Source and seed populations for relativistic electrons: Their roles in radiation belt changes

By A. Jaynes, D. N. Baker, H. Singer, Juan V. Rodriguez, T. M. Loto'aniu, A. Ali, S. Elkington, Xinlin Li, S. Kanekal, Seth G. Claudepierre and 6 more. 2015

280 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/2d539c9c52121f1e976fa9e42af2b3087201c1e3

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Wen Li
2. S. Gibson
3. M. Hudson
4. Xinlin Li
5. J. Fennell
6. Pete Riley
7. D. N. Baker
8. S. Cranmer

In Geophysics

1. M. Hudson
2. Wen Li
3. J. Fennell
4. A. Jaynes
5. J. Foster
6. D. N. Baker
7. C. Crabtree
8. Xinlin Li

Citations in the corpus

• The Challenge of Machine Learning in Space Weather: Nowcasting and Forecasting (2019, background): “As highlighted in Jaynes et al. (2015), a simple causal relationship between a fast solar wind driver and the enhancement of radiation belt electron fluxes might miss the rare occurrences when high-speed solar wind streams do not produce flux enhancements, if the two distinct population of…”
• Space Weather Effects in the Earth’s Radiation Belts (2018, methodology): “…in the core of the outer zone of the radiation belt involves the local acceleration (Horne and Thorne 1998; Reeves et al. 2013; Thorne et al. 2013a; Summers et al. 1998) of a seed population of energetic electrons (e.g. Jaynes et al. 2015) in interactions with (very low frequency) VLF chorus waves.”
• Particle Dynamics in the Earth's Radiation Belts: Review of Current Research and Open Questions (2020, background): “…(hundreds of kiloelectron volts), which penetrates the outer belt and drifts inward, becoming in turn, accelerated to much higher energies (up to megaelectron volts) through VLF wave resonant interactions generated by the electron source population (e.g., Jaynes et al., 2015; Rodger et al., 2016).”
• Origins of the Ambient Solar Wind: Implications for Space Weather (2017, background): “The primary impact of a fast stream appears to be the acceleration of additional energetic electrons in the radiation belts (e.g., Iles et al. 2002; Reeves et al. 2003; Jaynes et al. 2015; Kilpua et al. 2015).”
• Earth's Van Allen Radiation Belts: From Discovery to the Van Allen Probes Era (2019, background): “Realistic and dynamic seed electron populations are found to be critical for accurately modeling radiation belt electron dynamics (e.g., Boyd et al., 2014; Jaynes et al., 2015; Tu et al., 2014).”