Simulations show that a single-hemisphere, high-latitude-polarity-inversion magnetic topology on a moderately rotating M dwarf would produce mostly high-latitude CMEs and only mild CME-driven pressure enhancements at equatorial exoplanet orbits.
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Intense but Harmless: Exo-Space Weather Around an M Dwarf with a Single-Hemisphere Dynamo
Simulations show that a single-hemisphere, high-latitude-polarity-inversion magnetic topology on a moderately rotating M dwarf would produce mostly high-latitude CMEs and only mild CME-driven pressure enhancements at equatorial exoplanet orbits.