Articles | Volume 34, issue 11
https://doi.org/10.5194/angeo-34-943-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-34-943-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Regular paper
| 
04 Nov 2016
Regular paper |
| 04 Nov 2016
Evidence for transient, local ion foreshocks caused by dayside magnetopause reconnection
Earth Observation, Finnish Meteorological Institute, Helsinki, Finland
Department of Physics, University of Helsinki, Helsinki, Finland
Heli Hietala
Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, USA
Steve E. Milan
Department of Physics and Astronomy, University of Leicester, Leicester, UK
Liisa Juusola
Earth Observation, Finnish Meteorological Institute, Helsinki, Finland
Sanni Hoilijoki
Earth Observation, Finnish Meteorological Institute, Helsinki, Finland
Department of Physics, University of Helsinki, Helsinki, Finland
Urs Ganse
Department of Physics and Astronomy, University of Turku, Turku, Finland
Earth Observation, Finnish Meteorological Institute, Helsinki, Finland
Sebastian von Alfthan
CSC, IT Center for Science, Espoo, Finland
Minna Palmroth
Earth Observation, Finnish Meteorological Institute, Helsinki, Finland
Viewed
Total article views: 2,962 (including HTML, PDF, and XML)
Cumulative views and downloads
(calculated since 04 Nov 2016)
| HTML | XML | Total | Supplement | BibTeX | EndNote | |
|---|---|---|---|---|---|---|
| 2,039 | 797 | 126 | 2,962 | 232 | 99 | 92 |
- HTML: 2,039
- PDF: 797
- XML: 126
- Total: 2,962
- Supplement: 232
- BibTeX: 99
- EndNote: 92
Cited
24 citations as recorded by crossref.
- 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
- Ion Acceleration by Flux Transfer Events in the Terrestrial Magnetosheath R. Jarvinen et al. 10.1002/2017GL076192
- On the Importance of Spatial and Velocity Resolution in the Hybrid-Vlasov Modeling of Collisionless Shocks Y. Pfau-Kempf et al. 10.3389/fphy.2018.00044
- Fast plasma sheet flows and X line motion in the Earth's magnetotail: results from a global hybrid-Vlasov simulation L. Juusola et al. 10.5194/angeo-36-1183-2018
- Traveling Foreshocks and Transient Foreshock Phenomena P. Kajdič et al. 10.1002/2017JA023901
- Transmission of an ICME Sheath Into the Earth's Magnetosheath and the Occurrence of Traveling Foreshocks M. Ala‐Lahti et al. 10.1029/2021JA029896
- Ion Acceleration Efficiency at the Earth’s Bow Shock: Observations and Simulation Results A. Johlander et al. 10.3847/1538-4357/abfafc
- Hybrid-Vlasov Modelling of Ion Velocity Distribution Functions Associated with the Kelvin–Helmholtz Instability with a Density and Temperature Asymmetry V. Tarvus et al. 10.3847/1538-4357/ad697a
- The Scientific Foundations of Forecasting Magnetospheric Space Weather J. Eastwood et al. 10.1007/s11214-017-0399-8
- 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
- Foreshock Properties at Typical and Enhanced Interplanetary Magnetic Field Strengths: Results From Hybrid‐Vlasov Simulations L. Turc et al. 10.1029/2018JA025466
- Daring to think of the impossible: The story of Vlasiator M. Palmroth 10.3389/fspas.2022.952248
- Enabling technology for global 3D+3V hybrid-Vlasov simulations of near-Earth space U. Ganse et al. 10.1063/5.0134387
- Asymmetries in the Earth's dayside magnetosheath: results from global hybrid-Vlasov simulations L. Turc et al. 10.5194/angeo-38-1045-2020
- Magnetospheric responses to solar wind Pc5 density fluctuations: Results from 2D hybrid Vlasov simulation H. Zhou et al. 10.3389/fspas.2022.984918
- Spacecraft measurements constraining the spatial extent of a magnetopause reconnection X line B. Walsh et al. 10.1002/2017GL073379
- Dayside Pc2 Waves Associated With Flux Transfer Events in a 3D Hybrid‐Vlasov Simulation F. Tesema et al. 10.1029/2023GL106756
- Dayside Transient Phenomena and Their Impact on the Magnetosphere and Ionosphere H. Zhang et al. 10.1007/s11214-021-00865-0
- 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
- Vlasov methods in space physics and astrophysics M. Palmroth et al. 10.1007/s41115-018-0003-2
- Wave Activities Throughout a Low‐Mach Number Quasi‐Parallel Shock: 2‐D Hybrid Simulations Y. Hao et al. 10.1029/2023JA031295
- Transmission of foreshock waves through Earth’s bow shock L. Turc et al. 10.1038/s41567-022-01837-z
- Hybrid-Vlasov modeling of three-dimensional dayside magnetopause reconnection Y. Pfau-Kempf et al. 10.1063/5.0020685
- Local bow shock environment during magnetosheath jet formation: results from a hybrid-Vlasov simulation J. Suni et al. 10.5194/angeo-41-551-2023
Latest update: 30 Jun 2025
Short summary
We have simulated the interaction of the solar wind – the charged particles and magnetic fields emitted by the Sun into space – with the magnetic field of the Earth. The solar wind flows supersonically and creates a shock when it encounters the obstacle formed by the geomagnetic field. We have identified a new chain of events which causes phenomena in the downstream region to eventually cause perturbations at the shock and even upstream. This is confirmed by ground and satellite observations.
We have simulated the interaction of the solar wind – the charged particles and magnetic fields...
