A Statistical Study of Quasi-trapped Electron Energy Spectrum: DEMETER Measurements
Abstract
Quasi-trapped electrons (pitch angle in DLC) in Earth's inner radiation belt are an important particle population whose behaviors help reveal the scattering effects of trapped electrons and quantify the intensity of electron precipitation. However, a detailed systematic characterization of quasi-trapped electron energy spectra in inner belt has not yet been investigated. Here we present a statistical study of quasi-trapped electron energy spectra based on 8-year DEMETER measurements. The electron energy spectral are classified into three categories: CRAND-produced, ROH (Raise-On-Head), and exponential-type. More than 95% of the energy spectra can be categorized as one of these three energy spectrum types, while 10.12% are CRAND energy spectra, 75.78% are ROH energy spectra, and 9.19% are exponential energy spectra. Through event analysis and statistical analysis of distributions of spectral types and characteristic parameters, we analyze the spatiotemporal evolution of quasi-trapped electrons in the inner radiation belt and investigate the source mechanisms of quasi-trapped electrons. The CRAND energy spectrum is predominantly distributed at L
Fields of Study & Subjects
Ionosphere and magnetosphere dynamics
Solar and Space Plasma Dynamics
Lightning and Electromagnetic Phenomena
Publication details
- Journal / source
- EGU General Assembly Conference Abstracts
- Publication date
- 14 March 2026
- Language
- EN