Science Results from the Dual Van Allen Probes Mission

Event Details
Event Date
Speaker Name/Affiliation
Dan Baker / LASP, University of Colorado Boulder
Seminar Type/Subject
Event Details & Abstracts

A principal goal of the Radiation Belt Storm Probes (RBSP) mission was to develop a much deeper understanding of the structure and dynamics of Earth’s radiation belts. Almost immediately after the late-August 2012 launch of the twin RBSP spacecraft into their highly elliptical orbits, it was discovered that a third Van Allen belt (or “storage ring”) of highly relativistic electrons can exist near the inner part of the traditionally recognized outer Van Allen zone. This feature has been the subject of much theoretical investigation and speculation since its discovery. There also has been detected an “impenetrable” barrier at L~2.8 inside of which high-energy electrons have not diffused in over seven years of observations. In addition to morphological structures of the radiation zones such as the storage ring and barrier, it has also been a major achievement of the RBSP program (renamed the “Van Allen Probes” mission in November 2012) to understand more thoroughly how ultra-relativistic electrons are accelerated deep inside the radiation belts due to various wave-particle interactions. Van Allen Probes studies have demonstrated that electrons up to energies over 10 megaelectron volts (MeV) can be produced over broad regions of the outer Van Allen zone on timescales of minutes to a few hours. The key to such rapid acceleration is the interaction of “seed” populations of ~10 to ~200 keV electrons (and subsequently higher energies) with electromagnetic waves in the lower band whistler-mode chorus frequency range. In this presentation, we report observations of some of the largest geomagnetic storms of the last several years. We show long-term observations through animations that demonstrate dramatic effects on the relativistic and ultra-relativistic electrons measured by sensors on board the Van Allen Probes spacecraft. This talk also describes high-energy proton features in the inner radiation belt and demonstrates new features for the highest energy particles in the inner Van Allen zone.