| Preface: Physics of the Heliosphere: A 10 Year Retrospective |
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1 | (4) |
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TURBULENCE AND PLASMA PROCESSES |
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Solitons in two-fluid plasma |
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5 | (7) |
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Parametric decay of large-amplitude Alfvean waves: MHD and hybrid simulations |
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12 | (6) |
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Residual energy in MHD turbulence and in the solar wind |
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18 | (6) |
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Current sheets in the heliosheath: Voyager 1, 2009 |
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24 | (6) |
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Injection and acceleration of charged nano-dust particles from sungrazing comets |
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30 | (6) |
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Toward a self-consistent kinetic model of pickup ion isotropization |
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36 | (6) |
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Velocities of density structures in the solar wind |
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42 | (6) |
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Numerical modeling of the solar wind turbulence |
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48 | (7) |
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Electrostatic structures in space plasmas: Stability of two-dimensional magnetic bernstein-greene-kruskal modes |
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55 | (6) |
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Effects of suprathermal particles in space plasmas |
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61 | (6) |
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Stability of the strahl and solar burst electron distribution function and its dynamics |
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67 | (7) |
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74 | (6) |
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Solar wind electrons and Langmuir turbulence |
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80 | (9) |
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PARTICLE ACCELERATION AND TRANSPORT |
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Ion pickup and acceleration: Measurements from planetary missions |
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89 | (14) |
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Observations of the longitudinal spread of solar energetic particle events in solar cycle 24 |
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103 | (7) |
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Ion acceleration near CME-driven interplanetary shocks |
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110 | (6) |
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Energetic particle acceleration in the heliosphere |
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116 | (8) |
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The heliospheric current sheet and cosmic-ray transport in the heliosheath |
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124 | (6) |
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Suprathermal ions associated with strong interplanetary shocks |
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130 | (6) |
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Analysis of suprathermal tails using hourly-averaged proton velocity distributions at 1 AU |
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136 | (8) |
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Acceleration of energetic charged particles: Shocks, reconnection or turbulence? |
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144 | (13) |
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Anomalous cosmic rays in the heliosheath |
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157 | (6) |
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Magnetic reconnection as the cause of cosmic ray excess from the heliospheric tail |
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163 | (8) |
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The pre-heating and injection of bulk solar wind and suprathermal protons into first order Fermi acceleration at a fast traveling shock |
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171 | (7) |
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Diffusive shock acceleration in large SEP events |
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178 | (12) |
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Angular distribution of energetic particles scattered by strongly anisotropic MHD turbulence: Understanding Milagro/IceCube results |
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190 | (9) |
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Particle acceleration above the pick-up energy at comet 1P/Halley |
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199 | (7) |
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Evolution of suprathermal seed particle and solar energetic particle abundances |
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206 | (6) |
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Solar energetic particles: Shock acceleration and transport through self-amplified waves |
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212 | (9) |
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INTERSTELLAR AND ENERGETIC NEUTRAL ATOMS |
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Modeling energetic neutral atoms and the IBEX spectrum |
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221 | (6) |
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Potential sources for energetic neutrals from the heliosphere and beyond |
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227 | (6) |
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Primary neutral helium in the heliosphere |
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233 | (6) |
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Cassini ENA images of the heliosheath and Voyager "ground truth": Thickness of the heliosheath |
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239 | (8) |
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CORONAL MASS EJECTIONS AND SHOCKS |
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Factors affecting the intensity of solar energetic particle events |
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247 | (6) |
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Relationship between solar energetic oxygen flux and MHD shock mach number |
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253 | (6) |
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Magnetic field connection and large scale coronal disturbances in the context of gradual SEP events |
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259 | (6) |
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Statistical analysis of sparse data: Space plasma measurements |
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265 | (8) |
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Power-law spatial profile in an upstream region of CME-driven interplanetary shock |
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273 | (6) |
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A decade of coronagraphic and spectroscopic studies of CME-driven shocks |
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279 | (6) |
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Heliospheric three-dimensional global simulation of multiple interacting coronal mass ejections during the Halloween 2003 epoch |
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285 | (10) |
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How local is the local interstellar magnetic field? |
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295 | (7) |
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Simulations of magnetic minimum variance evolution in the solar wind |
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302 | (6) |
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The MHD simulation of the inner heliosphere over 9 years using the observation-based time-varying boundary data |
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308 | (6) |
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Insights gained using HHMS-PI from the Sun to Voyager 2 |
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314 | (7) |
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Numerical modeling of transient phenomena in the distant solar wind and in the heliosheath |
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321 | (10) |
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Plasma variability in the heliosheath |
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331 | (6) |
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Modeling the global structure of the heliosphere during the recent solar minimum: Model improvements and unipolar streamers |
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337 | (7) |
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Magnetohydrodynamic modeling of the solar wind in the outer heliosphere |
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344 | (6) |
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A preliminary analysis of dynamic and realistic heliosphere using interplanetary scintillation and photospheric magnetic data |
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350 | (6) |
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Exploration of the heliosphere and astrospheres with HST |
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356 | (7) |
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| Author Index |
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363 | |
