Index

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Index

Abbett W.: SII 26 A Magnetohydrodynamic
Abbo, L.: SI 78 Investigation of
Aboudarham J.: SVI 24 The European
AbramenkoV.: SV 5 Topological changes
Aellig M.: SIV 33 Investigations of
Ahluwalia H. S.: SI 46 A Meandering
Aletti V.: SII 31 A solar
Alexashov D.: SI 60 Modelling of
Allegrini F.: SV 46 Composition of
Allen L. A.: SII 32 A Three-fluid,
Alleyne H.: SIII 50 Terrestrial Bow
AlleyneH.: SIII 49 Plasma wave
Almeida J. S.: SII 13 Properties of
Ananthakrishnan S.: SII 41 Observations of
Anderson B. J.: SI 28 Radial Variation
Andre M.: SIII 34 Electric fields | SIII 49 Plasma wave | SIII 50 Terrestrial Bow
Andreev V.: SI 39 The Helios | SIII 23 Fine structure | SIII 25 Turbulence regimes
Andrews G. B.: SVI 12 A Realistic | SVI 15 The Energetic
Andrews M. D.: SI 3 LASCO Observations
Antiochos S.: SV 10 Composition and | SV 22 Simulations of | SV 38 The Origin
Antoni V.: SIII 15 Intermittency of | SV 36 Statistical properties
Antonucci E.: SI 21 Connections between | SI 78 Investigation of | SVI 22 Observing the | SVI 23 The Ultraviolet | SVI 24 The European
Araneda J. A.: SIII 44 Electromagnetic ion/beam
Arballo J.K.: SIII 63 Phase Steepened
Arber T.: SIII 61 Strongly Nonlinear
Arge C.: SI 44 A Solar | SI 50 A Simple | SI 53 Narrow coronal
Armand N.: SIII 24 Characteristics of
Astudillo H. F.: SIII 44 Electromagnetic ion/beam
Aurass H.: SV 19 Formation and
Avanov L.: SVI 20 All-sky camera
Axford W.: SII 24 Polar Plumes
Bale S. D.: SIII 34 Electric fields | SIII 38 Solar Wind | SVI 8 HELIX: A | SVI 14 A Radio
Balikhin M.: SIII 49 Plasma wave | SIII 50 Terrestrial Bow
Ballegooijen A. van: SV 45 Spectroscopy of | SVI 21 The Advanced
Balogh A.: SI 10 Open magnetic | SI 38 Ulysses observations | SI 70 Ulysses observations | SI 73 The density | SIII 30 Solar wind | SIV 37 Characterization of
Bamert K.: SI 24 Velocity dispersion | SIV 44 Charge-to-mass fractionation | SIV 45 Charge-to-mass fractionation
Barraclough B. L.: SIV 26 Comparison of
Bates I.: SIII 49 Plasma wave
Bavassano B.: SIII 1 Observations of | SIII 18 Alfenic turbulence | SIII 19 On the | SVI 10 Solar wind
Bedini P. D.: SVI 9 Solar Probe:
Ben-Jaffel L.: SV 25 Interstellar magnetic
Bentley B.: SVI 24 The European
Berdichevsky D.: SV 31 March 23-April | SV 35 Long-Distance coherence
Bhattacharjee A.: SIII 14 Anisotropic MHD
Bieber J. W.: SI 59 Sensitivity of | SIV 25 Cosmic Ray | SIV 41 Parallel and | SV 28 Mirroring within
Biesecker D.: SII 28 Solar wind
Bird M.: SI 39 The Helios | SII 14 Flow sources | SIII 16 On the | SIII 23 Fine structure | SIII 24 Characteristics of | SIII 25 Turbulence regimes
Biskamp D.: SIII 12 MHD turbulence
Blanco-Cano X.: SIII 33 Three second
Blush L. M.: SIV 33 Investigations of
Bochsler P.: SIV 33 Investigations of | SIV 34 Abundance Variations | SV 37 SOHO CTOF | SV 46 Composition of | SVI 13 Interstellar Pathfinder:
Bogdanov A. T.: SIV 38 Elemental Abundances
Bokulic R. S.: SVI 12 A Realistic
Bondi M.: SIII 2 Radial Evolution
Boone B. G.: SVI 12 A Realistic
Bosqued J. M.: SIII 30 Solar wind | SIII 62 Anomalous scaling
Bothmer V.: SV 8 Solar Wind
Bougeret J.-L.: SIII 39 WIND observations | SVI 5 Prospects for | SVI 14 A Radio
Boyle M. P.: SVI 12 A Realistic
Breech B.: SIII 51 Electric field
Breen A.: SII 43 Interplanetary scintillation
Breus T.: SII 24 Polar Plumes
Bruno R.: SIII 15 Intermittency of | SIII 18 Alfenic turbulence | SIII 19 On the | SIII 30 Solar wind | SIII 62 Anomalous scaling | SVI 10 Solar wind
Buchlin E.: SII 31 A solar
Buffington A.: SI 12 Time-Dependent Tomography
Burch J.: SV 43 Observations of
Burger R. A.: SI 59 Sensitivity of
Burlaga L. F.: SI 2 The heliospheric | SI 64 The Termination | SIII 54 Exploring the | SV 29 ACE Observations | SV 30 Comparison of
Buti B.: SIII 63 Phase Steepened | SIII 64 Dispersive and
Bzowski M.: SI 65 Solar wind
Canals A.: SII 43 Interplanetary scintillation
Cane H. V.: SIV 6 Solar flares, | SV 2 Spatial Relationship
Carbone V.: SIII 15 Intermittency of | SIII 19 On the | SV 5 Topological changes | SV 36 Statistical properties
Cargill P.: SV 3 Interaction of | SV 8 Solar Wind
Carlson C. W.: SIII 30 Solar wind | SIII 62 Anomalous scaling
Cattaneo M. B.: SIII 30 Solar wind | SIII 62 Anomalous scaling | SVI 10 Solar wind
Cavazzana R.: SIII 15 Intermittency of | SV 36 Statistical properties
CELIAS team: SIV 33 Investigations of
Chang T.: SII 4 Comparison of | SIII 27 ''Complexity'' Induced
