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A model of interplanetary and coronal magnetic fields
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What this work says
Outgoing claims: the papers this work cites, builds on, or argues with.
inferredcites →https://doi.org/10.1007/bf00147021openalex-snapshot
A large-scale pattern in the solar magnetic field
inferredcites →https://doi.org/10.1007/bf00147968openalex-snapshot
Influence of a solar active region on the interplanetary magnetic field
inferredcites →https://doi.org/10.1007/bf00179216openalex-snapshot
Implications of solar radio bursts for the study of the solar corona
inferredcites →https://doi.org/10.1007/bf00227565openalex-snapshot
The interplanetary magnetic field. Solar origin and terrestrial effects
inferredcites →https://doi.org/10.1029/jz070i023p05793openalex-snapshot
Quasi-stationary corotating structure in the interplanetary medium
inferredcites →https://doi.org/10.1086/149138openalex-snapshot
The Angular Momentum of the Solar Wind
inferredcites →https://doi.org/10.1103/physrevlett.13.461openalex-snapshot
Solar Origin of the Interplanetary Magnetic Field
inferredcites →https://doi.org/10.1146/annurev.aa.05.090167.001241openalex-snapshot
Structure of the Solar Corona
What points at this work
Incoming claims: where this work appears in other papers’ reference lists and arguments.
inferred← citeshttps://doi.org/10.1002/2013ja018991openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2013ja019412openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2013ja019464openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2013ja019478openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2013sw000989openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2014gl059391openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2014ja020000openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2014ja020256openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2015ja021022openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2015ja021194openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2015ja021757openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2015ja021853openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2015ja021941openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2015sw001174openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2015sw001232openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2015sw001308openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2016ja022433openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2016ja022750openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2016sw001481openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/2017sw001671openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/9781119815600.ch3openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/asna.201111621openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/ctpp.202400017openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/essoar.10501416.1openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/jgra.50223openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/jgra.50259openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/jgra.50772openalex-snapshot
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inferred← citeshttps://doi.org/10.1002/swe.20094openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/3-540-09417-2_4openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/3-540-27510-x_2openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-0-387-09649-0_19openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-0-387-45088-9_2openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-0-387-69532-7_15openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-0-387-69532-7_6openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-0-387-98154-3_5openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-1-4419-0239-9_19openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-1-4419-0247-4_8openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-1-4614-1493-3_2openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-1-4939-2038-9_28openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-1-4939-2038-9_3openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-1-4939-2038-9_7openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-1-4939-2584-1_11openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-1-4939-3547-5_8openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-3-031-11870-8_7openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-3-031-58177-9_3openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-3-031-58177-9_5openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-3-540-74302-6_4openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-3-642-27543-2_4openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-3-642-65414-5_5openalex-snapshot
