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MAVEN Spots First Zwan-Wolf Effect in Mars’ Atmosphere

The finding shows solar storms squeeze charged gas deep in Mars’ ionosphere to help explain how the planet loses atmosphere.

Overview

  • NASA disclosed in May 2026 that MAVEN data reveal the Zwan-Wolf effect inside Mars’ ionosphere during a strong solar storm in December 2023.
  • The peer-reviewed study in Nature Communications reports large magnetic structures plunging below 200 km, with five features tracked down to about 185 km and local plasma density dropping 30–40%.
  • Lead author Christopher Fowler first flagged odd magnetic “wiggles,” then a multi-instrument review of charged particles and fields ruled out other causes and matched the Zwan-Wolf mechanism.
  • The effect squeezes and redistributes ionospheric plasma, pointing to a pathway for atmospheric loss on Mars and likely operating, often too weak to see, on unmagnetized worlds like Venus and Titan.
  • MAVEN has been out of contact since December 6, 2025, and NASA formed an anomaly review board in February 2026 to assess the spacecraft’s state and prospects for recovery.