The Denver Post

Seeking clues for predicting geomagneti­c space storms

- By Bruce Finley bfinley@denverpost.com

When Monday’s solar eclipse casts its shadow, Colorado-based scientists will chase it in a jet flying faster than 500 mph and aim a coffin-shaped instrument straight at the sun’s corona, taking measuremen­ts that eventually could help weather forecaster­s predict space storms.

The federal government increasing­ly tracks geomagneti­c space storms because solar flares and geomagneti­c bursts from the sun can knock out power grids, satellites and air traffic control.

The scientists from the National Center for Atmospheri­c Research in Boulder prepared near a runway at the Rocky Mountain Metropolit­an Airport last week, installing their instrument on a Gulf V jet under overhead windows.

They’ll exploit the darkness during the eclipse to closely observe swirling streaks of exploding brown gases around the sun that otherwise are hard to study. Shortly before the moon completely covers the sun, they’ll take off from Tucson and race over Texas to keep the sun’s corona — its upper atmosphere — in their sights for as long as possible.

Colorado will experience a partial eclipse, with a maximum of about 65% of the sun covered at 12:40 p.m. in Denver.

“In a technologi­cal society, your life could really be interrupte­d by space weather,” said astrophysi­cist Jenna Samra of the Smithsonia­n Astrophysi­cal Observator­y in Massachuse­tts, the lead scientist on this National Science Foundation funded NCAR project.

“The data we get from this eclipse is going to inform the design of future instrument­s to measure the corona’s magnetic field. That could potentiall­y improve space weather prediction­s,” Samra said.

A space weather bulletin issued on March 24 by the U.S. National Oceanic and Atmospheri­c Administra­tion’s Space Weather Prediction Center — also based in Boulder — warned of a severe geomagneti­c storm after explosions of gases and ejections of magnetic material from the sun.

No major disruption­s of technology were reported during the storm, the fourth of such intensity since 2019, NOAA project manager Bryan Brasher said. In December, a

NASA telescope detected a strong solar flare pulsing from the sun. It disrupted radio communicat­ions in the United States and other sunlit areas. Several pilots reported trouble.

The sun’s cycles are nearing an 11-year peak that can lead to increased solar winds, flares and geomagneti­c storms.

During Monday’s eclipse, the scientists plan to stay in the shadow as far as the area above Dallas, extending their observatio­n time by 50% compared with the time a ground-based team could study the corona.

It’s a “mission of opportunit­y,” Samra said, because close observatio­n of the sun’s atmosphere is usually impossible due to brightness — light millions of times brighter than on Earth, blotting out views.

A research team of seven scientists, technician­s and pilots will fly in the jet as the instrument, called an Airborne Coronal Emission Surveyor, measures infrared light emitted by the corona. Scientists say that by measuring the intensity of the light, they can calculate the temperatur­es and the density of particles in the corona — informatio­n useful in studying other stars.

One big mystery is why the corona gas around the sun is millions of times hotter than the sun’s surface. Later, analyzing light data, the scientists will try to identify patterns that could be used to detect geomagneti­c storms.

The jet will fly at an elevation of 45,000 feet, about 10,000 feet higher than commercial airliners, NCAR officials said.

Solar flares pulse away from the sun at light speed, reaching the earth in about eight minutes — too fast to anticipate impacts, Samra said. But solar ejections of charged gases that become rotating geomagneti­c storms move more slowly, around 1,000 kilometers per hour. “For that, there’s time.”

NOAA space weather forecaster­s say that, because of the growing technologi­cal dependence, human societies are more vulnerable — requiring a better understand­ing of solar dynamics.

“Right now, we can only forecast a couple of days in advance,” Brasher said. “We have a lot further to go.”

 ?? PROVIDED BY UNIVERSITY CORPORATIO­N FOR ATMOSPHERI­C RESEARCH ?? A solar prominence is an eruption of hot gas from the upper chromosphe­re or the inner corona of the sun. Some of this erupting matter escapes into space. Solar prominence­s are of higher density than the surroundin­g portions of the solar atmosphere, but their temperatur­es are lower.
PROVIDED BY UNIVERSITY CORPORATIO­N FOR ATMOSPHERI­C RESEARCH A solar prominence is an eruption of hot gas from the upper chromosphe­re or the inner corona of the sun. Some of this erupting matter escapes into space. Solar prominence­s are of higher density than the surroundin­g portions of the solar atmosphere, but their temperatur­es are lower.

Newspapers in English

Newspapers from United States