High-speed solar wind with southward interplanetary magnetic field causes relativistic electron flux enhancement of the outer radiation belt via enhanced condition of whistler waves

Evolution of chorus waves and their source electrons during storms driven by corotating interaction regions

(2012) Wen Li et al.   JOURNAL OF GEOPHYSICAL RESEARCH

Science Objectives and Rationale for the Radiation Belt Storm Probes Mission

(2012) B. H. Mauk et al.   SPACE SCIENCE REVIEWS

Behavior of MeV electrons at geosynchronous orbit during last two solar cycles

(2011) X. Li et al.   JOURNAL OF GEOPHYSICAL RESEARCH

On the relationship between relativistic electron flux and solar wind velocity: Paulikas and Blake revisited

(2011) Geoffrey D. Reeves et al.   JOURNAL OF GEOPHYSICAL RESEARCH

Simultaneous satellite observations of VLF chorus, hot and relativistic electrons in a magnetic storm “recovery” phase

(2009) Y. Kasahara et al.   GEOPHYSICAL RESEARCH LETTERS

Superposed epoch analysis of a whistler instability criterion at geosynchronous orbit during geomagnetic storms

(2008) E.A. MacDonald et al.   JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS

Review of modeling of losses and sources of relativistic electrons in the outer radiation belt II: Local acceleration and loss

(2008) Yuri Y. Shprits et al.   JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS

Role of the Russell–McPherron effect in the acceleration of relativistic electrons

(2008) R.L. McPherron et al.   JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS

Flux enhancement of the outer radiation belt electrons after the arrival of stream interaction regions

(2008) Yoshizumi Miyoshi et al.   JOURNAL OF GEOPHYSICAL RESEARCH