Seasonal and Solar Wind Control of the Reconnection Line Location on the Earth's Dayside Magnetopause
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Y. Hoshi↗
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Microscale Processes Determining Macroscale Evolution of Magnetic Flux Tubes along Earth’s Magnetopause
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K.-J. Hwang↗
Reconnection layer bounded by switch‐off shocks: Dayside magnetopause crossing by THEMIS D
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Bengt Sonnerup↗
The Spatial Extent of Magnetopause Magnetic Reconnection From In Situ THEMIS Measurements
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Emil A. Atz↗
The permeability of the magnetopause to a multispecies substorm injection of energetic particles
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J. H. Westlake↗
Plasma Properties in the Earth's Magnetosheath Near the Subsolar Magnetopause: Implications for Geocoronal Density Estimates
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S. A. Fuselier↗
Investigating Potential Causes for the Prediction of Spurious Magnetopause Crossings at Geosynchronous Orbit in MHD Simulations
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Pauline M. Dredger↗
Observations of energetic particle escape at the magnetopause: Early results from the MMS Energetic Ion Spectrometer (EIS)
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I. J. Cohen↗
On the occurrence of magnetic reconnection equatorward of the cusps at the Earth's magnetopause during northward IMF conditions
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K. J. Trattner↗
Evolution of a Foreshock Bubble in the Midtail Foreshock and Impact on the Magnetopause: 3‐D Global Hybrid Simulation
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Chih‐Ping Wang↗
Electron Trapping in Magnetic Mirror Structures at the Edge of Magnetopause Flux Ropes
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S. L. Robertson↗
The Cold Ion Population at Geosynchronous Orbit and Transport to the Dayside Magnetopause: September 2015 to February 2016
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M. H. Denton↗
Investigating the Link Between Outer Radiation Belt Losses and Energetic Electron Escape at the Magnetopause: A Case Study Using Multi‐Mission Observations and Simulations
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I. J. Cohen↗
Geospace Plume and Its Impact on Dayside Magnetopause Reconnection Rate
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Ying Zou↗
Long and Active Magnetopause Reconnection X‐Lines During Changing IMF Conditions
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K. J. Trattner↗
Ion demagnetization in the magnetopause current layer observed by MMS
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Shan Wang↗
The influence of the magnetopause on cosmic ray particle trajectories.
Effects of deformed magnetic field on trajectories and asymptotic directions of arrival of medium energy cosmic rays at various stations, using spherical harmonics
COSMIC RAY PROPAGATION↗
Structure of the magnetopause at 6.6 R sub E in terms of 50- to 150-kev electrons.
Azimuthal sampling of electron flux on spinning satellite provide direction and magnitude of energetic electron space gradients at trapping magnetospheric boundaries
Lezniak, T. W.↗