Imperial College London
Alternate

Emeritus ProfessorStevenSchwartz

Faculty of Natural Sciences, Department of Physics

Distinguished Research Fellow
 
 
 
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Contact

 

s.schwartz Website

 
 
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Assistant

 

Mr Luke Kratzmann +44 (0)20 7594 7770

 
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Location

 

708BHuxley BuildingSouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@article{Archer:2014:10.1016/j.pss.2014.11.026,
author = {Archer, MO and Turner, DL and Eastwood, JP and Schwartz, SJ and Horbury, TS},
doi = {10.1016/j.pss.2014.11.026},
journal = {Planetary and Space Science},
pages = {56--66},
title = {Global impacts of a Foreshock Bubble: Magnetosheath, magnetopause and ground-based observations},
url = {http://dx.doi.org/10.1016/j.pss.2014.11.026},
volume = {106},
year = {2014}
}
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RIS format (EndNote, RefMan)

TY  - JOUR
AB  - Using multipoint observations we show, for the first time, that Foreshock Bubbles (FBs) have a global impact on Earths magnetosphere. We show that an FB, a transient kinetic phenomenon due to the interaction of backstreaming suprathermal ions with a discontinuity, modifies the total pressure upstream of the bow shock showing a decrease within the FBs core and sheath regions. Magnetosheath plasma is accelerated towards the intersection of the FBs current sheet with the bow shock resulting in fast, sunward, flows as well as outward motion of the magnetopause. Ground-based magnetometers also show signatures of this magnetopause motion simultaneously across at least 7 h of magnetic local time, corresponding to a distance of 21.5RE transverse to the Sun–Earth line along the magnetopause. These observed global impacts of the FB are in agreement with previous simulations and in stark contrast to the known localised, smaller scale effects of Hot Flow Anomalies (HFAs).
AU  - Archer,MO
AU  - Turner,DL
AU  - Eastwood,JP
AU  - Schwartz,SJ
AU  - Horbury,TS
DO  - 10.1016/j.pss.2014.11.026
EP  - 66
PY  - 2014///
SN  - 1873-5088
SP  - 56
TI  - Global impacts of a Foreshock Bubble: Magnetosheath, magnetopause and ground-based observations
T2  - Planetary and Space Science
UR  - http://dx.doi.org/10.1016/j.pss.2014.11.026
UR  - http://hdl.handle.net/10044/1/26214
VL  - 106
ER  -
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