Cargando…
CME–HSS Interaction and Characteristics Tracked from Sun to Earth
In a thorough study, we investigate the origin of a remarkable plasma and magnetic field configuration observed in situ on June 22, 2011, near L1, which appears to be a magnetic ejecta (ME) and a shock signature engulfed by a solar wind high-speed stream (HSS). We identify the signatures as an Earth...
Autores principales: | Heinemann, Stephan G., Temmer, Manuela, Farrugia, Charles J., Dissauer, Karin, Kay, Christina, Wiegelmann, Thomas, Dumbović, Mateja, Veronig, Astrid M., Podladchikova, Tatiana, Hofmeister, Stefan J., Lugaz, Noé, Carcaboso, Fernando |
---|---|
Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Springer Netherlands
2019
|
Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6936343/ https://www.ncbi.nlm.nih.gov/pubmed/31929659 http://dx.doi.org/10.1007/s11207-019-1515-6 |
Ejemplares similares
-
On Flare-CME Characteristics from Sun to Earth Combining Remote-Sensing Image Data with In Situ Measurements Supported by Modeling
por: Temmer, Manuela, et al.
Publicado: (2017) -
Earth-affecting solar transients: a review of progresses in solar cycle 24
por: Zhang, Jie, et al.
Publicado: (2021) -
The Dependence of the Peak Velocity of High‐Speed Solar Wind Streams as Measured in the Ecliptic by ACE and the STEREO satellites on the Area and Co‐latitude of Their Solar Source Coronal Holes
por: Hofmeister, Stefan J., et al.
Publicado: (2018) -
Earth's magnetosphere and outer radiation belt under sub-Alfvénic solar wind
por: Lugaz, Noé, et al.
Publicado: (2016) -
Strong coronal channelling and interplanetary evolution of a solar storm up to Earth and Mars
por: Möstl, Christian, et al.
Publicado: (2015)