Chashei I.: SIII 16 On the | SIII 24 Characteristics of | SIII 25 Turbulence regimes
Chen Y.: SII 16 Constraints on
Chian A. C.-L.: SIII 56 Alfven Turbulence
Chornay D.: SVI 20 All-sky camera
Christian E. R.: SIV 5 Are Solar | SIV 16 The Coronal | SIV 20 Coronal Abundances | SIV 22 Elemental Fractionation | SIV 32 Long-Term Fluences | SIV 35 How Common | SIV 40 Time Variations
Chuychai P.: SIV 42 Random Walk
Ciaravella A.: SV 45 Spectroscopy of | SVI 21 The Advanced
Cid C.: SV 23 The geoeffectiveness
Ciminiera L.: SVI 24 The European
Clack D.: SIII 55 Characteristics of
Classen H.-T.: SIV 14 On Electron | SV 19 Formation and
Clem J.: SIV 25 Cosmic Ray
Clette F.: SV 8 Solar Wind
Coffey, V.: SVI 20 All-sky camera
Cohen C. M. S.: SIV 5 Are Solar | SIV 16 The Coronal | SIV 20 Coronal Abundances | SIV 22 Elemental Fractionation | SIV 32 Long-Term Fluences | SIV 35 How Common | SIV 40 Time Variations | SV 29 ACE Observations | SV 30 Comparison of
Coles W. A.: SII 41 Observations of
Collier M. R.: SV 43 Observations of | SVI 20 All-sky camera
Cranmer S.: SVI 21 The Advanced
Cravens T. E.: SIV 15 Remote Sensing | SVI 7 Temporal and
Crooker N.: SI 16 The Nature | SI 45 Parameterizing the | SVI 16 Heliospheric Constellation:
Csillaghy A.: SVI 24 The European
Cummings A. C.: SI 4 The Location | SI 32 Mean Free | SIV 5 Are Solar | SIV 13 The Composition | SIV 16 The Coronal | SIV 20 Coronal Abundances | SIV 22 Elemental Fractionation | SIV 32 Long-Term Fluences | SIV 35 How Common | SIV 40 Time Variations
Cyr O. C. S.: SI 57 CMEs at
Czechowski A.: SV 15 Emission of
D'Amicis R.: SVI 10 Solar wind
Dahlburg R.: SII 46 Evolution of
Daibog E. I.: SIV 43 Invariance of
Dalgarno A.: SIV 15 Remote Sensing
Dalla S.: SIV 37 Characterization of | SIV 39 Multi-spacecraft observations
Dandouras I.: SIII 30 Solar wind | SIII 57 Magnetic holes | SIII 62 Anomalous scaling
Dasgupta B.: SIII 63 Phase Steepened
Dasso S.: SIII 52 Cross helicity | SV 42 The Magnetic
Davila J.: SI 26 Development of | SVI 21 The Advanced
Davis A. J.: SIV 32 Long-Term Fluences
Deane A.: SI 31 Three-Dimensional MHD | SIII 7 The Effects
Decker R. B.: SIV 29 ACE observations
Del Zanna L.: SIII 58 Nonlinear evolution
Demoulin P.: SV 42 The Magnetic
Deppo V. D.: SVI 23 The Ultraviolet
Desai M. I.: SIV 2 The Suprathermal | SIV 29 ACE observations | SV 29 ACE Observations | SV 30 Comparison of
Deters R.: SVI 12 A Realistic
Devore C. R.: SV 22 Simulations of
Dezeeuw D.: SV 1 3D Global | SVI 1 From the | SVI 17 3D Adaptive
Dmitriev A.: SV 8 Solar Wind | SV 16 Binary distributions
Dmitruk P.: SII 33 Coronal magnetohydrodynamic | SII 34 MHD turbulence
Dolla L.: SII 36 A search
Dorman L. I.: SI 36 Using galactic | SI 40 Changing of | SI 41 Solar Wind | SI 42 Solar Wind | SI 43 Solar Wind | SIV 17 Possible using
Dors E. E.: SIV 26 Comparison of
Dougherty M. K.: SIII 3 Electric Fluctuations
Dubinin E.: SIII 21 Solitons and | SIII 41 Nonlinear waves
Duldig M. L.: SIV 25 Cosmic Ray
Dunlop M.: SIII 50 Terrestrial Bow
Dwyer J. R.: SIV 2 The Suprathermal | SIV 21 Composition Variations | SIV 22 Elemental Fractionation | SIV 32 Long-Term Fluences | SIV 35 How Common | SV 29 ACE Observations | SV 30 Comparison of
Edenhofer P.: SIII 23 Fine structure | SIII 24 Characteristics of | SIII 25 Turbulence regimes
Edgar R. J.: SII 16 Constraints on
Efimov A.: SI 39 The Helios | SIII 16 On the | SIII 23 Fine structure | SIII 24 Characteristics of | SIII 25 Turbulence regimes
Einaudi G.: SII 31 A solar | SII 46 Evolution of
Elliott H. A.: SI 66 Solar Wind | SI 69 Latitudinal Extent
Endeve E.: SII 29 2D MHD-models
Erdelyi R.: SII 38 MHD wave
Erdos G.: SI 73 The density
Eselevich M. V.: SI 22 The common | SI 23 The fine
Eselevich V. G.: SI 22 The common | SI 23 The fine
Esser R.: SII 2 Observational and | SII 16 Constraints on | SVI 21 The Advanced
Evenson P.: SIV 25 Cosmic Ray
EvensonP.: SV 28 Mirroring within
Ewing M.: SVI 12 A Realistic
Fahr H. J.: SI 30 A revised
Fainberg J.: SV 20 Complexity Of
Fainshtein V. G.: SV 14 Some dynamic
Farrugia C.: SIV 34 Abundance Variations | SV 31 March 23-April | SV 34 Coherence Lengths | SV 35 Long-Distance coherence
Fazakerley A.: SIII 57 Magnetic holes
Fennell J.: SVI 16 Heliospheric Constellation:
Feynman J.: SVI 16 Heliospheric Constellation:
Fichtner H.: SII 18 On the
Figuero-Vinas A.: SV 20 Complexity Of
Fineschi S.: SVI 21 The Advanced | SVI 22 Observing the | SVI 23 The Ultraviolet
Finkelstein A.: SVI 24 The European
Fisk L. A.: SII 10 The Acceleration | SV 10 Composition and | SVI 13 Interstellar Pathfinder:
