MHD structures, waves and turbulence in the solar wind: Observations and theories

Space Science Reviews

Volumn 73, Issue 1-2, 1995, Pages 1-210

  Tu, C Y ^a,b   Marsch, E ^a  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b PEKING UNIVERSITY   (China)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0011247057     PISSN: 00386308     EISSN: 15729672     Source Type: Journal    
DOI: 10.1007/BF00748891     Document Type: Article

References (408)

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12. On the polarization state of hydromagnetic fluctuations in the solar wind
13. Radial evolution of power spectra of interplanetary Alfvénic turbulence
14. Properties of whistler mode waves between 0.3 and 1.0 AU from Helios observations
15. ALFVÉNIC Wave Pressures and the Solar Wind
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17. Large-amplitude Alfvén waves in the interplanetary medium, 2
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19. Evidence for long period Alfvén waves in the inner solar system
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34. Pressure-Balanced structures between 1 AU and 24 AU and their implications for solar wind electrons and interstellar pickup ions
35. Nonlinear Alfven waves in inhomogeneous plasmas
36. On the backscatter instability of solar wind Alfvén waves
37. Mode decay and evolution of the solar wind Alfvén wave spectrum
38. Turbulence, Viscosity, and Dissipation in the Solar-Wind Plasma
39. The radial dependence of the interplanetary magnetic field: 1.0-1.5 AU
40. Propagation observations of the solar wind near the sun
41. The solar wind density spectrum near the Sun: Results from Voyager radio measurements
42. Comparison of solar wind velocity measurements with a theoretical acceleration model
43. Growth of correlation in compressible two-dimensional magnetofluid turbulence
44. Alfvén wave refraction by interplanetary inhomogeneities
45. Multispacecraft observations of microscale fluctuations in the solar wind
46. Statistical properties of low-frequency magnetic field fluctuations in the solar wind from 0.29 to 1.0 AU during solar minimum conditions: HELIOS 1 and HELIOS 2
47. Modulational instability of finite-amplitude, circularly polarized Alfven waves
48. Compressional instability in the solar wind driven by wave dissipation
49. The Hydromagnetic Equations
50. Broadening of the resonantly scattered H I Lyman alpha line caused by Alfvén waves
51. Drawing inferences about solar wind acceleration from coronal minor ion observations
52. A two-fluid solar wind model with Alfven waves: Parameter study and application to observations
53. Estimates of solar wind heating inside 0.3 AU
54. The cold solar wind
55. An instability of finite amplitude circularly polarized Alfven waves
56. Systematic errors in determining the propagation direction of interplanetary Alfvenic fluctuations
57. The structure of helical interplanetary magnetic fields
58. large-amplitude waves in an anisotropic plasma
59. Onset and decay of two-dimensional magnetohydrodynamic turbulence with velocity–magnetic field correlation
60. Non-WKB Alfvén waves in the solar wind
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62. The helium component of solar wind velocity streams
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79. Alfven waves in stellar winds
80. A drift-kinetic treatment of the parametric decay of large-amplitude Alfvén waves
81. Nonlinear magnetogravity waves in a low-β plasma
82. Direct observations of higher frequency density fluctuations in the interplanetary plasma
83. Preliminary Power Spectra of the Interplanetary Plasma
84. Investigations of a turbulence-driven solar wind model
85. Finite amplitude Alfvén waves in a multi-ion plasma: Propagation, acceleration, and heating
86. On the preferential acceleration and heating of solar wind heavy ions
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88. Solar wind models with Alfven waves
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90. The polar heliospheric magnetic field
91. Anisotropy and minimum variance directions of solar wind fluctuations in the outer heliosphere
92. Energy addition in the solar wind
93. Magnetic field directional discontinuities: 1. Minimum variance errors
94. Dynamic magnetic structure of large amplitude Alfvénic variations in the solar wind
95. On Sound Generated Aerodynamically. I. General Theory
96. Solar wind proton temperature-velocity relationship
97. Steady hydromagnetic flows in open magnetic fields. I - A class of analytic solutions
98. A study of MHD fluctuations upstream and downstream of quasi-parallel interplanetary shocks
99. Oblique propagation of nonlinear hydromagnetic waves: One- and two-dimensional behavior
100. Variations of the occurrence rate of discontinuities in the interplanetary magnetic field
101. Turbulence in the Solar Wind
102. Ideal MHD equations in terms of compressive Elsässer variables
103. Spectral and spatial evolution of compressible turbulence in the inner solar wind
104. Spectral and spatial evolution of compressible turbulence in the inner solar wind
105. Modeling Results on Spatial Transport and Spectral Transfer of Solar Wind Alfvénic Turbulence
106. Pronounced proton core temperature anisotropy, ion differential speed, and simultaneous Alfvén wave activity in slow solar wind at 0.3 AU
107. Solar wind helium ions: Observations of the Helios solar probes between 0.3 and 1 AU
108. Solar wind protons: Three-dimensional velocity distributions and derived plasma parameters measured between 0.3 and 1 AU
