Cargando…
Ion‐driven instabilities in the solar wind: Wind observations of 19 March 2005
Intervals of enhanced magnetic fluctuations have been frequently observed in the solar wind. But it remains an open question as to whether these waves are generated at the Sun and then transported outward by the solar wind or generated locally in the interplanetary medium. Magnetic field and plasma...
Autores principales: | Gary, S. Peter, Jian, Lan K., Broiles, Thomas W., Stevens, Michael L., Podesta, John J., Kasper, Justin C. |
---|---|
Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
John Wiley and Sons Inc.
2016
|
Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5070513/ https://www.ncbi.nlm.nih.gov/pubmed/27818854 http://dx.doi.org/10.1002/2015JA021935 |
Ejemplares similares
-
Charge exchange in cometary coma: Discovery of H(−) ions in the solar wind close to comet 67P/Churyumov‐Gerasimenko
por: Burch, J. L., et al.
Publicado: (2015) -
Ion Acceleration at Solar Wind Termination Shock
por: Berezhko, E G
Publicado: (2005) -
Basics of the solar wind
por: Meyer-Vernet , Nicole
Publicado: (2007) -
Turbulence in the solar wind
por: Bruno, Roberto, et al.
Publicado: (2016) -
The evolution of the solar wind
por: Vidotto, Aline A.
Publicado: (2021)