Fitzenreiter R.: SV 20 Complexity Of
Florinski V. A.: SIV 31 Galactic cosmic
Fludra A.: SI 26 Development of
Fok M.-C.: SV 43 Observations of
Forman M. A.: SIII 53 Castaing scaling | SIII 54 Exploring the
Formisano V.: SIII 30 Solar wind | SIII 62 Anomalous scaling
Forsyth R.: SI 70 Ulysses observations | SIII 3 Electric Fluctuations | SV 11 ICME observations
Fraeman M. E.: SVI 12 A Realistic
Fraenz M.: SIII 57 Magnetic holes
François L.: SII 15 How does
Fujiki K.: SI 33 Evidences for | SI 34 Solar Cycle | SI 35 MHD Tomography | SI 66 Solar Wind | SV 18 Three-Dimensional Global
Funsten H.: SVI 13 Interstellar Pathfinder: | SVI 16 Heliospheric Constellation:
Fuselier S.: SV 43 Observations of
Gallagher D.: SVI 20 All-sky camera
Galtier S.: SII 31 A solar | SIII 43 A Weak
Galvan C.: SIII 63 Phase Steepened
Galvin A.: SIV 3 Ionic Charge | SIV 19 Comparison of | SIV 34 Abundance Variations | SIV 38 Elemental Abundances | SV 31 March 23-April | SV 35 Long-Distance coherence | SV 46 Composition of | SVI 2 Future Prospects
Gangopadhyay P.: SI 52 Interpretation of
Gardiol D.: SVI 22 Observing the | SVI 23 The Ultraviolet
Gardner L.: SVI 21 The Advanced
Gary S. P.: SII 27 Alpha Acceleration | SII 35 Heating and | SIII 48 Solar Wind
Gazis P. R.: SI 54 A Large-Scale
Geiss J.: SI 72 Fast Solar | SII 10 The Acceleration | SVI 13 Interstellar Pathfinder:
Genot V.: SIII 57 Magnetic holes
Geranios A.: SV 4 Comparison of
Gherardi A.: SVI 23 The Ultraviolet
Giacalone J.: SIV 10 Particle acceleration
Giannotti C.: SIII 64 Dispersive and
Gibson S.: SI 26 Development of
Giuliani P.: SV 36 Statistical properties
Gloeckler G.: SI 72 Fast Solar | SII 10 The Acceleration | SIV 3 Ionic Charge | SIV 4 Ubiquitous suprathermal | SIV 19 Comparison of | SIV 32 Long-Term Fluences | SV 29 ACE Observations | SV 30 Comparison of | SVI 13 Interstellar Pathfinder:
Goetz K.: SVI 14 A Radio
Gold R. E.: SIV 21 Composition Variations | SIV 32 Long-Term Fluences | SIV 35 How Common | SV 29 ACE Observations | SV 30 Comparison of | SVI 12 A Realistic
Goldstein B. E.: SII 12 Recent work | SIII 63 Phase Steepened | SVI 16 Heliospheric Constellation:
Goldstein M. L.: SI 31 Three-Dimensional MHD | SIII 5 Three-dimensional MHD | SIII 7 The Effects
Gombosi T.: SV 1 3D Global | SVI 1 From the | SVI 17 3D Adaptive
GombosiT.: SV 43 Observations of
Gonzalez-Esparza A.: SI 56 Numerical study | SI 58 Five-Spacecraft Observations
Gopalswamy N.: SI 56 Numerical study | SIV 12 Effect of | SV 44 Propagation Characteristics
Gori L.: SVI 23 The Ultraviolet
Gosling J. T.: SI 7 Is the | SI 55 Characterization of | SI 57 CMEs at | SI 76 On the | SIV 23 An Overview | SV 2 Spatial Relationship | SVI 16 Heliospheric Constellation:
Grünwaldt H.: SV 37 SOHO CTOF
Grappin R.: SII 8 Large amplitude | SIII 12 MHD turbulence | SIII 28 Hybrid simulations | SIII 64 Dispersive and | SV 26 Flows in
Greco A.: SII 7 Collisional filtration
Grib S. A.: SV 41 The Effect
Gruntman M.: SI 52 Interpretation of | SVI 13 Interstellar Pathfinder:
Guhathakurta M.: SI 26 Development of | SVI 6 NASA's Living
Gurman J.: SVI 24 The European
Gurnett D. A.: SIII 3 Electric Fluctuations
Habbal S. R.: SI 6 Observational evidence | SII 8 Large amplitude | SII 11 Characteristics of | SII 39 Effect of | SII 44 Connecting the
Hada T.: SIII 42 Phase coherence
Haggerty D.: SV 29 ACE Observations | SV 30 Comparison of | SVI 13 Interstellar Pathfinder:
Hakamada K.: SI 33 Evidences for
Haley D. R.: SVI 12 A Realistic
Hansteen V. H.: SII 17 Effect of | SII 30 Outer atmospheres | SIV 18 Thermal forces
Harvey K.: SI 53 Narrow coronal
Hayashi K.: SI 33 Evidences for | SI 35 MHD Tomography
Heber B.: SIV 37 Characterization of
HELIX team: SVI 8 HELIX: A
Hellinger P.: SIII 28 Hybrid simulations | SIII 29 Global hybrid
Hick P.: SI 12 Time-Dependent Tomography
Hidalgo M. A.: SV 23 The geoeffectiveness
Hilchenbach M.: SI 24 Velocity dispersion | SIV 34 Abundance Variations | SIV 44 Charge-to-mass fractionation | SV 15 Emission of
Hill F.: SVI 24 The European
Hiltula T.: SI 17 A systematic
Ho G.: SIV 21 Composition Variations | SIV 29 ACE observations | SVI 15 The Energetic
Hoang S.: SI 8 Large-Scale Structure | SI 68 Large-scale and
Hochedez J.-F.: SV 8 Solar Wind
Hoeksema J.: SI 44 A Solar
Hofer M.: SI 48 Composition Measurements | SI 71 Repeated Structures
Hollweg J. V.: SII 19 Ion heating
Holzer T.: SI 26 Development of
Horbury T.: SIII 57 Magnetic holes
Hospodarsky G. B.: SIII 3 Electric Fluctuations
