Interplanetary studies: Propagation of disturbances between the Sun and the magnetosphere

Space Science Reviews

Volumn 67, Issue 3-4, 1994, Pages 363-419

  Dryer, Murray ^a  

^a NOAA EARTH SYSTEM RESEARCH LABORATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000267155     PISSN: 00386308     EISSN: 15729672     Source Type: Journal    
DOI: 10.1007/BF00756075     Document Type: Article

References (139)

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2. Modeling of an Interplanetary Disturbance Event Tracked by the Interplanetary Scintillation Method
3. Modeling of a Series of Interplanetary Disturbance Events in September 1978
4. A Simulation Study of Two Major Events in the Heliosphere During the Present Sunspot Cycle
5. Structure and Evolution of Compound Streams at ≤1 AU
6. Magnetic Arcade Evolution and Instability
7. Compound Streams, Magnetic Clouds and Major Geomagnetic Storms
8. Type II Solar Radio Bursts, Interplanetary Shocks and Energetic Particle Events
9. Type II Solar Radio Events Observed in the Interplanetary Medium
10. Two Classes of Solar Energetic Particle Events Associated with Impulsive and Long-Duration Soft X-Ray Flares
11. Energetic Interplanetary Shocks, Radio Emission and Coronal Mass Ejections
12. Comparison of Solar Wind Velocity Measurements with a Theoretical Acceleration Model
13. Frequency Distributions and Correlations of Solar X-Ray Flare Parameters
14. A Three-Dimensional Magnetohydrodynamic Formalism for Coronal Helmet Streamers
15. A time-Dependent 3-D MHD Numerical Study of Interplanetary Plasmoids in the Solar Wind
16. Interplanetary Shock Waves Generated by Solar Flares
17. Coronal Transient Phenomena
18. Radio Data and a Theoretical Model for the Fast-Mode MHD Shock Wave Generated by the Solar Flare of 1973 September 5, 18:26 UT
19. Scientific Highlights of the Study of Traveling Interplanetary Phenomena (STIP) Intervals During the SMY/SMA
20. Comments on “Density Distribution in Looplike Coronal Transients: A Comparison of Observations and a Theoretical Model” by D. G. Sime, R. M. Macqueen, and A. J. Hundhausen
21. Magnetohydrodynamic Models of Coronal Transients in the Meridional Plane. II. Simulation of the Coronal Transient of 1973 August 21
22. Magnetohydrodynamic Modeling of Interplanetary Disturbances between the Sun and Earth
23. The Role of Magnetohydrodynamics in Heliospheric Space Plasma Physics Research
24. The February 1986 Solar Activity: a Comparison of GIOTTO Solar Wind Measurements with MHD Simulations
25. A Simulation Study of Distortion of the Heliospheric Current Sheet Caused by Solar Activity
26. The Three-Dimensional Geometry of the Heliospheric Current Sheet
27. The Solar Flares of February 1986 and the Ensuing Intense Geomagnetic Storm
28. Geomagnetic Activity Associated with Earth Passage of Interplanetary Shock Disturbances and Coronal Mass Ejections
29. Simulation of Three-Dimensional Solar Wind Disturbances and Resulting Geomagnetic Storms
30. A Three-Dimensional, Time-Dependent Modeling of Supersonic and Super-Alfvénic MHD Flow
31. Coronal Transients and Their Relation to Solar Flares
32. Comments on Coronal Mass Ejection onset Studies
33. Coronal Mass Ejecta and Flares: a Statistical Study
34. An Interplanetary Scintillation Index
35. Solar and Interplanetary Shock Effects on the Flux and Anisotropy Profiles of an ESP Event Observed on 23–25 April, 1979
36. On the Large-Scale Effects of Two Interplanetary Shocks on the Associated Particle Events
37. The Influence of the Large-Scale Interplanetary Shock Structure on a Low-Energy Particle Event
38. Origin of Strong Interplanetary Shocks
39. Prediction of Magnetic Orientation in Driver Gas-Associated- Bz Events
40. The Observation of a Coronal Transient Directed at the Earth
41. A Full-Implicit-Continuous-Eulerian (FICE) Scheme for Multidimensional Transient Magnetohydrodynamic (MHD) Flows
42. Configuration, Structure, and Dynamics of Magnetic Clouds from Solar Flares in Light of Measurements on Board Vega 1 and Vega 2 in January–February 1986
43. Disappearing Solar Filaments: a Useful Predictor of Geomagnetic Activity
44. Solar Flares and Coronal Mass Ejections
45. Probing the Magnetic Topologies of Magnetic Clouds by Means of Solar Energetic Particles
46. Associations between Coronal Mass Ejections and Solar Energetic Proton Events
47. Filament Eruptions and the Impulsive Phase of Solar Flares
48. Coronal Mass Ejections and Associated X-Ray Flare Duration
49. Force-Free Magnetic Fields: Is there a ‘Loss of Equilibrium”?