109. Wave heating and acceleration of solar wind ions by cyclotron resonance
110. Measurement of the rugged invariants of magnetohydrodynamic turbulence in the solar wind
111. Stationarity of magnetohydrodynamic fluctuations in the solar wind
112. Nearly incompressible magnetohydrodynamics at low Mach number
113. Turbulent magnetic reconnection
114. An interplanetary magnetic field ensemble at 1 AU
115. Evidence for the presence of quasi-two-dimensional nearly incompressible fluctuations in the solar wind
116. Nearly incompressible magnetohydrodynamics, pseudosound, and solar wind fluctuations
117. The Collimation of Cosmic Rays by the Interplanetary Magnetic Field
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119. Modifications of magnetohydrodynamics as applied to the solar wind
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121. Planar magnetic structures in the solar wind
122. Preliminary results from the Pioneer 6 Magnetic Field Experiment
123. Tangential discontinuities in the solar wind: Correlated field and velocity changes and the Kelvin-Helmholtz instability
124. Plasma fluctuations in the solar wind
125. Observations of the velocity distribution of solar wind ions
126. Helium, hydrogen, and oxygen velocities observed on ISEE 3
127. Anomalous scaling laws in multifractal objects
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129. Microstructure of the interplanetary magnetic field near 4 and 5 AU
130. Propagation directions of hydromagnetic waves in interplanetary space: Pioneer 10 and 11
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132. Helium in the solar wind
133. Interplanetary observational constraints on Alfvén wave acceleration of the solar wind
134. Heliocentric distance and temporal dependence of the interplanetary density-magnetic field magnitude correlation
135. Spectral signatures of jumps and turbulence in interplanetary speed and magnetic field data
136. Origin and evolution of fluctuations in the solar wind: Helios observations and Helios-Voyager comparisons
137. The amplitudes of interplanetary fluctuations: Stream structure, heliocentric distance, and frequency dependence
138. Velocity shear generation of solar wind turbulence
139. The nature and evolution of magnetohydrodynamic fluctuations in the solar wind: Voyager observations
140. The radial dependences of the interplanetary magnetic field between 1 and 5 AU: Pioneer 10
141. The spectrum of the interplanetary magnetic field near 1.3 AU
142. Interplanetary magnetic field power spectra: Mean field radial or perpendicular to radial
143. On temperature and speed of He++and O6+ions in the solar wind
144. The source of proton anisotropy in the high-speed solar wind
145. Power spectra and discontinuities of the interplanetary magnetic field: Mariner 4
146. On the minimum variance direction of magnetic field fluctuations in the azimuthal velocity structure of the solar wind
147. Plasma field characteristics of directional discontinuities in the interplanetary medium
148. Magnetopause structure and attitude from Explorer 12 observations
149. Decay instability of finite-amplitude circularly polarized Alfven waves: A numerical simulation of stimulated Brillouin scattering
150. The damping of interplanetary Alfvénic fluctuations and the heating of the solar wind
151. The Interplanetary MHD Fluctuations and Its Relation with the Heating and Acceleration of the Solar Wind
152. Evidence for a “background” spectrum of solar wind turbulence in the inner heliosphere
153. A model of solar wind fluctuations with two components: Alfvén waves and convective structures
154. Basic properties of solar wind MHD turbulence near 0.3 AU analyzed by means of Elsässer variables
155. The dependence of MHD turbulence spectra on the inner solar wind stream structure near solar minimum
156. Spectral evolution and cascade constant of solar wind Alfvénic turbulence
157. Decay instability of incoherent Alfvén waves in solar wind
158. An analysis of solar wind fluctuations between 1 and 10 AU
159. Waves from the sun?
160. The radial evolution of the amplitudes of “dissipationless” turbulent solar wind fluctuations
161. On the role of Alfvénic fluctuations in the inner solar system
162. Why fast solar wind originates from slowly expanding coronal flux tubes
163. The Angular Momentum of the Solar Wind
164. Nonlinear alfvénic fluctuations in uniform magnetic background fields
165. Alfvén waves in spiral interplanetary field
166. A magnetohydrodynamic model for corotating interplanetary structures
167. Evolution and interaction of interplanetary shocks
168. Expansion of the solar wind in high-speed streams
169. Thermodynamic properties of the heliospheric plasma
170. The temperature structure, mass, and energy flow in the corona and inner solar wind
171. Mass and Energy Flow in the Solar Chromosphere and Corona
172. Spacecraft radio scattering observations of the power spectrum of electron density fluctuations in the solar wind
173. Parametric instabilities of circularly polarized Alfvén waves including dispersion
174. Low-frequency fluctuations in the solar wind. I - Theory
175. Waves and turbulence in the solar wind
176. Temperature and density anti-correlations in solar wind fluctuations
177. Non-WKB evolution of solar wind fluctuations: A turbulence modeling approach
178. Transport and turbulence modeling of solar wind fluctuations
179. Remarks on transport theories of interplanetary fluctuations
180. Models of inertial range spectra of interplanetary magnetohydrodynamic turbulence