High-Speed Plasma Streams and Magnetic Sectors
inferred← citeshttps://doi.org/10.1007/978-3-642-65629-3_1openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-3-642-75361-9_2openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-3-642-75361-9_4openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-3-662-03653-2_8openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-94-009-1782-8_3openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-94-009-3693-5_11openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-94-009-3693-5_18openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-94-009-3693-5_3openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-94-009-4612-5_1openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-94-009-4612-5_30openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-94-009-4612-5_31openalex-snapshot
The Large-Scale Structure of the Heliospheric Magnetic Field
inferred← citeshttps://doi.org/10.1007/978-94-009-8479-0_27openalex-snapshot
Photospheric Magnetic Field Patterns and Their Coronal and Interplanetary Consequences
inferred← citeshttps://doi.org/10.1007/978-94-009-9100-2_1openalex-snapshot
Evolution of Coronal and Interplanetary Magnetic Fields
inferred← citeshttps://doi.org/10.1007/978-94-009-9100-2_11openalex-snapshot
The Origin of Interplanetary Sectors
inferred← citeshttps://doi.org/10.1007/978-94-010-0983-6_5openalex-snapshot
Interplanetary Magnetic Field Dynamics
inferred← citeshttps://doi.org/10.1007/978-94-010-1279-9_8openalex-snapshot
The Three-Dimensional Structure of the Interplanetary Medium
inferred← citeshttps://doi.org/10.1007/978-94-010-1481-6_7openalex-snapshot
Small-Scale Solar Magnetic Fields
inferred← citeshttps://doi.org/10.1007/978-94-010-2257-6_1openalex-snapshot
Magnetic Structure Responsible for Coronal Disturbances: Observations
inferred← citeshttps://doi.org/10.1007/978-94-010-2257-6_2openalex-snapshot
Magnetic Structure Responsible for Coronal Disturbances: Theory
inferred← citeshttps://doi.org/10.1007/978-94-010-2257-6_6openalex-snapshot
Boundary Fitting Problems Associated with Coronal Magnetic Models
inferred← citeshttps://doi.org/10.1007/978-94-010-3117-2_70openalex-snapshot
Large Scale Solar Magnetic Fields and Their Consequences
inferred← citeshttps://doi.org/10.1007/978-94-010-3117-2_74openalex-snapshot
The Magnetic Field Structure in the Active Solar Corona
inferred← citeshttps://doi.org/10.1007/978-94-010-3117-2_82openalex-snapshot
The Polar Fields and Time Fluctuations of the General Magnetic Field of the Sun
inferred← citeshttps://doi.org/10.1007/978-94-010-3117-2_88openalex-snapshot
Sector Structure of the Solar Magnetic Field
inferred← citeshttps://doi.org/10.1007/978-94-010-3128-8_5openalex-snapshot
Low-Energy Cosmic Rays in Interplanetary Space
inferred← citeshttps://doi.org/10.1007/978-94-010-3278-0_10openalex-snapshot
Magnetic Field Variations in Interplanetary Space
inferred← citeshttps://doi.org/10.1007/978-94-010-9376-7_66openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-94-010-9636-2_3openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-94-011-0167-7_25openalex-snapshot
The Large-Scale Structure of the Heliospheric Current Sheet during the Ulysses Epoch
inferred← citeshttps://doi.org/10.1007/978-94-011-0167-7_26openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-94-011-0167-7_32openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-94-011-0167-7_33openalex-snapshot
Latitude and Solar-Cycle Dependence of Radial IMF Intensity
inferred← citeshttps://doi.org/10.1007/978-94-011-5236-5_36openalex-snapshot
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inferred← citeshttps://doi.org/10.1007/978-94-017-1179-1_11openalex-snapshot
The Solar Origin of Corotating Interaction Regions and their Formation in the Inner Heliosphere
inferred← citeshttps://doi.org/10.1007/978-94-017-1179-1_13openalex-snapshot
Corotating Interaction Regions at High Latitudes
inferred← citeshttps://doi.org/10.1007/978-94-017-3230-7_13openalex-snapshot
Global Solar Wind Structure from Solar Minimum to Solar Maximum: Sources and Evolution
inferred← citeshttps://doi.org/10.1007/978-94-017-3230-7_27openalex-snapshot
