video: The NSF Daniel K. Inouye Solar Telescope presents its first map of the solar coronal magnetic field signals as measured using the Zeeman Effect. The Zeeman Effect polarizes the coronal emission, which requires the advancements of the Inouye to measure as its signals are only a few parts per billion of the Sun’s surface brightness.
Credit: Credit: NSF/NSO/AURA
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Summary: The U.S. National Science Foundation (NSF) Daniel K. Inouye Solar Telescope, the world’s most powerful solar telescope, operated by the NSF National Solar Observatory (NSO), achieved a major breakthrough in solar physics by successfully producing its first detailed maps of the Sun’s coronal magnetic fields. This milestone, led by NSO Associate Astronomer Dr. Tom Schad, was recently published in Science Advances, and promises to enhance our understanding of the Sun's atmosphere and how its changing conditions lead to impacts on Earth's technology-dependent society. The corona, or the Sun’s outer atmosphere, greatly influences solar winds and space weather events like solar flares and coronal mass ejections. However, the magnetic forces that drive these events and the corona are challenging to measure. |
Embargoed: Not for Release Until 2:00 pm U.S. Eastern Time Wednesday, 11 September 2024.
Maui, Hawaii - The U.S. National Science Foundation (NSF) Daniel K. Inouye Solar Telescope, the world’s most powerful solar telescope, designed, built, and operated by the NSF National Solar Observatory (NSO), achieved a major breakthrough in solar physics by directly mapping the strength of the magnetic field in the solar corona, the outer part of the solar atmosphere that can be seen during a total eclipse. This breakthrough promises to enhance our understanding of space weather and its impact on Earth’s technology-dependent society.
The Corona: The Launch Pad of Space Weather
The Sun's magnetic field generates regions in the Sun's atmosphere, often rooted by sunspots, that store vast amounts of energy that fuel explosive solar storms and drive space weather. The corona, the Sun’s outer atmosphere, is a superheated realm where these magnetic mysteries unfold. Mapping coronal magnetic fields is essential to understanding and predicting space weather - and to protect our technology in Earth and space.
Why It Matters
Earth’s magnetic field shields us from solar winds, protecting our atmosphere, and making life possible. However, the electromagnetic fields and energetic particles from extreme solar eruptions can disrupt satellites, power grids, and other systems we need in our increasingly technological society. Understanding these dynamic interactions, which change on timescales ranging from days to centuries, is crucial for safeguarding our infrastructure and current way of life.
Measuring the corona’s magnetic properties has long challenged astronomers and the limits of technology. Today, the Inouye Solar Telescope is the most advanced facility designed to study the corona, and has made a crucial first step in resolving these mysteries by producing its first coronal magnetic field maps - the most detailed to date.
The Inouye Solar Telescope’s First Maps of the Corona’s Magnetic Field
Since the 1950s, solar physicists have mapped the magnetic fields on the Sun’s surface, providing valuable insights. However, maps of the magnetic field in the zones above the surface, like the corona, have long been sought as it is in these locations that solar storms originate. The Inouye, located near the summit of Maui’s Haleakalā in Hawai'i, now provides the capabilities to meet this critical need.
The Inouye has created its first detailed magnetic field maps of the solar corona using the Zeeman Effect, which measures magnetic properties by observing spectral line splitting. Spectral lines are distinct lines that appear at specific wavelengths in the electromagnetic spectrum, representing the light absorbed or emitted by atoms or molecules. These lines act like “fingerprints,” as they are unique to each atom or molecule, allowing scientists to identify the chemical composition and physical properties of celestial objects by looking at their spectra. When exposed to a magnetic field, like in the Sun, these lines split, which gives us an insight into the object’s magnetic properties. Previous attempts at detecting these signals, last reported two decades ago (Lin et al. 2004), lacked the detail and regularity needed for extensive scientific investigation. Today, the Inouye’s unmatched capabilities allow for detailed, regular studies of these crucial signals.
Technological Marvel
Typically, one can only view the Sun's corona - a region one million times fainter than the solar disk - during a total solar eclipse, when most of the Sun's light is blocked and Earth's sky goes dark. The Inouye, however, uses a technique called coronagraphy to create artificial eclipses, allowing it to detect extremely faint polarized signals - a billion times fainter than the solar disk - highlighting its unparalleled sensitivity and solidifying its status as a unique window to our home star.
