Energetic, ˜5-90 keV neutral atom imaging of a weak substorm with STEREO/STE

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Magnetospheric Physics: Substorms, Interplanetary Physics: Energetic Particles (7514), Magnetospheric Physics: Ring Current

Scientific paper

We present imaging and high resolution energy spectra of energetic ˜5-90 keV neutral atoms (ENA) of a weak geomagnetic substorm (Dst > -8 nT and AE $\lesssim$ 200 nT), made by the Suprathermal Electron (STE) instrument on the STEREO B spacecraft. Enhanced ENA emissions were observed coming from around local midnight near the equator with different spatial distribution and/or temporal behavior at ˜5-20keV compared to ˜20-90 keV. By forward modeling using a parameterized ring-current model, we show that the ENA images imply the parent equatorial protons have pitch-angle distributions peaked at 90°, an energy spectrum consistent with in situ proton measurements at geosynchronous orbit, and a spatial asymmetry with the maximum flux at midnight for 5-20 keV and at 2240 MLT for 20-90 keV. These are the first ENA measurements at ˜5 to 26 keV from low altitude, and the first for such weak activity.

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