Fig. 5 from On Pitch‐Angle Scattering Rates of Interstellar Pickup Ions as Determined by in Situ Measurement of Velocity Distributions

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On Pitch‐Angle Scattering Rates of Interstellar Pickup Ions as Determined by in Situ Measurement of Velocity Distributions

Authors: Lukas Saul, Eberhard Möbius, Philip Isenberg, and Peter Bochsler

Saul et al. 2007 The Astrophysical Journal 655 672.

Provider: AAS Journals

Caption: Fig. 5.

SOHO CTOF helium energy flux velocity spectra averaged over times of indicated transverse wave power in near‐radial IMF, in the solar wind frame. The best‐fit hemispheric model is shown as a continuous line. The associated best‐fit parameter for each plot is given in Fig. 6.

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