Researchers have captured the most detailed view ever of the Sun, thanks to the National Science Foundation’s Daniel K. Inouye Solar Telescope (DKIST) on Haleakalā, Maui.
The imagery, released today, shows cell-like structures the size of Texas roiling on the Sun’s surface and the tiny footprints of magnetism that reach into space.
Scientists operating the Inouye Solar Telescope said the unprecedented detail demonstrates the sheer power of the ground-based telescope to map the magnetic fields within the Sun’s corona, where solar eruptions occur that impact life on Earth. Such activity can disrupt air travel, cause blackouts, and even disable technologies such as GPS used for navigation.
“It is literally the greatest leap in humanity’s ability to study the Sun from the ground since Galileo’s time. It’s a big deal,” said Professor Jeff Kuhn of the University of Hawaii at Mānoa’s Institute for Astronomy (IfA).
DKIST will be even more powerful after a suite of state-of-the-art instruments come online in the coming months. A team of IfA scientists constructed two complex infrared instruments that ultimately will allow scientists to predict the Sun’s magnetic activity and solar storms. The first is called the Cryogenic Near-Infrared Spectropolarimeter (CryoNIRSP). The nearly 2-ton instrument is designed to measure the Sun’s magnetism beyond the visible solar disk. The second, called the Diffraction-Limited Near-IR Spectropolarimeter (DL-NIRSP), will allow DKIST to view the evolution of the Sun’s magnetic fields in extreme detail.
“These instruments use sensitive infrared technology and complex optics that reveal sunspots and small magnetic features, and how their magnetism reaches into space. With these new tools we expect to learn how the Sun interacts with the Earth,” Kuhn said.
Solar research at the House of the Sun
DKIST is by far the world’s largest and most powerful solar telescope, and stands on the 10,000-foot summit of Maui’s majestic Haleakalā, which literally means “the house of the Sun.” Haleakalā’s favorable atmospheric conditions provide the best location for it, as proven by the National Solar Observatory and IfA during a world-wide site survey.
The unusual optical design of the 4-meter telescope allows it to measure the Sun’s magnetism out into space. It is also modeled after the UH/IfA designed proof-of-concept SOLARC telescope, in operation on Haleakalā since 2001. Once the Inouye Solar Telescope becomes fully operational in July 2020, UH community astronomers will be major users of the telescope while doing pioneering solar research.
UH Maui College was also awarded a $20-million grant from the National Science Foundation, to engage Native Hawaiian students to pursue careers in science, technology, engineering and math (STEM). The Akeakamai I Ka Lā Hiki Ola: Scientific Exploration Beneath the Life-Bringing Sun program will incorporate traditional cultural practices within its curriculum. The grant awards the program $2 million each year over the course of a decade. Part of the funding will go toward financial aid and paid internships for Native Hawaiians.
While the 4-meter solar telescope isn’t set to be completed until June, scientists will continue preliminary tests by making observations of the Sun in the coming months. But pointing a telescope directly at the scalding sphere comes with challenges. The Sun’s sweltering surface temperature is about 6,000 degrees Celsius. A specialized cooling system is in place to protect DKIST from massive amounts of heat.
“The focus of the telescope mirror is hot enough to melt metal within a short time. To deal with these heat problems we make the equivalent of a swimming pool full of ice every night to provide cooling for the optics and structure during the day,” said Inouye Solar Telescope Director Thomas Rimmele. More than 7 miles of piping will distribute coolant throughout the observatory.
The state-of-the-art telescope was renamed in honor of the late Sen. Daniel K. Inouye, a strong supporter of STEM education.