A Model of the Magnetic Field Long-Term Evolution at the Coronal Base and Polar Heliospheric Regions
inferred← citeshttps://doi.org/10.1007/978-94-024-1521-6_9openalex-snapshot
Coronal Magnetic Field Models
inferred← citeshttps://doi.org/10.1007/978-94-024-1570-4_7openalex-snapshot
Deflection and Rotation of CMEs from Active Region 11158
inferred← citeshttps://doi.org/10.1007/978-94-024-1588-9_3openalex-snapshot
Origins of the Ambient Solar Wind: Implications for Space Weather
inferred← citeshttps://doi.org/10.1007/978-981-13-9081-4_1openalex-snapshot
Current Status of MHD Simulations for Space Weather
inferred← citeshttps://doi.org/10.1007/978-981-13-9081-4_4openalex-snapshot
3D SIP-CESE MHD Model on Triangular Prism Grids
inferred← citeshttps://doi.org/10.1007/978-981-16-1030-1_2openalex-snapshot
1D Model with Compressional and Non-compressional Nonlinear Effects
inferred← citeshttps://doi.org/10.1007/978-981-96-6707-9_8openalex-snapshot
Investigating Coronal Loop Dynamics: Harmonic Behavior and Magnetic Field Estimation
inferred← citeshttps://doi.org/10.1007/bf00145734openalex-snapshot
Magnetic fields and the structure of the solar corona
inferred← citeshttps://doi.org/10.1007/bf00146182openalex-snapshot
The effect of newly erupting flux on the polar coronal holes
inferred← citeshttps://doi.org/10.1007/bf00146241openalex-snapshot
Open magnetic fields and the solar cycle
inferred← citeshttps://doi.org/10.1007/bf00147253openalex-snapshot
Mechanisms for the rigid rotation of coronal holes
inferred← citeshttps://doi.org/10.1007/bf00147832openalex-snapshot
The determination of coronal potential magnetic fields using line-of-sight boundary conditions
inferred← citeshttps://doi.org/10.1007/bf00148028openalex-snapshot
On acceleration and motion of ions in corona and solar wind
inferred← citeshttps://doi.org/10.1007/bf00148029openalex-snapshot
Evidence for a coronal magnetic bottle at 10 solar radii
inferred← citeshttps://doi.org/10.1007/bf00148521openalex-snapshot
On the uniqueness of the determination of the coronal potential magnetic field from line-of-sight boundary conditions
inferred← citeshttps://doi.org/10.1007/bf00148838openalex-snapshot
Active solar radio regions at metric frequencies and the interplanetary sector structures
inferred← citeshttps://doi.org/10.1007/bf00149468openalex-snapshot
Comparison of the mean photospheric magnetic field and the interplanetary magnetic field
inferred← citeshttps://doi.org/10.1007/bf00149469openalex-snapshot
Magnetic fields and the structure of the solar corona
inferred← citeshttps://doi.org/10.1007/bf00149473openalex-snapshot
Unified theory of the interplanetary magnetic field
inferred← citeshttps://doi.org/10.1007/bf00149692openalex-snapshot
Solar noise storms and magnetic sector structures
inferred← citeshttps://doi.org/10.1007/bf00149859openalex-snapshot
Coronal holes as sources of solar wind
inferred← citeshttps://doi.org/10.1007/bf00150142openalex-snapshot
Motion of solar cosmic rays in the coronal magnetic field
inferred← citeshttps://doi.org/10.1007/bf00151551openalex-snapshot
Green corona and solar sector structure
inferred← citeshttps://doi.org/10.1007/bf00151752openalex-snapshot
Magnetic field configurations associated with fast solar wind
inferred← citeshttps://doi.org/10.1007/bf00151854openalex-snapshot
A ?source surface theory? corollary: The mean solar field-interplanetary field correlation
inferred← citeshttps://doi.org/10.1007/bf00152023openalex-snapshot
Polarity neutral lines on the solar surface and magnetic structures in the corona
inferred← citeshttps://doi.org/10.1007/bf00152078openalex-snapshot
Radial variation of differential rotation in the solar electron corona
inferred← citeshttps://doi.org/10.1007/bf00152320openalex-snapshot
Flare-produced coronal MHD-fast-mode wavefronts and Moreton's wave phenomenon
inferred← citeshttps://doi.org/10.1007/bf00152334openalex-snapshot
Coronal magnetic-field model with non-spherical source surface
inferred← citeshttps://doi.org/10.1007/bf00152591openalex-snapshot
Large-scale three-dimensional structure of the interplanetary magnetic field
inferred← citeshttps://doi.org/10.1007/bf00153050openalex-snapshot
The structure of the white-light corona and the large-scale solar magnetic field
inferred← citeshttps://doi.org/10.1007/bf00153379openalex-snapshot
�tude hydrodynamique du grand jet coronal ne observ� � l'�clipse du 7 Mars 1970
inferred← citeshttps://doi.org/10.1007/bf00154048openalex-snapshot
The relationship between the interplanetary magnetic field inhomogeneous structure and the distribution of large-scale magnetic fields in the photosphere (1969?1975)
