Measurements of 3D Structure in Solar Wind Langmuir Waves David Malaspina / Robert Ergun University of Colorado, Boulder, USA Laboratory for Atmospheric and Space Physics (LASP) STEREO SWG April 21, 2008 Meudon, France. Classification of 3D Structure. -0.5 0 0.5 .
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Solar Wind Langmuir Waves
David Malaspina / Robert Ergun
University of Colorado, Boulder, USA
Laboratory for Atmospheric and Space Physics (LASP)
April 21, 2008
-0.5 0 0.5
-6 0 6
E || Bz
E || Bx
E || By
Angle Between XMax and B
Green: Distinct Packets Red: Other WaveformsBlue: All waveforms
STA – GreenSTB- Red
0 15 250
Imin / Imid
Count / Day
0 40 80
1 5 10 15 20 25 30Day of Month (Jan. 2007)
Does not appear to be shock correlated…
5 Plasma oscillation periods
Rotation Freq. << Plasma Freq.
(~ 25 – 75 Hz ) << (~ 10 kHz – 35 kHz)
Langmuir wave has components || and ┴ to B
Response of plasma wave to Ion-Acoustic wave?
300 Plasma oscillation periods
Scale size (km)
Similar Packet Scale Sizes in || and ┴ directions
Reflection at density gradients
Kellogg, P.J., Goetz, K., Monson, S.J., Bale, S.D., Langmuir waves in a fluctuating solar wind, J. Geophys. Res. 104. 17,069, 1999.
Langmuir Z-mode Coupling
Bale, S.D., Goetz, K., Monson, S.J., Transverse Z-Mode waves in the terrestrial electron foreshock. Geophys. Res. Lett., 25, 1, 9, 1998.
A Langmuir wave Eigenmode is:
High frequency response of the Zakharov equations to an energetic electron beam passing through a shallow, pre-existing parabolic density cavity in the solar wind.
Pre-Existing Density Cavity:
Electric Field High-Frequency Response
Power Spectrum Fit
Etotal = ΣEnx*Eny*Enz
Artificial 3D Eigenmode