Traveling foreshocks and transient foreshock phenomena
Primoz Kajdic, Xochitl Blanco-Cano, Nojan Omidi, Diana Rojas-Castillo,, David G. Sibeck, Laurence Billingham

TL;DR
This paper identifies and characterizes two types of foreshocks using multi-spacecraft data, revealing their properties, boundaries, and related phenomena like cavities and hot flow anomalies.
Contribution
It distinguishes between global and traveling foreshocks, introduces the concept of foreshock cavities, and provides statistical analysis of related transient phenomena.
Findings
Traveling foreshocks are bounded by rotational discontinuities and propagate along the bow-shock.
Foreshock cavities are a subset of traveling foreshocks with minimal wave development.
Spontaneous hot flow anomalies are highly depleted in magnetic field and plasma density.
Abstract
We use the multi-spacecraft capabilities of the Cluster and THEMIS missions to show that two types of foreshock may be detected in spacecraft data. One is the global foreshock that appears upstream of the Earth's quasi-parallel bow-shock under steady or variable interplanetary magnetic field. Another type is a traveling foreshock that is bounded by two rotational discontinuities in the interplanetary magnetic field and propagates along the bow-shock. Foreshock compressional boundaries are found at the edges of both types of foreshock. We show that isolated foreshock cavities are a subset of the traveling foreshock that form when two bounding rotational discontinuities are so close that the ultra-low frequency waves do not develop in the region between them. We also report observations of a spontaneous hot flow anomaly inside a traveling foreshock. This means that other phenomena, such…
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