In December 2023, scientists looking at Mars data stumbled across something completely unexpected — observations of an atmospheric effect never before seen in the Red Planet’s atmosphere. Using instruments aboard NASA’s MAVEN (Mars Atmosphere and Volatile Evolution) mission, scientists identified a phenomenon known to occur in Earth’s magnetosphere, where charged particles are squeezed like toothpaste coming out of a tube along magnetic structures called flux tubes. This so-called Zwan-Wolf effect aids in the deflection of solar wind around Earth and has been observed and studied there for decades. Now, a new study published in Nature Communications provides the first comprehensive observations of the same effect in Mars’ atmosphere.
An artistic representation of the Zwan-Wolf effect at
Mars, as observed by NASA’s MAVEN (Mars Atmosphere and Volatile Evolution)
mission. While this effect typically helps to deflect the solar wind at Earth,
at Mars it is shown to “squeeze” the atmosphere and have implications on how
space weather interacts with the planet. The yellow arrows represent the
movement of the effect in the Martian atmosphere.
LASP/CU Boulder
“When investigating the data, I all of a
sudden noticed some very interesting wiggles,” said Christopher Fowler, a
research assistant professor at West Virginia University in Morgantown and lead
author of the study. “I would never have guessed it would
be this effect, since it’s never been seen in a planetary atmosphere before.”
The Zwan-Wolf effect was first
discovered in 1976, and until now has only been observed in planetary
magnetospheres, not their atmospheres. Unlike Earth, Mars is not protected by a
global magnetic field, affecting how it interacts with the solar wind and space
weather. In this new study, the Zwan-Wolf effect was observed in the ionosphere
— deep within the Martian atmosphere below 200 km — which contains significant
numbers of electrically charged particles. The data showed that these charged
particles were being squeezed and distributed around Mars’ atmosphere.
Although Mars has an induced
magnetosphere, a magnetic field generated by the solar wind interacting with
the Martian ionosphere, it can greatly change in size and shape with large
solar wind and space weather events. That is what Fowler and his team saw in
the MAVEN data when a large solar storm hit Mars. Based on their findings, the
Zwan-Wolf effect may be occurring constantly in the Martian ionosphere but at
levels undetectable by MAVEN’s instrumentation. The impact of the space weather
event appears to have amplified the effect, allowing the scientists to observe
it in the data.
In the beginning, Fowler and his team
came across some interesting-looking fluctuations in measurements of the
magnetic field as the spacecraft flew through the atmosphere. To explain this,
they dug into observations made by several instruments on MAVEN, including
measurements of the charged particle environment in the ionosphere. Their
sleuthing uncovered even more weird and interesting features in the data. After
ruling out several other possibilities, the team was able to identify the
culprit as the Zwan-Wolf effect, which explained all the features they were
seeing.
“No one expected that this effect could
even occur in the atmosphere,” said Fowler. “That’s what makes this even more
exciting. It introduces interesting physics that we haven’t yet explored and a
new way the Sun and space weather can change the dynamics in the Martian
atmosphere.”
Understanding the Zwan-Wolf effect at
Mars will further our understanding of how space weather affects the planet and
provides new insight into how this effect might occur at similar unmagnetized
bodies, such as Venus and Saturn’s moon Titan. Observations like this also
highlight the importance of knowing how large space weather events can lead to
changes in the environment at and around the Red Planet and potentially affect
assets on or near Mars.
“Knowing how space weather interacts
with Mars is essential,” said Shannon Curry, the principal investigator of
MAVEN and research scientist at the Laboratory for Atmospheric Space Physics at
the University of Colorado Boulder. “The MAVEN team continues making new
discoveries with our datasets and finding these links between our host star and
the Red Planet.”
The MAVEN spacecraft launched in
November 2013 and entered Mars’ orbit in September 2014. The mission’s goal is
to explore the planet’s upper atmosphere, ionosphere, and interactions with the
Sun and solar wind to explore the loss of the Martian atmosphere to space.
Understanding atmospheric loss gives scientists insight into the history of the
Red Planet’s atmosphere and climate, liquid water, and planetary habitability.
The MAVEN spacecraft, in orbit around Mars, experienced a loss of signal with
ground stations on Earth on Dec. 6, 2025. In Feb. 2026, NASA launched an
anomaly review board to assess the probable current state of the spacecraft and
the likelihood of its recovery.
The
MAVEN mission is part of NASA’s Mars Exploration Program portfolio. The
mission’s principal investigator is based at the
Laboratory for Atmospheric and Space Physics at the University of Colorado
Boulder, which is also responsible for managing science operations and public
outreach and communications. NASA’s Goddard Space Flight Center in
Greenbelt, Maryland, manages the MAVEN mission. Lockheed Martin Space built the
spacecraft and is responsible for mission operations. NASA’s Jet Propulsion
Laboratory in Southern California provides navigation and Deep Space Network
support.
By
Willow Reed
Laboratory
for Atmospheric and Space Physics, University of Colorado Boulder
Source: NASA’s MAVEN Makes 1st Discovery of Atmospheric Effect at Mars - NASA Science

