Articles | Volume 37, issue 4
Ann. Geophys., 37, 689–697, 2019
https://doi.org/10.5194/angeo-37-689-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Ann. Geophys., 37, 689–697, 2019
https://doi.org/10.5194/angeo-37-689-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
ANGEO Communicates
06 Aug 2019
ANGEO Communicates
| 06 Aug 2019
Jets in the magnetosheath: IMF control of where they occur
Laura Vuorinen et al.
Viewed
Total article views: 1,421 (including HTML, PDF, and XML)
Cumulative views and downloads
(calculated since 06 May 2019)
| HTML | XML | Total | BibTeX | EndNote | |
|---|---|---|---|---|---|
| 921 | 482 | 18 | 1,421 | 27 | 17 |
- HTML: 921
- PDF: 482
- XML: 18
- Total: 1,421
- BibTeX: 27
- EndNote: 17
Total article views: 1,029 (including HTML, PDF, and XML)
Cumulative views and downloads
(calculated since 06 Aug 2019)
| HTML | XML | Total | BibTeX | EndNote | |
|---|---|---|---|---|---|
| 692 | 322 | 15 | 1,029 | 23 | 14 |
- HTML: 692
- PDF: 322
- XML: 15
- Total: 1,029
- BibTeX: 23
- EndNote: 14
Total article views: 392 (including HTML, PDF, and XML)
Cumulative views and downloads
(calculated since 06 May 2019)
| HTML | XML | Total | BibTeX | EndNote | |
|---|---|---|---|---|---|
| 229 | 160 | 3 | 392 | 4 | 3 |
- HTML: 229
- PDF: 160
- XML: 3
- Total: 392
- BibTeX: 4
- EndNote: 3
Viewed (geographical distribution)
Total article views: 1,215 (including HTML, PDF, and XML)
Thereof 1,209 with geography defined
and 6 with unknown origin.
Total article views: 883 (including HTML, PDF, and XML)
Thereof 879 with geography defined
and 4 with unknown origin.
Total article views: 332 (including HTML, PDF, and XML)
Thereof 330 with geography defined
and 2 with unknown origin.
| Country | # | Views | % |
|---|
| Country | # | Views | % |
|---|
| Country | # | Views | % |
|---|
| Total: | 0 |
| HTML: | 0 |
| PDF: | 0 |
| XML: | 0 |
- 1
1
| Total: | 0 |
| HTML: | 0 |
| PDF: | 0 |
| XML: | 0 |
- 1
1
| Total: | 0 |
| HTML: | 0 |
| PDF: | 0 |
| XML: | 0 |
- 1
1
Cited
14 citations as recorded by crossref.
- Mechanisms and Evolution of Geoeffective Large-Scale Plasma Jets in the Magnetosheath A. Dmitriev et al. 10.3390/universe7050152
- 3D Space‐Time Adaptive Hybrid Simulations of Magnetosheath High‐Speed Jets Y. Omelchenko et al. 10.1029/2020JA029035
- Solar Wind Control of Magnetosheath Jet Formation and Propagation to the Magnetopause A. LaMoury et al. 10.1029/2021JA029592
- Magnetosheath Microstructure: Mirror Mode Waves and Jets during Southward IP Magnetic Field X. Blanco‐Cano et al. 10.1029/2020JA027940
- On the Generation of Pi2 Pulsations due to Plasma Flow Patterns Around Magnetosheath Jets C. Katsavrias et al. 10.1029/2021GL093611
- Connection Between Foreshock Structures and the Generation of Magnetosheath Jets: Vlasiator Results J. Suni et al. 10.1029/2021GL095655
- Evolution of High‐Speed Jets and Plasmoids Downstream of the Quasi‐Perpendicular Bow Shock O. Goncharov et al. 10.1029/2019JA027667
- Statistical Study of Magnetosheath Jet‐Driven Bow Waves T. Liu et al. 10.1029/2019JA027710
- Magnetosheath jet evolution as a function of lifetime: global hybrid-Vlasov simulations compared to MMS observations M. Palmroth et al. 10.5194/angeo-39-289-2021
- Classifying Magnetosheath Jets Using MMS: Statistical Properties S. Raptis et al. 10.1029/2019JA027754
- Electron Acceleration by Magnetosheath Jet‐Driven Bow Waves T. Liu et al. 10.1029/2019JA027709
- Scale Sizes of Magnetosheath Jets F. Plaschke et al. 10.1029/2020JA027962
- Magnetic Field in Magnetosheath Jets: A Statistical Study of B Z Near the Magnetopause L. Vuorinen et al. 10.1029/2021JA029188
- Classifying the Magnetosheath Behind the Quasi‐Parallel and Quasi‐Perpendicular Bow Shock by Local Measurements T. Karlsson et al. 10.1029/2021JA029269
14 citations as recorded by crossref.
- Mechanisms and Evolution of Geoeffective Large-Scale Plasma Jets in the Magnetosheath A. Dmitriev et al. 10.3390/universe7050152
- 3D Space‐Time Adaptive Hybrid Simulations of Magnetosheath High‐Speed Jets Y. Omelchenko et al. 10.1029/2020JA029035
- Solar Wind Control of Magnetosheath Jet Formation and Propagation to the Magnetopause A. LaMoury et al. 10.1029/2021JA029592
- Magnetosheath Microstructure: Mirror Mode Waves and Jets during Southward IP Magnetic Field X. Blanco‐Cano et al. 10.1029/2020JA027940
- On the Generation of Pi2 Pulsations due to Plasma Flow Patterns Around Magnetosheath Jets C. Katsavrias et al. 10.1029/2021GL093611
- Connection Between Foreshock Structures and the Generation of Magnetosheath Jets: Vlasiator Results J. Suni et al. 10.1029/2021GL095655
- Evolution of High‐Speed Jets and Plasmoids Downstream of the Quasi‐Perpendicular Bow Shock O. Goncharov et al. 10.1029/2019JA027667
- Statistical Study of Magnetosheath Jet‐Driven Bow Waves T. Liu et al. 10.1029/2019JA027710
- Magnetosheath jet evolution as a function of lifetime: global hybrid-Vlasov simulations compared to MMS observations M. Palmroth et al. 10.5194/angeo-39-289-2021
- Classifying Magnetosheath Jets Using MMS: Statistical Properties S. Raptis et al. 10.1029/2019JA027754
- Electron Acceleration by Magnetosheath Jet‐Driven Bow Waves T. Liu et al. 10.1029/2019JA027709
- Scale Sizes of Magnetosheath Jets F. Plaschke et al. 10.1029/2020JA027962
- Magnetic Field in Magnetosheath Jets: A Statistical Study of B Z Near the Magnetopause L. Vuorinen et al. 10.1029/2021JA029188
- Classifying the Magnetosheath Behind the Quasi‐Parallel and Quasi‐Perpendicular Bow Shock by Local Measurements T. Karlsson et al. 10.1029/2021JA029269
Latest update: 26 May 2022
Short summary
Before the solar wind encounters the Earth's magnetic field, it is first slowed down and deflected by the Earth's bow shock. We find that downstream of the bow shock regions where the shock normal and the solar wind magnetic field are almost parallel and the shock is more rippled, plasma jets with high earthward velocities are observed significantly more often than elsewhere downstream of the shock. Our results help us forecast the occurrence of these jets and their effects on Earth.
Before the solar wind encounters the Earth's magnetic field, it is first slowed down and...
