Motors whirred as a gleaming white dome slowly opened, allowing one of the premier solar telescopes in the world to track the magnetic fields and exploding flares of the sun. In a few hours, computers would translate that data into detailed video and pictures of the sun's turbulent surface. Images captured weeks earlier already were shown on the monitors in a darkened control room at the Big Bear Solar Observatory. They revealed mysterious displays of dancing and flashing lights hovering between bubbles of solar plasma.
John Varsik, a research astronomer at the observatory perched high up in California's San Bernardino Mountains, allowed a boyish grin to spread across his face. These lights "will be the focus of future research for years to come," he said.
But Varsik, 57, will probably not be leading that research. The $6 million telescope completed in 2009 is already being eclipsed by a much bigger solar telescope under construction in Hawaii. Over the next five years, it will gradually shift to a new primary mission: operating as a test bed for technology destined to be used elsewhere.
Around the country, many older solar telescopes are being shut down to pay for a new generation of space-based observatories and the $360 million facility under construction atop Maui's Haleakala Crater.
"In solar astronomy, as well as other areas of science, the cost of doing business has gone way up," said Dale Gary, a solar physicist and director of the Big Bear telescope. "The only way to make that work is to shut down smaller operations or change their missions."
With a 1.6-meter primary mirror, the Big Bear Solar Observatory is — for now — at the forefront of solar astronomy.
At the heart of its main telescope system is a computer-driven mirror that corrects the distortions caused by atmospheric turbulence due to moisture, wind or thin clouds. The surface of the 4-inch mirror is continually warped by 357 tiny computer-controlled pistons that create deformations about 1/50th the width of a human hair, said Nicolas Gorceix, an optical engineer at the observatory.
Among the Big Bear scientists' recent discoveries are the first detailed observations of "umbral spikes," the clusters of long, cone-shaped filaments that appear in the darkest portion of sunspots, where magnetic fields are strongest. Spectral analysis of these filaments, which exist for only two to three minutes, suggests they are blasts of plasma along narrow magnetic tubes.