作者: M. A. Shea , D. F. Smart , Leendert Dirk de Feiter , Shi Tsan Wu
DOI:
关键词: Corona 、 Astronomy 、 Astrophysics 、 Interplanetary medium 、 Interplanetary magnetic field 、 Coronal mass ejection 、 Solar wind 、 Magnetopause 、 Heliospheric current sheet 、 Interplanetary scintillation 、 Physics
摘要: I. Solar Physics as it Concerns the Study of Travelling Interplanetary Phenomena (STIP).- Mass Ejections from Corona into Space.- Energetic Flare Particles and Shock Waves.- Dynamic Modeling Coronal Responses to Events.- II. Radio Astronomy Scintillations.- Stereo Radioastronomy.- Measurements Wind Using Spacecraft Scattering Observations.- Observations Scintillation: Velocity Measurements.- Scintillation Plasma.- III. Theory The Three-Dimensional Structure Medium.- Theoretical Contributions Research - A Review.- Large Scale Long Term Evolution Speed Distribution High Streams.- Pioneer 10, 11 Evolving Streams Shocks Beyond 1 AU.- Wave-Particle Interaction Associated with in Wind.- IV. Cometary Topics.- Comets STIP Context.- Comet-Solar Interaction.- Type-1 Comet Tails.- V. Cosmic Ray Propagation, Modulation, Acceleration.- Signatures Events Their Relation Propagation Acceleration Processes.- Below 10 MeV.- Modulation Electrons Ions by Propagating Shocks.- VI. Stip Interval I II.- Summary Significant Solar-Initiated During Intervals Overview HELIOS 2 Missions Participation Index Authors Cited.