Heliophysics Division, Planetary Sciences and Aeronomy, National Institute for Space Research (INPE), São José dos Campos, SP, 12227-010, Brazil
Márcio E. S. Alves
Universidade Estadual Paulista (UNESP), Instituto de Ciência e Tecnologia, São José dos Campos, SP, 12247-004, Brazil
now at: Universidade Estadual Paulista (UNESP), Faculdade de Engenharia e Ciências de Guaratinguetá, Departamento de Física e Química, Guaratinguetá, SP, 12516-410, Brazil
Ligia A. da Silva
Heliophysics Division, Planetary Sciences and Aeronomy, National Institute for Space Research (INPE), São José dos Campos, SP, 12227-010, Brazil
State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, São José dos Campos, SP, Brazil
Vinicius Deggeroni
Heliophysics Division, Planetary Sciences and Aeronomy, National Institute for Space Research (INPE), São José dos Campos, SP, 12227-010, Brazil
Paulo R. Jauer
Heliophysics Division, Planetary Sciences and Aeronomy, National Institute for Space Research (INPE), São José dos Campos, SP, 12227-010, Brazil
State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, São José dos Campos, SP, Brazil
David G. Sibeck
NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
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Total article views: 3,391 (including HTML, PDF, and XML)
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We derive the wave–particle interaction time (IT) equation considering the effects of special relativity theory for whistler-mode chorus waves and relativistic electrons in Earth's radiation belt. Results show that IT has a non-linear dependence on the wave group velocity, electrons' energy, and initial pitch angle. Our results show that the interaction time is generally longer when applying the complete relativistic approach compared to a non-relativistic calculation.
We derive the wave–particle interaction time (IT) equation considering the effects of special...
