National Solar Observatory

Check out the National Science Foundation (NSF) National Solar Observatory's exciting results from the 2024 total solar eclipse, now featured on the cover of the University of Colorado Boulder's Research & Innovation Office news! Dive into our story, "Total Solar Eclipse Fuels Research, Education," and explore the latest in other research and creative projects: https://ow.ly/Gxry50TRaVN

MAGFiLO is a highly detailed dataset with expert annotations for 10,244 solar filaments. Its purpose is to train machine learning models to automatically identify and analyze solar filaments in real-time using data from the U.S. National Science Foundation (NSF) Global Oscillation Network Group (GONG). This will enhance early filament detection, improve space weather prediction models, and help keep us one step ahead of the Sun's most extreme outbursts. The development of MAGFiLO represents the convergence of two rapidly advancing fields - solar physics and Artificial Intelligence. This dataset, captured by NSF GONG stations operated by the NSF National Solar Observatory with support from the NOAA: National Oceanic & Atmospheric Administration, is the result of 1,593 solar observations and over 1,000 person-hours of expert manual annotation and review processes. The application of AI/ML to the study of solar filaments signals a transformative phase in solar physics. These findings were published in Nature'sa Scientific Data journal. Learn more below. https://lnkd.in/gaYFmVne

Three National Science Foundation (NSF) National Solar Observatory NISP scientists - Kiran Jain, Gordon Petrie, and Alexei Pevtsov - are attending the Solar Cycle Variability: From Understanding to Making Prediction conference in Nainital, India! Kiran (pictured) presented a solicited talk titled "Solar-cycle related changes below the surface of the Sun," Gordon gave an invited talk on "Polarity reversals of the solar magnetic field," and Alexei gave an invited review titled "Studies on the solar magnetic field." Many conference presentations by non-NSO participants included NSF GONG and NSF SOLIS data, mainly magnetograms, but also helioseismic data and results on internal solar rotation, meridional flows, and torsional oscillations. Magnetograms were used in Coronal Mass Ejections/flare studies, machine learning, and solar cycle studies. Alexei also took questions about the next generation ngGONG!

Congrats to National Science Foundation (NSF) NSO Scientist Gordon Petrie (right) on receiving Springer Nature's 2024 Kees de Jager Prize for the best article published in the journal Solar Physics in 2023!🏆👏 Full announcement: https://lnkd.in/gwtbHaY4

In a remarkable breakthrough, a group of scientists led by U.S. National Science Foundation (NSF) National Solar Observatory (NSO) scientist Tetsu Anan has unveiled the scale of electric fields driving explosive phenomena in the solar atmosphere. The team used unique data from the NSF Daniel K. Inouye Solar Telescope, built and operated by the NSO. They discovered that the spatial scale of these electric fields reach a staggering one megameter, challenging prior estimates around the centimeter to meter range. These findings, published in Nature Communications, challenge long-held assumptions about the triggers behind solar flares, and other energetic solar events. Read more at the link below. https://lnkd.in/gwWV9aVP #NSFfunded #InouyeSolarTelescope #SolarResearch

Congrats to NSO Senior Mechanical Engineer, Brialyn Onodera, for winning the Best Paper Prize at the SPIE Ground-based and Airborne Telescope X conference! Her paper details the efforts made to surveil and mitigate vibrations at the National Science Foundation (NSF) Daniel K. Inouye Solar Telescope to ensure crystal-clear solar observations. View the paper, "An Update on the DKIST's Sitewide Vibration Surveillance and Mitigation Efforts," here: https://lnkd.in/gaujrVrp #SPIE #WomenInStem #InouyeSolarTelescope #Engineer

Two key instruments, the Vector Spectromagnetograph and the Full Disk Patrol, were successfully installed on the main telescope mount of the U.S. National Science Foundation (NSF) Synoptic Optical Long-term Investigations of the Sun (SOLIS) facility at Big Bear Solar Observatory, in California. This marks a significant step forward in bringing SOLIS to first light! https://lnkd.in/gSEkPUXQ

As the National Science Foundation (NSF) Daniel K. Inouye Solar Telescope patiently awaits the Sun's return at dawn, the Milky Way majestically arcs across Haleakalā's night sky. 📷: Irina Singer #InouyeSolarTelescope #Astrophotography

What a fun day at Kihei Charter School in Maui, Hawai'i! Our Outreach team visited to share the wonders of the Sun and the exciting research happening at the National Science Foundation (NSF) Inouye Solar Telescope. Students got a safe, up-close view of the Sun through our solar telescopes, seeing multiple sunspots and a solar prominence!

A recent study using invaluable data from the U.S. National Science Foundation (NSF) Daniel K. Inouye Solar Telescope, operated by the NSF National Solar Observatory, has documented the rotation of two small, dark features on the Sun's surface, known as pores, which appear to be linked to a less powerful C-class solar flare. Flares are classified according to their strength—the weakest are B-class, followed by C, M and X, the strongest. These pores, which are very small sunspots, and tiny compared to the Sun's overall scale, rotated in a manner never before observed, raising intriguing questions about the interaction between different layers of the Sun's atmosphere during solar flares. https://lnkd.in/gVkv_wV5