Solar Wind Composition and What We Expect to Learn from Out-of-Ecliptic Measurements.- Comets and Three-Dimensional Solar Wind Structure.- Structure and Dynamics of Corotating and Transient Streams in Three Dimensions.- Propagation of Solar Wind Features: A Model Comparison Using Voyager Data.- Section V: Heliospheric Structure.- 3-D Coronal and Heliospheric Structure from Radio Observations.- Latitude Distribution of Interplanetary Magnetic Field Lines Rooted in Active Regions.- Heliospheric Structure and Multispacecraft Observations of Type III Radio Bursts.- The Relationship of the Large-Scale Solar Field to the Interplanetary Magnetic Field: What Will Ulysses Find ?.- The Large-Scale Structure of the Heliospheric Magnetic Field.- The Heliospheric Current Sheet: 3-Dimensional Structure and Solar Cycle Changes.- Solar Wind Speed Azimuthal Variation Along the Heliospheric Current Sheet.- 3-Dimensional Structure of the Heliosphere as Inferred from Observations with a Japanese Halley Spacecraft.- 3-Dimensional Structure of the Heliospheric Current Sheet.- Section VI: Energetic Particles.- Separation and Analysis of Temporal and Spatial Variations in the 10 April 1969 Solar Flare Particle Event.- Acceleration of Energetic Particles at Solar Wind Shocks.- Shock Acceleration of Nucleons at ?16° Solar Latitude Associated with Interplanetary Corotating Interaction Regions.- Latitude Dependence of Co-Rotating Shock Acceleration in the Outer Heliosphere.- Three-Dimensional Gradients of Solar Particles Inside 5 AU.- A Spatially Confined, Long-Lived Stream of Solar Particles.- Super-Events in the Inner Solar System and Their Relation to the Solar Cycle.- The Maximum Entropy Principle in Cosmic Ray Transport Theory.- Section VII: Cosmic Rays.- Modulation of Galactic Cosmic Rays in the Heliosphere.- Effects of 3-Dimensional Heliospheric Structures on Cosmic-Ray Modulation.- Measurement of Radial and Latitudinal Gradients of Cosmic Ray Intensity During the Decreasing Phase of Sunspot Cycle 21.- North/South Asymmetry in Solar Activity and its Effects on the High Energy Cosmic Ray Diurnal Variation.- The Anomalous Component, Its Variation With Latitude and Related Aspects of Modulation.- Pick-Up Ions in the Solar Wind as a Source of Suprathermal Particles.- Section VIII: Interstellar Gas and Interplanetary Dust.- Neutral Interstellar Gases in the Heliosphere: New Aspects of the Problem.- Interstellar Gas Parameters and Solar Wind Anisotropies Deduced from H and HE Observations in the Solar System.- The 3-Dimensional Structure of the Interplanetary Dust Cloud.- The Interaction of Solid Particles with the Interplanetary Medium.- Section IX: Ulysses.- The Ulysses Mission.- Section X: Summary.- Summary Remarks.- List of Participants.