Howard D. R.: SI 3 LASCO Observations | SVI 21 The Advanced
Hsieh K. C.: SV 15 Emission of
Hubert D.: SII 15 How does | SIII 38 Solar Wind
Hudson H. S.: SI 53 Narrow coronal
Hulburt E. O.: SI 2 The heliospheric
Humble J. E.: SIV 25 Cosmic Ray
Ipavich F.: SV 37 SOHO CTOF | SV 46 Composition of
Isenberg P.: SII 6 Ion-Cyclotron Generation | SIII 31 A Kinetic | SV 37 SOHO CTOF
Issautier K.: SI 8 Large-Scale Structure | SI 68 Large-scale and | SII 5 Basic aspects
Iucci N.: SI 41 Solar Wind | SI 42 Solar Wind | SI 43 Solar Wind
Izmodenov V. V.: SI 9 Hydrogen wall | SI 52 Interpretation of | SI 60 Modelling of
Jackson B. V.: SI 12 Time-Dependent Tomography
Janardhan P.: SII 14 Flow sources | SIII 23 Fine structure
Jokipii J. R.: SI 18 Probing the | SIV 10 Particle acceleration
Jones G. H.: SI 38 Ulysses observations
Jordanova V. K.: SV 35 Long-Distance coherence
Judge D.: SI 52 Interpretation of | SVI 13 Interstellar Pathfinder:
Jurac S.: SVI 19 The scale
Kahler S. W.: SI 45 Parameterizing the | SI 53 Narrow coronal
Kaiser M. L.: SI 37 CME Dynamics | SIV 12 Effect of
Kallenbach R.: SI 24 Velocity dispersion | SIV 44 Charge-to-mass fractionation | SIV 45 Charge-to-mass fractionation | SIV 46 Isotopic Fractionation
Karpen J. T.: SV 38 The Origin
Kasper J. C.: SI 49 Solar Wind | SIII 48 Solar Wind | SIII 55 Characteristics of | SVI 19 The scale
Keath E.: SVI 15 The Energetic
Kecskemety K.: SIV 43 Invariance of
Keller J.: SVI 20 All-sky camera
Kellogg P. J.: SIII 3 Electric Fluctuations | SIII 38 Solar Wind | SIII 39 WIND observations | SIII 47 Comparison of
Keppler E.: SIV 14 On Electron
Kharchenko V.: SIV 15 Remote Sensing
Killie M. A.: SII 30 Outer atmospheres
Kistler L. M.: SIII 30 Solar wind | SIII 62 Anomalous scaling | SIV 38 Elemental Abundances
Klassen A.: SV 19 Formation and
Klecker B.: SI 24 Velocity dispersion | SIII 30 Solar wind | SIII 62 Anomalous scaling | SIV 3 Ionic Charge | SIV 19 Comparison of | SIV 34 Abundance Variations | SIV 38 Elemental Abundances | SIV 44 Charge-to-mass fractionation | SV 37 SOHO CTOF
Koga D.: SIII 42 Phase coherence
Kohl J.: SVI 21 The Advanced
Kojima M.: SI 33 Evidences for | SI 34 Solar Cycle | SI 35 MHD Tomography | SI 66 Solar Wind | SV 18 Three-Dimensional Global | SV 27 Radial dependence
Kortenkamp P. S.: SIII 2 Radial Evolution
Korth A.: SIII 30 Solar wind | SIII 62 Anomalous scaling
Kota J.: SI 18 Probing the | SIV 10 Particle acceleration
Krasnoselskikh V.: SII 20 Multi-scale energy | SII 21 Classification of
Krimigis S.: SIV 32 Long-Term Fluences | SIV 35 How Common | SVI 13 Interstellar Pathfinder:
Krishnan R.: SVI 12 A Realistic
Krucker S.: SIV 37 Characterization of
Kucharek H.: SIV 34 Abundance Variations | SV 37 SOHO CTOF
Kurth W. S.: SIII 3 Electric Fluctuations
Kyr'ol'a E.: SI 65 Solar wind
Léorat J.: SII 8 Large amplitude | SV 26 Flows in
Lacombe C.: SIII 38 Solar Wind | SIII 39 WIND observations
Laitinen T. L.: SII 18 On the
Lakhina G.S.: SIII 63 Phase Steepened
Lallement R.: SI 9 Hydrogen wall
Lamy H.: SII 22 The minor | SII 23 New exospheric | SII 45 A kinetic
Landi E.: SII 1 Plasma velocities
Landi S.: SII 42 Kinetic simulations
Landini F.: SVI 23 The Ultraviolet
Lanzerotti L. J.: SI 74 Time Series | SIII 59 Coherent and
Lara A.: SI 56 Numerical study
Lario D.: SIV 21 Composition Variations | SIV 29 ACE observations
Larson D. E.: SI 19 Cold electrons | SI 45 Parameterizing the | SIII 38 Solar Wind
Lazarus A.: SI 49 Solar Wind | SIII 48 Solar Wind | SIII 55 Characteristics of | SVI 19 The scale
Le G.: SIII 33 Three second
Leamon R. L.: SIII 13 Solar Wind
Ledvina S.: SII 26 A Magnetohydrodynamic
Lee M. A.: SIV 19 Comparison of | SV 37 SOHO CTOF
Leer E.: SII 17 Effect of | SII 30 Outer atmospheres | SIV 18 Thermal forces
Lefebvre B.: SII 20 Multi-scale energy | SII 21 Classification of
Lellis A. M. Di: SIII 62 Anomalous scaling
Lemaire J.: SII 22 The minor | SII 45 A kinetic
Lemaire P.: SII 36 A search
Lepping R.: SV 31 March 23-April | SV 35 Long-Distance coherence
Lepreti F.: SIII 15 Intermittency of | SV 36 Statistical properties
Lepri S. T.: SIV 9 Anomalous composition
Leske R. A.: SIV 5 Are Solar | SIV 12 Effect of | SIV 16 The Coronal | SIV 20 Coronal Abundances | SIV 22 Elemental Fractionation | SIV 32 Long-Term Fluences | SIV 35 How Common | SIV 40 Time Variations | SV 29 ACE Observations | SV 30 Comparison of
Lester D.: SVI 12 A Realistic
Levy G.: SI 39 The Helios
Li G.: SIV 27 Particle Acceleration | SIV 28 The Transport
Li W.: SIV 34 Abundance Variations
