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Advances in Space Research, 1995
Plasma waves observed in the VLF range upstream of planetary bow shocks not only modify the particle distributions, but also provide important information about the acceleration processes that occur at the bow shock. Electron plasma oscillations observed near the tangent field line in the electron foreshock are generated by electrons reflected at the ...
E.W Greenstadt, G Le, R.J Strangeway
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Plasma waves observed in the VLF range upstream of planetary bow shocks not only modify the particle distributions, but also provide important information about the acceleration processes that occur at the bow shock. Electron plasma oscillations observed near the tangent field line in the electron foreshock are generated by electrons reflected at the ...
E.W Greenstadt, G Le, R.J Strangeway
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Finding foreshocks in the damage zone
Science, 2017Geophysics![Figure][1] Damage done by a 2005 earthquake in Balakot, Pakistan PHOTO: AGENCJA FOTOGRAFICZNA CARO/ALAMY STOCK PHOTO Foreshocks are small earthquakes that precede much larger and more damaging earthquakes.
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Foreshock Transients and Their Geoeffects
2020<p>Foreshock transients are frequently observed upstream from the bow shock (such as Hot Flow&#160;Anomalies, foreshock cavities, and foreshock bubbles). They play a significant role in the mass, energy&#160;and momentum transport from the solar wind into the magnetosphere and impact the whole&#160 ...
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Foreshock fluctuation and its behaviors
The foreshock region is a turbulent area that forms before a quasi-parallel shock. It is caused by the interaction between reflected particles from the bow shock and oncoming waves in the solar wind. Typically, the foreshock is located on the dawn side.Gilbert Pi +2 more
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