Roger R. Anderson

TL;DR: In this paper, an empirical model of equatorial electron density in the magnetosphere covering the L range 2.25-8.9043 was presented for application to the local time interval 00-15 MLT, and a way to extend the model to the 15-24 MLT period is presented.

TL;DR: In this paper, the authors present CRRES data on the spatial distribution of chorus emissions during active conditions and calculate the pitch angle and energy diffusion rates in three magnetic local time (MLT) sectors and obtain a timescale for acceleration.

TL;DR: In this article, a survey of wave data from the CRRES Plasma Wave Experiment for lower band (0.1-0.5f(ce)) and upper band ( 0.5-1.0f(c)) chorus was presented to assess whether these waves could play an important role in the acceleration of a seed population of electrons to relativistic energies during and following geomagnetic storms.

TL;DR: In this article, a statistical analysis of over 800 EMIC wave events observed on the CRRES spacecraft is performed to establish whether scattering can occur at geophysically interesting energies (less than or equal to 2 MeV).

TL;DR: In this article, the authors used the combined Release and Radiation Effects Satellite (CRRES) sweep frequency receiver data to develop an empirical model of the plasmasphere and trough number density.