inferred← citeshttps://doi.org/10.1007/bf00154071openalex-snapshot
On the correlation of coronal green-line intensity and solar wind velocity
inferred← citeshttps://doi.org/10.1007/bf00154277openalex-snapshot
The coronal and interplanetary magnetic fields at the time of the solar eclipse of 7 March, 1970
inferred← citeshttps://doi.org/10.1007/bf00154967openalex-snapshot
The large-scale solar magnetic field
inferred← citeshttps://doi.org/10.1007/bf00155703openalex-snapshot
Direct solution of laplace's equation for coronal magnetic fields using line-of-sight boundary conditions
inferred← citeshttps://doi.org/10.1007/bf00156118openalex-snapshot
Simulation of the magnetic structure of the inner heliosphere by means of a non-spherical source surface
inferred← citeshttps://doi.org/10.1007/bf00156388openalex-snapshot
An atlas of photospheric magnetic field observations and computed coronal magnetic fields: 1976?1985
inferred← citeshttps://doi.org/10.1007/bf00156963openalex-snapshot
The quiet corona: Temperature and temperature gradient
inferred← citeshttps://doi.org/10.1007/bf00157566openalex-snapshot
A new technique for the determination of coronal magnetic fields: A fixed mesh solution to Laplace's equation using line-of-sight boundary conditions
inferred← citeshttps://doi.org/10.1007/bf00157852openalex-snapshot
A model combining the polar and the sector structured solar magnetic fields
inferred← citeshttps://doi.org/10.1007/bf00159933openalex-snapshot
A sheet-current approach to coronal-interplanetary modeling
inferred← citeshttps://doi.org/10.1007/bf00162392openalex-snapshot
Solar-interplanetary modeling: 3-D solar wind solutions in prescribed non-radial magnetic field geometries
inferred← citeshttps://doi.org/10.1007/bf00165455openalex-snapshot
Potential field extrapolation using three components of a solar vector magnetogram with a finite field of view
inferred← citeshttps://doi.org/10.1007/bf00167401openalex-snapshot
The mean coronal magnetic field determined from HELIOS Faraday rotation measurements
inferred← citeshttps://doi.org/10.1007/bf00167404openalex-snapshot
Radio mapping of the heliospheric current sheet
inferred← citeshttps://doi.org/10.1007/bf00170987openalex-snapshot
Magnetostatic atmospheres: A family of isothermal solutions
inferred← citeshttps://doi.org/10.1007/bf00216372openalex-snapshot
High resolution mapping of the magnetic field of the solar corona
inferred← citeshttps://doi.org/10.1007/bf00619095openalex-snapshot
Unique determination of model coronal magnetic fields using photospheric observations
inferred← citeshttps://doi.org/10.1007/bf00627591openalex-snapshot
Coronal force-free magnetic field: Source-surface model
inferred← citeshttps://doi.org/10.1007/bf00627602openalex-snapshot
Comparison of single-site interplanetary scintillation solar wind speed structure with coronal features
inferred← citeshttps://doi.org/10.1007/bf00642204openalex-snapshot
The propagation of Alfv�n waves and their directional anisotropy in the solar wind
inferred← citeshttps://doi.org/10.1007/bf00643885openalex-snapshot
Solution of one-fluid model equations with short range retarding magnetic forces for the quiet solar wind
inferred← citeshttps://doi.org/10.1007/bf00644040openalex-snapshot
Coronal hole flux tubes and the problem of relating interplanetary and solar features
inferred← citeshttps://doi.org/10.1007/bf00645623openalex-snapshot
Spatial dependence of the pitch-angle and associated spatial diffusion coefficients for cosmic rays in interplanetary space
inferred← citeshttps://doi.org/10.1007/bf00646187openalex-snapshot
A model of the solar atmosphere and wind
inferred← citeshttps://doi.org/10.1007/bf00654084openalex-snapshot
A coronal magnetic field model with horizontal volume and sheet currents
inferred← citeshttps://doi.org/10.1007/bf00712514openalex-snapshot
Solar wind speed and its acceleration inferred using the interplanetary scintillation method in carrington rotation 1753
inferred← citeshttps://doi.org/10.1007/bf00732811openalex-snapshot
Solar flare activity and the structure of the coronal neutral line
inferred← citeshttps://doi.org/10.1007/bf00733033openalex-snapshot
A simple method to compute spherical harmonic coefficients for the potential model of the coronal magnetic field
inferred← citeshttps://doi.org/10.1007/bf00768770openalex-snapshot
The large-scale structure of the heliospheric current sheet during the Ulysses epoch
inferred← citeshttps://doi.org/10.1007/bf00768771openalex-snapshot