Li X.: SII 9 Heating in | SII 32 A Three-fluid, | SII 39 Effect of
Li Y.: SI 44 A Solar
Lie-Svendsen Ø.: SII 16 Constraints on | SII 17 Effect of | SIV 18 Thermal forces
Liewer P. C.: SI 5 Active Region | SII 12 Recent work | SIII 64 Dispersive and | SVI 16 Heliospheric Constellation: | SVI 17 3D Adaptive
Lin N.: SIII 47 Comparison of
Lin R.: SI 19 Cold electrons | SIII 38 Solar Wind | SVI 8 HELIX: A | SVI 13 Interstellar Pathfinder:
Linker J. A.: SI 13 Understanding the | SI 61 Three-dimensional Magnetohydrodynamic | SV 7 Models of
Lionello R.: SI 61 Three-dimensional Magnetohydrodynamic
Litvinenko Y.: SV 37 SOHO CTOF
Livi S.: SVI 13 Interstellar Pathfinder: | SVI 15 The Energetic
Londrillo P.: SIII 58 Nonlinear evolution
Lopate C.: SIV 11 Solar Energetic
Lotova N. A.: SI 25 Evolution of | SII 14 Flow sources
Luhmann J.: SI 44 A Solar | SII 26 A Magnetohydrodynamic
Lundin R.: SIII 30 Solar wind | SIII 62 Anomalous scaling
Lyman R.: SVI 12 A Realistic
Lynch B. J.: SV 10 Composition and
Müller W.: SIII 12 MHD turbulence
M'akinen T.: SI 65 Solar wind
Macdowall R. J.: SIII 47 Comparison of
Macek W. M.: SIII 46 The multifractal
Maclennan C. G.: SI 74 Time Series | SIII 59 Coherent and
Macneice P. J.: SV 6 Numerical Simulation | SV 22 Simulations of | SV 38 The Origin
Maksimovic M.: SII 5 Basic aspects | SII 22 The minor | SII 23 New exospheric | SII 45 A kinetic | SVI 14 A Radio
Malara F.: SIII 35 Parametric instability
Malvezzi M. A.: SVI 23 The Ultraviolet
Manchester W. B.: SV 1 3D Global | SVI 1 From the | SVI 17 3D Adaptive
Mandrini C.: SV 42 The Magnetic
Mangeney A.: SII 5 Basic aspects | SIII 28 Hybrid simulations
Mann G. J.: SIII 22 Kinetics of | SIV 14 On Electron | SV 19 Formation and
Manning R. E.: SVI 14 A Radio
Manoharan P.: SV 44 Propagation Characteristics
Mantovani F.: SIII 2 Radial Evolution
Markovskii S. A.: SII 19 Ion heating
Marsch E.: SII 25 Equatorial Coronal | SIII 4 Cyclotron-resonant diffusion | SIII 6 The microscopic
Marsden R. G.: SI 48 Composition Measurements | SVI 4 Solar Dynamics
Martines E.: SIII 15 Intermittency of
Mason G. M.: SIV 2 The Suprathermal | SIV 21 Composition Variations | SIV 22 Elemental Fractionation | SIV 24 3He-rich solar | SIV 32 Long-Term Fluences | SIV 35 How Common | SV 29 ACE Observations | SV 30 Comparison of
MASSE Science Team: SVI 11 Multi-Angle Exploration
Matsui H.: SV 34 Coherence Lengths | SV 35 Long-Distance coherence
Matsuoka A.: SI 27 NOZOMI observation
Matthaeus W. H.: SI 59 Sensitivity of | SII 33 Coronal magnetohydrodynamic | SII 34 MHD turbulence | SIII 10 The Interaction | SIII 13 Solar Wind | SIII 37 Nearly Incompressible | SIII 51 Electric field | SIII 52 Cross helicity | SIV 36 A Quasi-linear | SIV 41 Parallel and | SIV 42 Random Walk
Mayer L.: SI 50 A Simple
Mazur J. E.: SIV 2 The Suprathermal | SIV 21 Composition Variations | SIV 22 Elemental Fractionation | SIV 24 3He-rich solar | SIV 32 Long-Term Fluences | SIV 35 How Common | SV 29 ACE Observations | SV 30 Comparison of | SVI 16 Heliospheric Constellation:
McAdams J. V.: SVI 12 A Realistic
McCarthy M.: SIII 62 Anomalous scaling
McCarthyM.: SIII 30 Solar wind
McComas D. J.: SI 1 The Three-Dimensional | SI 55 Characterization of | SI 66 Solar Wind | SI 69 Latitudinal Extent | SI 70 Ulysses observations | SI 72 Fast Solar | SIV 23 An Overview | SV 29 ACE Observations | SV 30 Comparison of | SV 43 Observations of | SVI 13 Interstellar Pathfinder:
McFadden J. P.: SIII 30 Solar wind | SIII 62 Anomalous scaling
McKenzie J.: SII 24 Polar Plumes | SIII 21 Solitons and | SIII 41 Nonlinear waves | SV 25 Interstellar magnetic
McKibben R. B.: SIV 11 Solar Energetic
McNutt R. L.: SI 51 Fluid modeling | SVI 12 A Realistic | SVI 13 Interstellar Pathfinder: | SVI 15 The Energetic
McPherson M.: SVI 12 A Realistic
Messerotti M.: SVI 24 The European
Mewaldt R. A.: SI 14 Recent Observations | SIV 5 Are Solar | SIV 16 The Coronal | SIV 20 Coronal Abundances | SIV 22 Elemental Fractionation | SIV 32 Long-Term Fluences | SIV 35 How Common | SIV 40 Time Variations
Meyer-Vernet N.: SII 5 Basic aspects
Michalek G.: SIV 12 Effect of
Mikic Z.: SI 13 Understanding the | SI 61 Three-dimensional Magnetohydrodynamic | SV 7 Models of
Milano L.: SII 33 Coronal magnetohydrodynamic | SIII 51 Electric field | SIII 52 Cross helicity | SIV 36 A Quasi-linear
Mitchell D.: SVI 13 Interstellar Pathfinder: | SVI 15 The Energetic
