Solar wind control of the tail lobe magnetic field as deduced from Geotail, AMPTE/IRM, and ISEE 2 data
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- Type
- article
- Published
- 2000-03-01
- Cited by
- 24
- References
- 32
- OpenAlex
- https://openalex.org/W2012687095
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:140667944
Keywords
Solar wind, Interplanetary magnetic field, Physics, Magnetometer, Magnetosphere
References
- Effects of the solar wind conditions on the global magnetospheric configuration as deduced from data-based field models
- The Low Energy Particle (LEP) Experiment onboard the GEOTAIL Satellite
- A magnetospheric magnetic field model with flexible current systems driven by independent physical parameters
- A magnetospheric magnetic field model with a warped tail current sheet
- An empirical relationship between interplanetary conditions and Dst
- The IRM Fluxgate Magnetometer
- Relation of the magnetic field in the magnetosphere to the geomagnetic and solar wind activity
- A large magnetosphere magnetic field database
- Magnetic field structures of the magnetotail as observed by GEOTAIL
- Outline of the Active Magnetospheric Particle Tracer Explorers (AMPTE) Mission
- Identification of high‐latitude acoustic gravity wave sources using the Goose Bay HF Radar
- Variability of the tail lobe field strength
- Influences of solar wind parameters and geomagnetic activity on the tail lobe magnetic field: A statistical study
- A quantitative magnetospheric model derived from spacecraft magnetometer data
- The relationship between interplanetary quantities and Birkeland current densities
- The Plasma Instrument for AMPTE IRM
- Interplanetary energy flux associated with magnetospheric substorms
- Determination of the magnetospheric current system parameters and development of experimental geomagnetic field models based on data from IMP and HEOS satellites
- Dst is not a pure ring-current index
- International Sun-Earth Explorer: A Three-Spacecraft Program
Cited by
- Statistical Characteristics of the Heliospheric Plasma and Magnetic Field at the Earth's Orbit during Four Solar Cycles 20-23
- The Fields of Magnetospheric Current Systems on the Earth's Surface in an Interval of the Magnetic Storm Studied under the International Program on Solar–Terrestrial Physics
- Further evidence for the role of magnetotail current shape in substorm initiation
- Ballooning stability of the Earth's magnetosphere
- Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms
- Magnetospheric configurations from a high-resolution data-based magnetic field model
- Energetics of the magnetosphere during the magnetic storm
- A model of the near magnetosphere with a dawn-dusk asymmetry 2. Parameterization and fitting to observations: A NEW MAGNETOSPHERE MAGNETIC FIELD MODEL, 2
- Role of solar wind dynamic pressure in driving ionospheric Joule heating
- Toward a global magnetospheric equilibrium model
- Statistical survey of magnetic and velocity fluctuations in the near-Earth plasma sheet: International Sun Earth Explorer (ISEE-2) measurements
- Lognormal form of the ring current energy content
- Algebra and statistics of the solar wind
- The Shape of Strongly Disturbed Dayside Magnetopause
- Quantitative magnetotail characteristics of different magnetospheric states
- Statistical study of the substorm onset: its dependence on solar wind parameters and solar illumination
- Assessing the performance of community‐available global MHD models using key system parameters and empirical relationships
- Statistical study on ultralow‐frequency waves in the magnetotail lobe observed by Cluster
- Statistical properties of substorm auroral onset beads/rays
- Anomalous dynamics of the extremely compressed magnetosphere during 21 January 2005 magnetic storm
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