All previously observed images were captured from the Sun’s equatorial region. This is due to the fact that Earth, along with other planets and operational spacecraft, orbits the Sun in a flat disk known as the zodiac plane. By adjusting its orbit away from this plane, the ESA Solar Orbiter spacecraft unveils the Sun from an entirely new perspective.
A lower-half image of the Sun, highlighting a square area around its Antarctic. Captured in ultraviolet rays, it reveals hot gases in the Sun’s corona, glowing yellow as they extend outwards with threads and loops. Image credits: ESA/NASA/SOLAR ORBITER/EUI Team/D. Berghmans, Rob.
Professor Carol Mandel, ESA’s Director of Science, remarked:
“The Sun, being our closest star, is essential for life but can also disrupt modern power systems in space and on Earth. Therefore, understanding its mechanisms and predicting its behavior is crucial.”
“The new and unique perspectives provided by the Solar Orbiter mission signal the beginning of a new era in solar science.”
The images were captured by three different scientific instruments on the Solar Orbiter: Polarimetry and Helioseismology Imager (PHI), Extreme Ultraviolet Imager (EUI), and Spectral Imaging of the Coronal Environment (SPICE).
“Initially, I was uncertain of what to anticipate from these observations. The solar pole is truly a Terra Incognita,” said Professor Sami Solanki, leader of the PHI team at the Max Planck Institute for Solar System Research.
This collage shows the Antarctic of the Sun captured on March 16-17, 2025, as the solar orbiter observed from a 15° angle relative to the solar equator. This marked the first high-angle observation campaign just days before achieving its current maximum viewing angle of 17°. Image credits: ESA/NASA/Solar Orbiter/PHI/EUI/SPICE Team.
Each instrument on the Solar Orbiter observes the Sun differently.
PHI captures images of the Sun in visible light (top left) and maps its surface magnetic field (top center).
EUI images the Sun in ultraviolet light (top right), unveiling the corona, a multi-million-degree gas layer in the Sun’s outer atmosphere.
SPICE captures light from various temperatures of charged gases at the Sun’s surface, thereby revealing different layers of its atmosphere.
By analyzing and comparing observations from these three imaging instruments, we can understand how materials in the Sun’s outer layer move.
This could uncover unexpected patterns like polar vortices (swirling gases), reminiscent of those found around the poles of Venus and Saturn.
These innovative observations are crucial for understanding the solar magnetic field, particularly why it inverts every 11 years, aligning with peaks in solar activity.
Current predictive models for the 11-year solar cycle struggle to accurately forecast when and how the Sun will reach its peak activity.
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One of the primary scientific discoveries from Solar Orbiter’s polar observations is that the solar magnetic field is currently disordered in the Antarctic region.
While traditional magnets exhibit defined Arctic and Antarctic poles, magnetic measurements from the PHI instrument demonstrate that both polarities exist in the Antarctic region of the Sun.
This phenomenon occurs only briefly during each solar cycle when the magnetic field is reversed at the solar maximum.
Following this reversal, a single polarity gradually takes over the solar pole.
After 5-6 years, the Sun reaches the minimum phase of its cycle, during which its magnetic field is most organized, resulting in the lowest activity levels.
“How this accumulation occurs is not fully understood, so the timing of the solar orbiter’s high latitude observations is remarkably advantageous for tracking the entire process,” noted Professor Solanki.
PHI’s perspective on the solar magnetic field contextualizes these measurements.
The intensity of color (red or blue) signifies the strength of the magnetic field along the line of sight from the solar orbiter to the Sun.
The strongest magnetic fields manifest as two bands flanking the solar equator.
Dark red and blue regions highlight areas of concentrated magnetic fields associated with solar spots on the Sun’s surface (photosphere).
Additionally, both the Antarctic and Arctic regions exhibit red and blue spots, indicating a complex, constantly evolving solar magnetic structure on a smaller scale.
Another noteworthy discovery from the Solar Orbiter comes from the SPICE instrument.
This imaging spectrograph analyzes light (spectral lines) emitted by specific chemical elements such as hydrogen, carbon, oxygen, neon, and magnesium, at known temperatures.
Over the last five years, SPICE has employed this method to uncover processes occurring in various layers of the Sun’s surface.
For the first time, the SPICE team was able to utilize precise spectral line tracing to measure the velocity of moving solar material.
This technique, known as “Doppler measurement,” is named after the effect observed with an ambulance siren as it approaches and recedes, causing a change in pitch.
The resulting velocity map illustrates the movement of solar material within specific solar layers.
“Measurements from high latitudes, made possible with the Solar Orbiter, will revolutionize solar physics,” stated Dr. Frederic Aucele, leader of the SPICE team at Paris Sacree University.
Source: www.sci.news
