Solar Physicist Says Weak Sun Produces Record Solar Outburst

"The odd thing about this outburst was that the Sun is supposed to be at the minimum phase of its 11-year cycle," said Gary. "Nevertheless, the disruption lasted more than an hour, produced a record amount of radio noise, and caused massive disruptions of Global Positioning Satellite (GPS) receivers world wide."

Since 1997, Gary has directed Owens Valley Solar Array (OVSA), one of the world's leading research facilities to study the sun's impact upon earth. Using special instruments, Gary and researchers at NJIT's Center for Solar-Terrestial Research study solar outbursts. The National Science Foundation and NASA support the work.

A complex sunspot on the Sun was responsible for the outburst, which occurred Dec. 6, 2006 at 3:45 p.m. EST, said Gary. Before the outburst, the radio output of the Sun in the GPS broadcasting band was 54 on the scale of solar flux units. During the outburst, associated with a large solar flare, the radio noise reached around 1 million solar flux units, according OVSA instruments.

"This reading is more than 10 times the previous record, and calls into question scientists' assumptions of the extent to which the Sun can interfere with GPS and wireless communications," Gary said. "OVSA's results are especially useful because they monitor the same right-hand circular polarization that the GPS satellites use for broad-casts. Most other radio instruments measure total intensity rather than circular polarization, which undercounts the noise effect on GPS signals."

The recognition of the record-setting nature of the burst was delayed because the US Air Force Radio Solar Telescope Network (RSTN) reported lower numbers--13,000 solar flux units. But after OVSA researchers triple-checked their figures, it appeared that NJIT's group was correct. Cornell University researchers later independently confirmed OVSA findings.

"The Cornell researchers gave us indirect evidence of a burst at least 10 times the strength reported by RSTN," said Gary. "Eventually we learned," he added, "that the RSTN report pertained only to the beginning of the burst, and the recording was stopped early due to a software error. At the same time, additional quantitative reports of effects on GPS receivers also point to a burst up to 1 million solar flux units."

"When colleagues elsewhere, learned of the burst and saw the OVSA numbers, they just said, 'Wow,'" said Gary. Gary expects to see more important results emerge from the data. "Early examination of the data taken during the burst, ought to provide a gold-mine of scientific information about how the Sun produces such amazing events," Gary said. "Ultimately we hope to understand these bursts well enough to predict them and their effect on wireless systems on Earth."

Before arriving at NJIT, Gary was a research associate in astrophysics at Caltech for 15 years. He is the author of more than 100 peer-reviewed articles. Gary received his BS in physics from the University of Michigan and his PhD in astro-geophysics from the University of Colorado.

OVSA, located in Big Pine, California, http://www.ovsa.njit.edu/ receives more than $750,000 in annual funding from NSF and NASA to study the Sun's radio emission. Current research interests focus on developing a new radio facility, the Frequency Agile Solar Radiotelescope, studying solar flares, and studying the effects of solar radio emission on wireless systems on Earth. OVSA began operations in 1991, although various forerunner instruments have been in operation since 1980. Under the direction of Gary, a leader in solar radio physics, the facility has been has been expanded and operated by NJIT since 1997.