English
 
Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT
Add to Basket
  Local TagsRelease HistoryDetailsSummary

Released
Conference Paper

Compressive foreshock structures and their association with the foreshock boundary and the bow shock

Authors

Xirogiannopoulou,  Niki
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

Goncharov,  Oleksandr
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

Safrankova,  Jana
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

Nemecek,  Zdenek
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

External Ressource
No external resources are shared
Fulltext (public)
There are no public fulltexts stored in GFZpublic
Supplementary Material (public)
There is no public supplementary material available
Citation

Xirogiannopoulou, N., Goncharov, O., Safrankova, J., Nemecek, Z. (2023): Compressive foreshock structures and their association with the foreshock boundary and the bow shock, XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG) (Berlin 2023).
https://doi.org/10.57757/IUGG23-0970


Cite as: https://gfzpublic.gfz-potsdam.de/pubman/item/item_5016507
Abstract
The turbulent foreshock region upstream of the quasi- parallel bow shock is dominated by waves and reflected particles that interact with each other and create a large number of different foreshock phenomena. Plasma structures with enhanced magnetic field (Short Large Amplitude Magnetic Structures or SLAMS), and density spikes, named plasmoids, are frequently observed. Based on our previous results, we have found that there is a category of events exhibiting both magnetic field and density enhancements simultaneously and we introduce the term “mixed structure” for them. Using measurements of the Magnetospheric Multiscale Spacecraft (MMS) and OMNI solar wind database, we try to explore the origin of these structures, their occurrence rate and properties in association with the foreshock boundary. Moreover, we attempt to trace and observe their interaction with the bow shock, using multi-spacecraft analysis by simultaneous measurements of Cluster, THEMIS, GEOTAIL and MMS and discuss their evolution.