Moebius E.: SIII 30 Solar wind | SIII 62 Anomalous scaling | SIV 3 Ionic Charge | SIV 19 Comparison of | SIV 34 Abundance Variations | SIV 38 Elemental Abundances | SV 29 ACE Observations | SV 30 Comparison of | SV 37 SOHO CTOF | SVI 3 Where do | SVI 13 Interstellar Pathfinder:
Moldwin M. B.: SVI 16 Heliospheric Constellation:
Moncuquet M.: SI 8 Large-Scale Structure | SI 68 Large-scale and
Moore T.: SV 43 Observations of | SVI 20 All-sky camera
Morgan H.: SII 44 Connecting the
Morris D.: SIV 19 Comparison of
Moullard O.: SIII 57 Magnetic holes
Mountford C. J.: SII 39 Effect of
MozerF. S.: SIII 34 Electric fields
Mueller H.: SI 15 Modeling heavy | SI 63 Benefits of | SV 32 Influence of
Mueller-Mellin R.: SIV 37 Characterization of
Mullan D. J.: SIII 36 Day the
Mulligan T.: SI 28 Radial Variation | SI 29 The Limitation
Murphy N.: SI 75 Strongly Underwound
Mursula K.: SI 17 A systematic | SI 67 Annual and | SV 24 Mid-term periodicities | SV 33 Long-term occurrence
Naes L.: SVI 12 A Realistic
Nakagawa T.: SI 27 NOZOMI observation
Nakariakov V.: SIII 60 A Three | SIII 61 Strongly Nonlinear
Naletto G.: SVI 22 Observing the | SVI 23 The Ultraviolet
Nazarenko S. V.: SIII 43 A Weak
Ness N. F.: SI 2 The heliospheric | SIII 36 Day the | SV 29 ACE Observations | SV 30 Comparison of
Neugebauer M.: SI 5 Active Region | SIII 63 Phase Steepened | SIV 26 Comparison of
Newell A. C.: SIII 43 A Weak
Ng C.-S.: SIII 14 Anisotropic MHD
Nicolosi P.: SVI 23 The Ultraviolet
Nieves-Chinchilla T.: SV 23 The geoeffectiveness
Noci G.: SVI 21 The Advanced
Noullez A.: SV 5 Topological changes
NOZOMI MGF team: SI 27 NOZOMI observation
Obridko V. N.: SI 25 Evolution of | SII 14 Flow sources
Odstrcil D.: SI 50 A Simple | SV 6 Numerical Simulation
Ofman L.: SI 26 Development of | SII 27 Alpha Acceleration | SII 35 Heating and | SV 26 Flows in
Ogilvie K.: SV 31 March 23-April
Ohmi T.: SI 33 Evidences for | SI 34 Solar Cycle | SI 66 Solar Wind
Opher M.: SV 1 3D Global | SVI 17 3D Adaptive
Osherovich V. A.: SV 20 Complexity Of
Oughton S.: SII 33 Coronal magnetohydrodynamic | SIII 11 Waves and | SIII 13 Solar Wind
Pace E.: SVI 23 The Ultraviolet
Pallocchia G.: SIII 30 Solar wind | SIII 62 Anomalous scaling | SVI 10 Solar wind
Pantellini F.: SII 5 Basic aspects | SII 37 On the | SII 42 Kinetic simulations
Parhi S.: SI 59 Sensitivity of
Parisi M.: SI 41 Solar Wind | SI 42 Solar Wind | SI 43 Solar Wind
Parks G. K.: SIII 30 Solar wind | SIII 62 Anomalous scaling
Passot T.: SIII 32 Influence of | SIII 40 Magnetic pressure
Pelizzo M. G.: SVI 23 The Ultraviolet
Perez-Tijerina E.: SI 56 Numerical study
Pierrard V.: SII 22 The minor | SII 23 New exospheric
PierrardV.: SII 45 A kinetic
Pietropaolo E.: SIII 18 Alfenic turbulence | SIII 19 On the
Pike D.: SVI 24 The European
Pizzo V.: SI 50 A Simple | SV 6 Numerical Simulation | SVI 16 Heliospheric Constellation:
Plettemeier D.: SIII 23 Fine structure | SIII 24 Characteristics of | SIII 25 Turbulence regimes
Podladchikov V.: SII 21 Classification of
Podladchikova O.: SII 20 Multi-scale energy | SII 21 Classification of
Pogorelov N. V.: SIV 31 Galactic cosmic
Poletto G.: SI 20 Solar wind | SII 1 Plasma velocities | SII 28 Solar wind
Politano H.: SV 5 Topological changes
Pommois P.: SIII 8 Magnetic turbulence, | SIII 26 Particle transport
Popecki M. A.: SIV 3 Ionic Charge | SIV 19 Comparison of | SIV 34 Abundance Variations | SIV 38 Elemental Abundances | SV 29 ACE Observations | SV 30 Comparison of
Potocki K. A.: SVI 9 Solar Probe:
Pouquet A.: SIII 43 A Weak | SV 5 Topological changes
Powell K.: SV 1 3D Global | SVI 1 From the | SVI 17 3D Adaptive
Prenger R. J.: SIII 34 Electric fields
Primavera L.: SIII 35 Parametric instability
Pyle R.: SIV 25 Cosmic Ray | SV 28 Mirroring within
Qin G.: SIV 41 Parallel and
Quémerais E.: SI 65 Solar wind
Quereshi N. S.: SIII 30 Solar wind
Ramirez J.: SIII 33 Three second
Rao A. P.: SII 41 Observations of
Rappazzo F.: SII 46 Evolution of
Ratkiewicz R.: SII 24 Polar Plumes | SV 25 Interstellar magnetic
Raymond J.: SV 45 Spectroscopy of | SVI 21 The Advanced
Read D.: SVI 12 A Realistic
Reames D.: SIV 12 Effect of | SV 31 March 23-April
Reardon K.: SVI 24 The European
Regnoli G.: SV 36 Statistical properties
Reinard A. A.: SIV 9 Anomalous composition | SIV 26 Comparison of
Reiner M. J.: SI 37 CME Dynamics
Reisenfeld D. B.: SI 57 CMEs at | SIV 26 Comparison of | SIV 26 Comparison of
Reme H.: SIII 30 Solar wind | SIII 57 Magnetic holes | SIII 62 Anomalous scaling
Rempel E. L.: SIII 56 Alfven Turbulence
Rice W.: SIII 10 The Interaction | SIV 27 Particle Acceleration | SIV 28 The Transport
