Evidence of Microbursts Observed Near the Equatorial Plane in the Outer Van Allen Radiation Belt
- Shumko, Mykhaylo [ Montana State University: Physics ] [ Space Science Applications Laboratory, The Aerospace Corporation, Los Angeles, CA ]
- Turner, Drew L. [ Space Science Applications Laboratory, The Aerospace Corporation, Los Angeles, CA ]
- O'Brien, T. P. [ Space Science Applications Laboratory, The Aerospace Corporation, Los Angeles, CA ]
- Claudepierre, Seth G. [ Space Science Applications Laboratory, The Aerospace Corporation, Los Angeles, CA ]
- Sample, John [ Montana State University: Physics ]
- Hartley, D. P. [ Department of Physics and Astronomy, The University of Iowa, Iowa City, IA ]
- Fennel, Joseph [ Space Science Applications Laboratory, The Aerospace Corporation, Los Angeles, CA ]
- Blake, J. Bernard [ Space Science Applications Laboratory, The Aerospace Corporation, Los Angeles, CA ]
- Gkioulidou, Matina [ Johns Hopkins University Applied Physics Laboratory, Laurel, MD ]
- Mitchell, Donald G. [ Johns Hopkins University Applied Physics Laboratory, Laurel, MD ]
We present the first evidence of electron microbursts observed near the equatorial plane in Earth's outer radiation belt. We observed the microbursts on 31 March 2017 with the Magnetic Electron Ion Spectrometer and Radiation Belt Storm Probes Ion Composition Experiment on the Van Allen Probes. Microburst electrons with kinetic energies of 29–92 keV were scattered over a substantial range of pitch angles, and over time intervals of 150–500 ms. Furthermore, the microbursts arrived without dispersion in energy, indicating that they were recently scattered near the spacecraft. We have applied the relativistic theory of waveâ€particle resonant diffusion to the calculated phase space density, revealing that the observed transport of microburst electrons is not consistent with the hypothesized quasiâ€linear approximation.