Fourier parameters of heliospheric current sheet and their significance
inferred← citeshttps://doi.org/10.1007/bf00768777openalex-snapshot
Modeling the out-of-ecliptic interplanetary magnetic field in the declining phase of sunspot Cycle 22
inferred← citeshttps://doi.org/10.1007/bf00768778openalex-snapshot
Latitude and solar-cycle dependence of radial IMF intensity
inferred← citeshttps://doi.org/10.1007/bf00963948openalex-snapshot
Magnetic fields and the solar corona
inferred← citeshttps://doi.org/10.1007/bf02276573openalex-snapshot
Interpretation of type I- and IV mB-bursts and noise storms by mode coupling in the warm plasma
inferred← citeshttps://doi.org/10.1007/bf02848200openalex-snapshot
A phenomenological, kinematical model of the coronal magnetic fields in terms of thin flux tubes rising from the photosphere
inferred← citeshttps://doi.org/10.1007/lrsp-2015-5openalex-snapshot
Solar Magnetism in the Polar Regions
inferred← citeshttps://doi.org/10.1007/s00159-014-0078-7openalex-snapshot
The magnetic field in the solar atmosphere
inferred← citeshttps://doi.org/10.1007/s00585-997-1379-1openalex-snapshot
Non-spherical source-surface model of the heliosphere: a scalar formulation
inferred← citeshttps://doi.org/10.1007/s10509-015-2639-2openalex-snapshot
Kelvin–Helmholtz instability in an active region jet observed with Hinode
inferred← citeshttps://doi.org/10.1007/s10509-026-04639-4openalex-snapshot
Closed-field electron acceleration in the solar corona: insights from J- and U-type solar radio bursts
inferred← citeshttps://doi.org/10.1007/s11207-005-2759-xopenalex-snapshot
Comparative Analyses of the CSSS Calculation in the UCSD Tomographic Solar Observations
inferred← citeshttps://doi.org/10.1007/s11207-005-3304-7openalex-snapshot
Correlation between Expansion Rate of the Coronal Magnetic Field and Solar Wind Speed in a Solar Activity Cycle
inferred← citeshttps://doi.org/10.1007/s11207-005-4280-7openalex-snapshot
Polar Coronal Structures and the Global Magnetic Field Evolution Through the Cycle
inferred← citeshttps://doi.org/10.1007/s11207-005-4982-xopenalex-snapshot
The Sun’s Large-Scale Magnetic Field and Its Long-Term Evolution
inferred← citeshttps://doi.org/10.1007/s11207-006-0266-3openalex-snapshot
Computing Nonlinear Force-Free Coronal Magnetic Fields in Spherical Geometry
inferred← citeshttps://doi.org/10.1007/s11207-007-9026-2openalex-snapshot
Principal Components and Independent Component Analysis of Solar and Space Data
inferred← citeshttps://doi.org/10.1007/s11207-007-9030-6openalex-snapshot
The Magnetic Field of the Solar Corona from Pulsar Observations
inferred← citeshttps://doi.org/10.1007/s11207-007-9097-0openalex-snapshot
Modelling the Global Solar Corona II: Coronal Evolution and Filament Chirality Comparison
inferred← citeshttps://doi.org/10.1007/s11207-008-9280-yopenalex-snapshot
The Solar Wind at 1 AU During the Declining Phase of Solar Cycle 23: Comparison of 3D Numerical Model Results with Observations
inferred← citeshttps://doi.org/10.1007/s11207-009-9345-6openalex-snapshot
Effects of the Weak Polar Fields of Solar Cycle 23: Investigation Using OMNI for the STEREO Mission Period
inferred← citeshttps://doi.org/10.1007/s11207-010-9556-xopenalex-snapshot
Organization of Energetic Particles by the Solar Wind Structure During the Declining to Minimum Phase of Solar Cycle 23
inferred← citeshttps://doi.org/10.1007/s11207-010-9586-4openalex-snapshot
Multiwavelength Study of the M8.9/3B Solar Flare from AR NOAA 10960
inferred← citeshttps://doi.org/10.1007/s11207-010-9599-zopenalex-snapshot
Transient Structures and Stream Interaction Regions in the Solar Wind: Results from EISCAT Interplanetary Scintillation, STEREO HI and Venus Express ASPERA-4 Measurements
inferred← citeshttps://doi.org/10.1007/s11207-010-9687-0openalex-snapshot
Nonlinear Force-Free and Potential-Field Models of Active-Region and Global Coronal Fields during the Whole Heliosphere Interval
inferred← citeshttps://doi.org/10.1007/s11207-010-9699-9openalex-snapshot
Coronal Field Opens at Lower Height During the Solar Cycles 22 and 23 Minimum Periods: IMF Comparison Suggests the Source Surface Should Be Lowered
inferred← citeshttps://doi.org/10.1007/s11207-011-9713-xopenalex-snapshot
Nonlinear Force-Free Reconstruction of the Global Solar Magnetic Field: Methodology
inferred← citeshttps://doi.org/10.1007/s11207-011-9737-2openalex-snapshot
Comparing Solar Minimum 23/24 with Historical Solar Wind Records at 1 AU
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