Richardson I.: SV 2 Spatial Relationship | SV 31 March 23-April | SV 35 Long-Distance coherence
Richardson J.: SI 11 The Solar | SV 17 The interaction | SVI 19 The scale
Riley P.: SI 13 Understanding the | SI 57 CMEs at | SI 69 Latitudinal Extent
Roberts D. A.: SI 31 Three-Dimensional MHD | SIII 7 The Effects
Robertson I.: SVI 7 Temporal and
Roelof E.: SIV 8 CME-driven coronal | SIV 14 On Electron | SIV 21 Composition Variations | SIV 29 ACE observations | SVI 13 Interstellar Pathfinder:
Romashets E.: SI 47 Propagation of | SV 3 Interaction of | SV 8 Solar Wind
Romoli M.: SII 28 Solar wind | SVI 21 The Advanced | SVI 22 Observing the | SVI 23 The Ultraviolet
Rosenvinge T., von: SIV 5 Are Solar | SIV 12 Effect of | SIV 16 The Coronal | SIV 20 Coronal Abundances | SIV 22 Elemental Fractionation | SIV 32 Long-Term Fluences | SIV 35 How Common | SIV 40 Time Variations
Roussev I.: SV 1 3D Global | SVI 1 From the | SVI 17 3D Adaptive
Roux J. A. le: SIV 36 A Quasi-linear
Ruderman M.: SIII 50 Terrestrial Bow
Ruffolo D.: SIV 42 Random Walk | SV 28 Mirroring within
Rujiwarodom M.: SV 28 Mirroring within
Russell C. T.: SI 28 Radial Variation | SI 29 The Limitation | SIII 33 Three second | SVI 16 Heliospheric Constellation:
Ruzmaikin A.: SVI 11 Multi-Angle Exploration
Sabbah I.: SI 77 Internal relations
Sakurai T.: SII 3 Relation Between
Salem C.: SIII 38 Solar Wind | SIII 39 WIND observations
Samoznaev L.: SI 39 The Helios | SIII 23 Fine structure | SIII 24 Characteristics of | SIII 25 Turbulence regimes
Sanderson T.: SI 48 Composition Measurements
Santillan A.: SI 56 Numerical study
Santo A. G.: SVI 12 A Realistic
Sauer K.: SIII 21 Solitons and | SIII 41 Nonlinear waves
Saul L. A.: SV 37 SOHO CTOF
Sauvaud J.-A.: SIII 30 Solar wind | SIII 62 Anomalous scaling
Schmidt J.: SV 3 Interaction of
Scholl I.: SVI 24 The European
Schwadron N.: SI 75 Strongly Underwound | SII 10 The Acceleration | SIV 7 Pickup Ion | SIV 15 Remote Sensing | SVI 13 Interstellar Pathfinder:
Schwenn R.: SV 9 The angular | SV 31 March 23-April | SV 35 Long-Distance coherence
Seidel B.: SI 39 The Helios
Severino G.: SVI 24 The European
Sheeley N. R.: SI 2 The heliospheric | SI 64 The Termination
Shimazu H.: SV 21 A self-similar
Shimizu Y.: SI 34 Solar Cycle
Sierks H.: SI 24 Velocity dispersion
Silbergleit V. M.: SIV 47 Solar Wind
Simnett G. M.: SIV 8 CME-driven coronal
Sittler E. C.: SI 26 Development of
Skoug R. M.: SI 26 Development of | SI 55 Characterization of | SI 76 On the | SIII 36 Day the | SIV 23 An Overview | SV 29 ACE Observations | SV 30 Comparison of | SV 39 The Transition
Slocum P. L.: SIV 16 The Coronal | SIV 20 Coronal Abundances | SIV 22 Elemental Fractionation | SIV 35 How Common | SIV 40 Time Variations
Smirnov V.: SVI 20 All-sky camera
Smith C. W.: SIII 9 The Geometry | SIII 13 Solar Wind | SIII 36 Day the | SIII 51 Electric field | SIII 52 Cross helicity | SIV 29 ACE observations | SV 29 ACE Observations | SV 30 Comparison of | SV 39 The Transition
Smith E. J.: SI 10 Open magnetic | SI 70 Ulysses observations | SI 75 Strongly Underwound
Smith P.: SVI 21 The Advanced
Snowden S.: SVI 7 Temporal and
Socker D.: SVI 21 The Advanced
Sokolov I.: SV 1 3D Global | SVI 1 From the | SVI 17 3D Adaptive
SolankiS. K.: SI 72 Fast Solar
Solomon J.: SII 36 A search
Sorriso-Valvo L.: SIII 15 Intermittency of | SV 5 Topological changes
Spada E.: SV 36 Statistical properties
Spangler S. R.: SIII 2 Radial Evolution
Srivastava N.: SV 40 Relation of
St.Cyr O. C.: SV 12 Observations of
Steiger R. von: SI 72 Fast Solar | SIII 45 Temperature Anisotropies | SIV 9 Anomalous composition
Steinberg J. T.: SI 57 CMEs at | SIII 36 Day the | SIV 26 Comparison of
Stelzried C.: SI 39 The Helios
Stolpovskii V. G.: SIV 43 Invariance of
Stone E. C.: SI 4 The Location | SI 32 Mean Free | SIV 5 Are Solar | SIV 13 The Composition | SIV 16 The Coronal | SIV 20 Coronal Abundances | SIV 22 Elemental Fractionation | SIV 32 Long-Term Fluences | SIV 35 How Common | SIV 40 Time Variations
Storini M.: SI 71 Repeated Structures
Strachan L.: SV 45 Spectroscopy of | SVI 21 The Advanced
Suess S. T.: SI 20 Solar wind | SII 3 Relation Between
Sulem P.-L.: SIII 32 Influence of
Summanen T.: SI 65 Solar wind
Suvorova A.: SV 16 Binary distributions
Szabo A.: SI 49 Solar Wind | SIII 48 Solar Wind | SV 39 The Transition | SVI 18 The Living
Takalo J.: SI 67 Annual and
Tam S. W.: SII 4 Comparison of
Teriaca L.: SII 28 Solar wind
Thomson D. J.: SI 74 Time Series | SIII 59 Coherent and
