Physics
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsh43a1636b&link_type=abstract
American Geophysical Union, Fall Meeting 2008, abstract #SH43A-1636
Physics
7815 Electrostatic Structures, 7829 Kinetic Waves And Instabilities, 7839 Nonlinear Phenomena (4400, 6944), 7852 Solitons And Solitary Waves (4455), 7867 Wave/Particle Interactions (2483, 6984)
Scientific paper
Bipolar electrostatic structures are commonly observed in planetary magnetospheric environments but also in the solar wind. They may play a crucial role in transporting energy over long distances. In an earlier work, Mangeney et al. (1998) and Lacombe et al. (2002) have shown, in the solar wind, the presence of a small potential drop across the structures. This work was based on in-situ measurements obtained by the WAVES radio instrument of the WIND mission. The STEREO/WAVES instruments provide us with new in-situ measurements of bipolar electrostatic structures. We will present a comparative study of the observations from the three instruments. A model based on Vlasov-Ampere simulations will be proposed to explain the differences between the measurements of the two instruments.
Bale Stuart D.
Briand Carine
Califano Francesco
Goetz Keith
Henri Pierre
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