Details

Autor(en) / Beteiligte

• Wilson III, L. B.
• Koval, A.
• Szabo, A.
• Breneman, A.
• Cattell, C. A.
• Goetz, K.
• Kellogg, P. J.
• Kersten, K.
• Kasper, J. C.
• Maruca, B. A.
• Pulupa, M.

Titel

Electromagnetic waves and electron anisotropies downstream of supercritical interplanetary shocks

Ist Teil von

• Journal of geophysical research. Space physics, 2013-01, Vol.118 (1), p.5-16

Ort / Verlag

Washington: Blackwell Publishing Ltd

Erscheinungsjahr

2013

Link zum Volltext

Quelle

Wiley Blackwell Single Titles

Beschreibungen/Notizen

• We present waveform observations of electromagnetic lower hybrid and whistler waves with fci ≪ f < fce downstream of four supercritical interplanetary shocks using the Wind search coil magnetometer. The whistler waves were observed to have a weak positive correlation between δB and normalized heat flux magnitude and an inverse correlation with Teh/Tec. All were observed simultaneous with electron distributions satisfying the whistler heat flux instability threshold and most with T⊥ h/T∥ h > 1.01. Thus, the whistler mode waves appear to be driven by a heat flux instability and cause perpendicular heating of the halo electrons. The lower hybrid waves show a much weaker correlation between δB and normalized heat flux magnitude and are often observed near magnetic field gradients. A third type of event shows fluctuations consistent with a mixture of both lower hybrid and whistler mode waves. These results suggest that whistler waves may indeed be regulating the electron heat flux and the halo temperature anisotropy, which is important for theories and simulations of electron distribution evolution from the Sun to the Earth. Key Points Whistler mode waves are driven unstable by heat flux instability Separation of core and halo is crucial for instability analysis in solar wind Whistler mode waves can cause halo temperature anisotropies