Articles | Volume 36, issue 4
https://doi.org/10.5194/angeo-36-1081-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/angeo-36-1081-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Regular paper
| 
08 Aug 2018
Regular paper |
| 08 Aug 2018
| 08 Aug 2018
Cavitons and spontaneous hot flow anomalies in a hybrid-Vlasov global magnetospheric simulation
Xochitl Blanco-Cano
CORRESPONDING AUTHOR
Instituto de Geofisica, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico
Markus Battarbee
Department of Physics, University of Helsinki, Helsinki, Finland
Lucile Turc
Department of Physics, University of Helsinki, Helsinki, Finland
Andrew P. Dimmock
Swedish Institute of Space Physics, Uppsala, Sweden
Department of Electronics and Nanoengineering, School of Electrical Engineering, Aalto University, Espoo, Finland
Emilia K. J. Kilpua
Department of Physics, University of Helsinki, Helsinki, Finland
Sanni Hoilijoki
Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, USA
Urs Ganse
Department of Physics, University of Helsinki, Helsinki, Finland
David G. Sibeck
NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
Paul A. Cassak
Department of Physics and Astronomy, West Virginia University, Morgantown, West Virginia, USA
Robert C. Fear
Department of Physics and Astronomy, University of Southampton, Southampton, UK
Riku Jarvinen
Department of Electronics and Nanoengineering, School of Electrical Engineering, Aalto University, Espoo, Finland
Finnish Meteorological Institute, Helsinki, Finland
Liisa Juusola
Finnish Meteorological Institute, Helsinki, Finland
Department of Physics, University of Helsinki, Helsinki, Finland
Yann Pfau-Kempf
Department of Physics, University of Helsinki, Helsinki, Finland
Rami Vainio
Department of Physics and Astronomy, University of Turku, Turku, Finland
Minna Palmroth
Department of Physics, University of Helsinki, Helsinki, Finland
Finnish Meteorological Institute, Helsinki, Finland
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Cited
13 citations as recorded by crossref.
- HYPERS simulations of solar wind interactions with the Earth's magnetosphere and the Moon Y. Omelchenko et al. 10.1016/j.jastp.2021.105581
- Dayside Transient Phenomena and Their Impact on the Magnetosphere and Ionosphere H. Zhang et al. 10.1007/s11214-021-00865-0
- Transmission of foreshock waves through Earth’s bow shock L. Turc et al. 10.1038/s41567-022-01837-z
- Energy Flux Through the Magnetopause During Flux Transfer Events in Hybrid‐Vlasov 2D Simulations M. Ala‐Lahti et al. 10.1029/2022GL100079
- What are the fundamental modes of energy transfer and partitioning in the coupled Magnetosphere-Ionosphere system? J. Rae et al. 10.1007/s10686-022-09861-w
- Helium in the Earth's foreshock: a global Vlasiator survey M. Battarbee et al. 10.5194/angeo-38-1081-2020
- Resolution dependence of magnetosheath waves in global hybrid-Vlasov simulations M. Dubart et al. 10.5194/angeo-38-1283-2020
- Motion of Classic and Spontaneous Hot Flow Anomalies Observed by Cluster X. Zhu et al. 10.1029/2021JA029418
- Foreshock cavitons and spontaneous hot flow anomalies: a statistical study with a global hybrid-Vlasov simulation V. Tarvus et al. 10.5194/angeo-39-911-2021
- Bursty magnetic reconnection at the Earth's magnetopause triggered by high-speed jets J. Ng et al. 10.1063/5.0054394
- Comment on “Cavitons and spontaneous hot flow anomalies in a hybrid-Vlasov global magnetospheric simulation” by Blanco-Cano et al. (2018) G. Facskó 10.5194/angeo-37-763-2019
- Non-locality of Earth's quasi-parallel bow shock: injection of thermal protons in a hybrid-Vlasov simulation M. Battarbee et al. 10.5194/angeo-38-625-2020
- Properties of Magnetic Reconnection and FTEs on the Dayside Magnetopause With and Without Positive IMF Bx Component During Southward IMF S. Hoilijoki et al. 10.1029/2019JA026821
12 citations as recorded by crossref.
- HYPERS simulations of solar wind interactions with the Earth's magnetosphere and the Moon Y. Omelchenko et al. 10.1016/j.jastp.2021.105581
- Dayside Transient Phenomena and Their Impact on the Magnetosphere and Ionosphere H. Zhang et al. 10.1007/s11214-021-00865-0
- Transmission of foreshock waves through Earth’s bow shock L. Turc et al. 10.1038/s41567-022-01837-z
- Energy Flux Through the Magnetopause During Flux Transfer Events in Hybrid‐Vlasov 2D Simulations M. Ala‐Lahti et al. 10.1029/2022GL100079
- What are the fundamental modes of energy transfer and partitioning in the coupled Magnetosphere-Ionosphere system? J. Rae et al. 10.1007/s10686-022-09861-w
- Helium in the Earth's foreshock: a global Vlasiator survey M. Battarbee et al. 10.5194/angeo-38-1081-2020
- Resolution dependence of magnetosheath waves in global hybrid-Vlasov simulations M. Dubart et al. 10.5194/angeo-38-1283-2020
- Motion of Classic and Spontaneous Hot Flow Anomalies Observed by Cluster X. Zhu et al. 10.1029/2021JA029418
- Foreshock cavitons and spontaneous hot flow anomalies: a statistical study with a global hybrid-Vlasov simulation V. Tarvus et al. 10.5194/angeo-39-911-2021
- Bursty magnetic reconnection at the Earth's magnetopause triggered by high-speed jets J. Ng et al. 10.1063/5.0054394
- Comment on “Cavitons and spontaneous hot flow anomalies in a hybrid-Vlasov global magnetospheric simulation” by Blanco-Cano et al. (2018) G. Facskó 10.5194/angeo-37-763-2019
- Non-locality of Earth's quasi-parallel bow shock: injection of thermal protons in a hybrid-Vlasov simulation M. Battarbee et al. 10.5194/angeo-38-625-2020
Latest update: 19 Apr 2024
Short summary
We use the Vlasiator code to study the characteristics of transient structures that exist in the Earth's foreshock, i.e. upstream of the bow shock. The structures are cavitons and spontaneous hot flow anomalies (SHFAs). These transients can interact with the bow shock. We study the changes the shock suffers via this interaction. We also investigate ion distributions associated with the cavitons and SHFAs. A very important result is that the arrival of multiple SHFAs results in shock erosion.
We use the Vlasiator code to study the characteristics of transient structures that exist in the...