50. Solar Cycle Evolution of Solar Wind Speed Structure between 1973 and 1985 Observed with the Interplanetary Scintillation Method
51. A Three-Dimensional Simulation of a Coronal Streamer
52. Avalanches and the Distribution of Solar Flares
53. The Deceleration of Solar Shock Waves in Space
54. The Kinematics of Solar Inner Coronal Transients
55. Determination of Solar-Wind Velocities Using Single-Station Measurements of Interplanetary Scintillation
56. ISEE 3 Observations of Low-Energy Proton Bidirectional Events and their Relation to Isolated Interplanetary Magnetic Structures
57. An Example of a Piston-Driven Shock in the Solar Corona
58. Dynamical Evolution of a Solar Coronal Magnetic Field Arcade
59. The Evolution of Corotating Stream Fronts Near the Ecliptic Plane in the Inner Solar System. 1. Two-Dimensional Fronts
60. The Evolution of Corotating Stream Fronts Near the Ecliptic Plane. 2. Three-Dimensional Tilted-Dipole Fronts
61. The Structure and Parameter of Flare Streams
62. Evolution of the Solar Wind Structure over a Solar Cycle: Interplanetary Scintillation Velocity Measurements Compared with Coronal Observations
63. 80 MHZ Observations of a Moving Type IV Solar Burst, March 1, 1969
64. Correlated Particle and Magnetic Field Observations of a Large-Scale Magnetic Loop Structure Behind an Interplanetary Shock
65. Relationship of Coronal Transients to Interplanetary Shocks: 3D Aspects
66. Associations between Coronal Mass Ejections and Soft X-ray Events
67. Associations between Coronal Mass Ejections and Metric Type II Bursts
68. Coronal Mass Ejections and Interplanetary Shocks
69. Density Distribution in Looplike Coronal Transients: A Comparison of Observations and a Theoretical Model
70. MHD Study of Temporal and Spatial Evolution of Simulated Interplanetary Shocks in the Ecliptic Plane within 1 AU
71. Numerical Simulations of High-Speed Solar Wind Streams within 1 AU and Their Signatures at 1 AU
72. Interplanetary Shock Collisions: Forward with Reverse Shocks
73. Activity Associated with Coronal Mass Ejections at Solar Minimum: SMM Observations from 1984–1986
74. Solar Maximum Mission Observations of Activity Associated with the Coronal Mass Ejection of October 13, 1988
75. Coronal Evolution Due to Shear Motion
76. Three-Dimensional Structure of Coronal Mass Ejections
77. MHD Intermediate Shock in Coronal Mass Ejections
78. Magnetohydrodynamic Models of Coronal Transients in the Meridional Plane. I. The Effect of the Magnetic Field
79. The Steady Global Corona
80. Calibration of the Kinematic Method of Studying Solar Wind Disturbances on the Basis of a One-Dimensional MHD Solution and a Simulation Study of the Heliosphere between November 22–December 6, 1977
81. Tracking a Major Interplanetary Disturbance
82. Expected IPS Variations Due to a Disturbance Described by a 3-D MHD Model
83. Scintillation, Density and Turbulence in the Interplanetary Medium
84. Great Magnetic Storms
85. Interplanetary Magnetic Field Structure and Solar Wind Parameters as Inferred from Solar Magnetic Field Observations and by Using a Numerical 2-D MHD Model
86. A Global Numerical 3-D MHD Model of the Solar Wind
87. Spherical and Cylindrical Models of Magnetized Plasma Clouds and Their Comparison with Spacecraft Data
88. Full-Implicit-Continuous-Eulerian Scheme in the Spherical Coordinates and Its Applications to Solar Phenomena
89. Structure of Interplanetary magnetic Field Near the Sun
90. Simulation of Period Doubling of Recurrent Solar Wind Structures
91. Comparison of Doppler Scintillation and in situ Space Plasma Measurements of Interplanetary Disturbances
92. Doppler Scintillation Observations of Interplanetary Shocks within 0.3 AU
93. Numerical Tests of a Modified Full Implicit Eulerian (FICE) Scheme with Projected Normal Characteristic Boundary Conditions for MHD Flows
94. Numerical Simulation of Extended Corona
95. Magnetohydrodynamics of Atmospheric Transients. II. Two-Dimensional Numeric Results for a Model Solar Corona
96. Induced Mass and Wave Motions in the Lower Solar Atmosphere. I. Effects of Shear Motion of Flux Tubes
97. Non-Planar MHD Model for Solar Flare-Generated Disturbances in the Heliospheric Equatorial Plane
98. Interplanetary Disturbances in the Solar Wind Produced by Density, Temperature or Velocity Pulses at 0.08 AU
99. Shear-Induced Instability and Arch Filament Eruption: A Magnetohydrodynamic (MHD) Numerical Simulation
100. A Time-Dependent Solution of Trans-Sonic and Trans-Alfvénic MHD Flow in the Solar Meridional Plane