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Over the southern solar pole: low-energy interplanetary charged particles
L J Lanzerotti1, T P Armstrong, R E Gold
1AT&T Bell Laboratories, Murray Hill, NJ 07974, USA.
Summary
The heliospheric current sheet significantly shapes the heliosphere, even in polar regions. Interplanetary shocks accelerated electrons far from Ulysses
Area of Science:
- Space physics
- Heliophysics
- Plasma physics
Background:
- The heliosphere's structure is influenced by solar activity and magnetic fields.
- Understanding particle transport in the heliosphere is crucial for space weather prediction.
Purpose of the Study:
- To investigate the influence of the heliospheric current sheet on particle fluxes in the southern polar region.
- To analyze the acceleration mechanisms of low-energy ions and electrons.
Main Methods:
- Utilized data from the Heliosphere Instrument for Spectrum, Composition, and Anisotropy (HISCALE) on the Ulysses spacecraft.
- Analyzed fluxes of low-energy ions and electrons (> 50 keV) during polar crossings.
Main Results:
- The heliospheric current sheet significantly influenced the heliosphere's structure down to -75 degrees heliolatitude.
- Interplanetary reverse shocks accelerated electrons far from the Ulysses spacecraft.
- Anomalous oxygen flux and Ne/O ratios were measured at high heliolatitudes.
Conclusions:
- The heliospheric current sheet plays a dominant role in shaping the heliosphere.
- Particle acceleration is linked to current sheet dynamics and interplanetary shocks.
- Further research is needed to clarify low-energy electron flux enhancements at higher heliolatitudes.
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