Compressional boundaries in the Earth's foreshock
Journal Article
·
· AIP Conference Proceedings
- Instituto de Geofisica, Universidad Nacional Autonoma de Mexico, Coyoacan (Mexico)
- Institut de Recherche en Astrophysique et Planetologie, Toulouse (France)
- Solana Scientific Inc., Solana Beach, California (United States)
The terrestrial foreshock is a highly dynamic region populated by particles, waves and non-linear structures such as shocklets, SLAMS, hot flow anomalies, cavities and cavitons. Recently a new structure named foreshock compressional boundary (FCB) was reported in global hybrid simulations by Omidi et al. (2009). This structure represents a transition region that separates the highly disturbed foreshock plasma from pristine solar wind or from the region of field-aligned ion beams. The FCB is associated with a strong compression of magnetic field and density. Besides the enhancements in the field and density, the FCB also shows a region where these two quantities decrease below the ambient solar wind (SW) values. Here, we study a FCB observed by Cluster-1. This FCB shows that although sometimes FCBs are transition regions between the pristine solar wind plasma and the foreshock plasma, in this case the FCB separates a region with large amplitude waves from regions with high frequency (f{approx}1.7 Hz) small amplitude waves. We analyze the FCB properties, ion distributions inside them, and the waves near the structure.
- OSTI ID:
- 22118617
- Journal Information:
- AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1539; ISSN APCPCS; ISSN 0094-243X
- Country of Publication:
- United States
- Language:
- English
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