Tokumaru M.: SI 12 Time-Dependent Tomography | SI 33 Evidences for | SI 34 Solar Cycle | SI 35 MHD Tomography | SI 66 Solar Wind | SV 18 Three-Dimensional Global | SV 27 Radial dependence
Tooprakai P.: SV 28 Mirroring within
Torbert R. B.: SV 34 Coherence Lengths | SV 35 Long-Distance coherence
Toth G.: SV 1 3D Global | SVI 1 From the | SVI 17 3D Adaptive
Tranquille A. C.: SI 48 Composition Measurements
Travnicek P.: SIII 28 Hybrid simulations | SIII 29 Global hybrid
Tsiklauri D.: SIII 60 A Three | SIII 61 Strongly Nonlinear
Tsurutani B.T.: SIII 63 Phase Steepened
Tu C.-Y.: SIII 4 Cyclotron-resonant diffusion
Turkmani R.: SII 40 Parametric decay
Usmanov A. V.: SIII 5 Three-dimensional MHD
Vainio R.: SII 18 On the
Vaisberg O. L.: SVI 20 All-sky camera
Vandas M.: SI 47 Propagation of | SV 4 Comparison of | SV 6 Numerical Simulation | SV 21 A self-similar
Vazquez-Semadeni E.: SIII 40 Magnetic pressure
Velli M.: SII 12 Recent work | SII 31 A solar | SII 46 Evolution of | SIII 58 Nonlinear evolution | SIII 64 Dispersive and
Veltri P.: SII 7 Collisional filtration | SIII 8 Magnetic turbulence, | SIII 15 Intermittency of | SIII 26 Particle transport | SIII 35 Parametric instability | SV 5 Topological changes | SV 36 Statistical properties
Veselovsky I.: SIII 17 On the | SV 8 Solar Wind | SV 16 Binary distributions
Viñas A.: SII 35 Heating and | SIII 44 Electromagnetic ion/beam
Vial J.-C.: SII 31 A solar | SII 36 A search
Villoresi G.: SI 41 Solar Wind | SI 42 Solar Wind | SI 43 Solar Wind
Vilppola J. H.: SV 24 Mid-term periodicities
Vladimirovich G. S.: SV 14 Some dynamic
Vladimirskii K. V.: SI 25 Evolution of | SII 14 Flow sources
Vocks C.: SIII 22 Kinetics of
Volland H.: SI 39 The Helios
Walker S. N.: SIII 49 Plasma wave
Wang A.-H.: SIII 20 Coronal Mass
Wang C.: SI 11 The Solar | SV 17 The interaction
Wang L.-H.: SIII 4 Cyclotron-resonant diffusion
Wang Y.-M.: SI 2 The heliospheric | SI 62 Nature of | SI 64 The Termination
Watari S.: SV 4 Comparison of
Webb D. F.: SV 13 The Characteristics
Weygand J.: SVI 16 Heliospheric Constellation:
Whang Y. C.: SI 64 The Termination
Wiedenbeck M. E.: SIV 5 Are Solar | SIV 16 The Coronal | SIV 20 Coronal Abundances | SIV 22 Elemental Fractionation | SIV 24 3He-rich solar | SIV 32 Long-Term Fluences | SIV 35 How Common | SIV 40 Time Variations
Wiens R. C.: SIV 26 Comparison of
Williams B. D.: SVI 12 A Realistic
Wimmer-Schweingruber R. F.: SIV 1 The Composition | SIV 3 Ionic Charge | SIV 19 Comparison of | SIV 33 Investigations of | SIV 44 Charge-to-mass fractionation | SIV 45 Charge-to-mass fractionation | SV 46 Composition of
Winske D.: SII 27 Alpha Acceleration
Winterhalter D.: SIII 63 Phase Steepened
Witte M.: SVI 13 Interstellar Pathfinder:
Woch J.: SI 72 Fast Solar | SVI 13 Interstellar Pathfinder:
Wohlmuth R.: SIII 23 Fine structure | SIII 24 Characteristics of | SIII 25 Turbulence regimes
Woo R.: SI 6 Observational evidence
Wood B.: SI 9 Hydrogen wall | SI 63 Benefits of
Wu S. T.: SIII 20 Coronal Mass
Wurz P.: SIV 33 Investigations of | SV 43 Observations of | SV 46 Composition of | SVI 13 Interstellar Pathfinder:
Xia L.: SII 25 Equatorial Coronal
Yakovshuk O.: SV 16 Binary distributions
Yamamoto E.: SIII 42 Phase coherence
Yamashita M.: SI 12 Time-Dependent Tomography | SV 18 Three-Dimensional Global | SV 27 Radial dependence
Yamauchi Y.: SII 3 Relation Between
Yashiro S.: SIV 12 Effect of | SV 44 Propagation Characteristics
Yokobe A.: SI 33 Evidences for | SI 34 Solar Cycle | SI 66 Solar Wind
Yurchyshyn V.: SV 5 Topological changes
Zangrilli L.: SVI 23 The Ultraviolet
Zank G.: SI 15 Modeling heavy | SI 63 Benefits of | SIII 10 The Interaction | SIII 13 Solar Wind | SIII 37 Nearly Incompressible | SIV 27 Particle Acceleration | SIV 28 The Transport | SIV 31 Galactic cosmic | SIV 36 A Quasi-linear | SV 32 Influence of
Zhang J.: SI 72 Fast Solar
Zhao X.: SI 44 A Solar
Zharkova V.: SVI 24 The European
Zhou Y.: SIII 10 The Interaction | SIII 37 Nearly Incompressible
Zhukov A.: SV 8 Solar Wind
Zieger B.: SI 17 A systematic | SV 33 Long-term occurrence
Zimbardo G.: SIII 8 Magnetic turbulence, | SIII 26 Particle transport
Zurbuchen T. H.: SI 13 Understanding the | SI 72 Fast Solar | SII 10 The Acceleration | SIII 45 Temperature Anisotropies | SIV 3 Ionic Charge | SIV 9 Anomalous composition | SIV 19 Comparison of | SIV 26 Comparison of | SIV 32 Long-Term Fluences | SV 2 Spatial Relationship | SV 10 Composition and | SV 29 ACE Observations | SV 30 Comparison of | SVI 13 Interstellar Pathfinder:

Marco Velli
2002-05-29