The Inouye accomplishes this with its Cryogenic Near-Infrared Spectropolarimeter (Cryo-NIRSP), one of the telescope’s primary instruments used to study the corona and map its magnetic fields. This instrument was designed and built by the University of Hawai‘i Institute for Astronomy.
Dr. Tom Schad’s Research
“The Inouye’s achievement in mapping the Sun’s coronal magnetic fields is a testament to the innovative design and capabilities of this trailblazing unique observatory,” said Tom Schad, scientist at NSO, and first author of the study. “This breakthrough promises to significantly enhance our understanding of the solar atmosphere and its influence on our solar system.”
Future Prospects
This milestone marks the beginning of a new era in solar physics. The Inouye’s success in mapping the Sun’s coronal magnetic fields reaffirms its vision and mission, and opens new frontiers in understanding the Sun’s influence on space weather.
“Just as detailed maps of the Earth's surface and atmosphere have enabled more accurate weather prediction, this thrillingly complete map of the magnetic fields in the sun's corona will help us better predict solar storms and space weather," says Dr. Carrie Black, NSF program director for the NSO. "The invisible yet phenomenally powerful forces captured in this map will propel solar physics through the next century and beyond.”
Christoph Keller, NSO Director, remarks that "Mapping the strength of the magnetic field in the corona is a fundamental scientific breakthrough, not just for solar research, but for astronomy in general.” He anticipates that “This is the beginning of a new era where we will understand how the magnetic fields of stars affect planets, here in our own solar system and in the thousands of exoplanetary systems that we now know about."
Ongoing and future studies will refine diagnostic tools and techniques, leading to deeper insights into the Sun’s magnetic environment and its impact on Earth and our solar system.
More information, including a copy of the paper, can be found online at the Science Advances press package at https://www.eurekalert.org/press/vancepak/ or https://www.science.org/journal/sciadv.
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About the U.S. NSF Daniel K. Inouye Solar Telescope
The U.S. National Science Foundation (NSF) Daniel K. Inouye Solar Telescope is operated by the National Solar Observatory (NSO), a federally funded research and development center focused on solar research, under management by the Association of Universities for Research in Astronomy (AURA). The Inouye and NSO are funded by NSF through a cooperative agreement with AURA. The Inouye Solar Telescope is located on land of spiritual and cultural significance to Native Hawaiian people. The use of this important site to further scientific knowledge is done so with appreciation and respect. For more information, visit www.nso.edu.
The Inouye is the largest solar telescope in the world. With a focus on understanding the Sun’s explosive behavior, observations of magnetic fields are at the forefront of this innovative telescope. A combination of an off-axis design, to reduce scattered light, and cutting-edge polarimetery produces the first ongoing measurements of the magnetic fields in the Sun’s corona. The Inouye’s 4-meter mirror provides views of the solar atmosphere like we have never seen before. Focusing on small observing changes, the cutting-edge instrument suite gathers unprecedented images from the Sun’s surface to the lower solar atmosphere. The Inouye Solar Telescope reveals features three times smaller than anything we can see on the Sun today, and does so multiple times a second. Not only do the world-class instruments and optical assembly allow spectacular imagery, but also have incredible spectroscopic capabilities. Observing the specific fingerprints of hundreds of atoms and ions throughout the solar surface and atmosphere will help us explain the dynamic nature of the Sun’s behavior.
About the U.S. NSF National Solar Observatory
The mission of the U.S. National Science Foundation (NSF) National Solar Observatory (NSO) is to advance knowledge of the Sun, both as an astronomical object and as the dominant external influence on Earth, by providing forefront observational opportunities to the research community. The mission includes the operation of cutting edge facilities, the continued development of advanced instrumentation both in-house and through partnerships, conducting solar research, and educational and public outreach.
Contact
For media inquiries, please contact:
Evan Pascual
Communications Specialist
U.S. NSF National Solar Observatory
media@nso.edu
For science inquiries, please contact:
Tom Schad
Associate Astronomer
U.S. NSF National Solar Observatory
tschad@nso.edu
Journal
Science Advances
Method of Research
Observational study
Subject of Research
Not applicable
Article Title
Mapping the Sun’s coronal magnetic field using the Zeeman effect
Article Publication Date
11-Sep-2024