Driven Alfven waves and electron acceleration: A FAST case study

By C. Chaston, John W. Bonnell, L. Peticolas, C. Carlson, J. Mcfadden, R. Ergun. 2002

142 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/6f2bf7a839e7ed295bff432ea7c92ae7d30074f2

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. T. Van Doorsselaere
2. Valery M. Nakariakov
3. Giuseppe Nisticò
4. J. Mcfadden
5. Petr Jelínek
6. John W. Bonnell
7. D. Kolotkov
8. H. Hudson

In Geophysics

1. T. Van Doorsselaere
2. John W. Bonnell
3. H. Hudson
4. Valery M. Nakariakov
5. J. Mcfadden
6. R. Strangeway

Citations in the corpus

• Properties of small‐scale Alfvén waves and accelerated electrons from FAST (2003, methodology): “This occurs as the wave partially reflects on the strong gradients in VA which further enhances the parallel wave field over the altitude range from 1 to 2 RE for the nightside case and at higher altitudes for the dayside case [Chaston et al., 2002].”
• Impulsive Phase Flare Energy Transport by Large-Scale Alfvén Waves and the Electron Acceleration Problem (2007, methodology): “Chaston et al. (2002) have demonstrated that the value of the energy flux carried by auroral electrons is similar to the Poynting flux of low-frequency Alfvén oscillations of the magnetospheric field.”
• Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding (2016, background): “For example, kinetic small-scale Alfvénic structures can carry a very localised, but intense, field-aligned electric field, resulting in a downward acceleration of auroral electrons (Chaston et al. 2002a).”