1. Quasi‐Trapped Electron Fluxes Induced by NWC Transmitter and CRAND: Observations and Simulations.
- Author
-
Liu, Yangxizi, Xiang, Zheng, Ni, Binbin, Li, Xinlin, Zhang, Kun, Fu, Song, Gu, Xudong, Liu, Jiang, and Cao, Xing
- Subjects
- *
COSMIC rays , *ELECTRON distribution , *TRANSMITTERS (Communication) , *PROTON decay , *ELECTRONS , *ELECTRON sources - Abstract
Signals from the NWC ground‐based very low frequency (VLF) transmitter can leak into the magnetosphere and scatter trapped energetic electrons into drift loss cones. Recent studies also suggest that cosmic ray albedo neutron decay (CRAND) is probably an important source for quasi‐trapped electrons in the inner belt. To investigate their relative contributions, this study comprehensively analyzes the long‐term variations of quasi‐trapped 206 keV electrons at L = 1.7, which is roughly the L shell where NWC is located. Furthermore, a drift‐diffusion‐source model is used to reproduce longitudinal distributions of quasi‐trapped electrons and investigate sensitivities of simulation results to VLF transmitter intensities. These results suggest that CRAND is the main source of quasi‐trapped hundreds of keV electrons when the NWC station is at dayside. In contrast, pitch angle diffusions become the main source mechanism of these quasi‐trapped electrons when the NWC station operates at nightside with more VLF transmitter energy leaking into the magnetosphere. Plain Language Summary: Very low frequency (VLF) signals emitted from NWC transmitter locating at west Australia are used for submarine communications. The VLF signals propagate along the Earth‐ionosphere waveguide and a portion can leak into the magnetosphere. Low‐Earth orbit satellite observations demonstrate that the NWC transmitter signals in the magnetosphere can scatter trapped energetic electrons into the drift loss cone at L = 1.7, which is roughly of the L shell of the NWC location, resulting in the enhancement of approximately 200 keV quasi‐trapped electron fluxes. Cosmic ray albedo neutron decay (CRAND) describes the process that galaxy cosmic rays (the majority consist of high‐energy protons and helium nucleus) collide with atmosphere atoms and produce albedo neutrons, which have a mean lifetime of 887 s and then decay into protons, electrons, and antineutrinos, which is also considered as a source of >200 keV quasi‐trapped electrons in the inner belt. In this study, we compare the model results with DEMETER measurements and find that CRAND is the main source of quasi‐trapped hundreds of keV electrons when the NWC transmitter is at dayside. In contrast, the pitch angle diffusion induced by NWC transmitter signals becomes the main source mechanism of these quasi‐trapped electrons due to VLF signals leaking into the magnetosphere easily when the NWC transmitter operates at nightside. Key Points: CRAND is the main source of 200–700 keV quasi‐trapped electrons at L = 1.7 when NWC transmitter is at daysideFor quasi‐trapped 206 keV electrons at L = 1.7, pitch angle diffusion is the main source mechanism when NWC station operates at nightsideThe 〈Dαα〉 $\langle {D}_{\alpha \alpha }\rangle $ from NWC needs to be approximately 10−6 to 10−5 s−1 to reproduce the satellite observations of quasi‐trapped 206 keV electrons at L = 1.7 [ABSTRACT FROM AUTHOR]
- Published
- 2022
- Full Text
- View/download PDF