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Solar Tantrums Could Last Two More Years, Space Telescopes Feeling the Pain
By Robert Roy Britt
Senior Science Writer
posted: 07:00 am ET
15 December 2000

History paints a stormy future

The last solar cycle officially peaked in July 1989, as measured by the number of monthly sunspots. But a second, only slightly less active peak came four months later. And the worst space storms from that cycle came after the main peak -- in November 1989, and even into July 1991.

Smooth Sunspot Number

Averaging 13 months of data generates a "smoothed" figure for each month. The past six solar maximums are shown in grey. April 2000 is a possible peak, but researchers won't know for many months. The most recent figures available are for May.

Apr 1937
119.2
May 1947
151.8
Mar 1958
201.3
Nov 1968
110.6
Dec 1979
164.5
Jul 1989
158.5
Apr 2000
120.7
May 2000
118.9

SPACE.COM GRAPHIC
SOURCE: NOAA

All about space weather

Will we stay on a plateau for two years, like the last cycle, or has a slow decline already begun?

"No good answer," Murtagh said. "We certainly do expect several active periods in the next two years."

While this solar maximum has not been an historical whopper, it's no slouch. Two radiation storms this year were the third and fourth most severe since 1975. And a geomagnetic storm on July 15 was the worst since 1991. Geomagnetic storms arrive later than radiation storms, last longer and fuel the colorful lights known as auroras.

But major problems have not come, as they did in 1989 when a solar storm triggered a power surge that damaged a transformer at Hydro-Quebec, leaving 6 million people in Canada and the northeastern United States without power for more than nine hours. The current cycle has caused no more than some relatively minor radio blackouts and a few small satellite problems.

Satellites: Weathering the storms

Engineers design satellites to handle space weather. They know that heavy doses of radiation can fry an expensive electronic camera or disable navigational equipment.

The Barrage

Radiation levels on the XMM's EPIC MOS cameras for each orbit during the past few months. Main peaks correspond to the solar flare outbursts of July 14, September 13 and November 8. Orbit number is shown at bottom of graph. Click to enlarge

SOURCE: ESA/XMM

Unexpected Protons

Proton impacts imaged by an XMM camera. Click to enlarge

SOURCE: Leicester University Space Research Center


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But space can be a tricky place, and there's a lot going on up there that is still a mystery. Just ask the scientists who operate the XMM-Newton.

Twice on each orbit, both XMM and Chandra cross Earth's radiation belts, which extend out from the planet some 25,000 miles (40,000 kilometers). In this danger zone, charged particles -- essentially protons and electrons -- are trapped by Earth's magnetic field. Engineers planned for this, and forecasters can predict the arrival of major space storms that heighten the danger. Sensitive instruments on the spacecraft are shut down.

But more minor and mysterious waves of radiation, not confined the radiation belts, have buffeted the craft without warning -- and so far have stumped researchers.

In one gust, a sheet or cloud of protons, estimated to be 6 miles (10 kilometers) thick, pounded the telescope with 300 impacts per square centimeter (0.16 square inch) every second for fifteen seconds. The mysterious brief gusts are made of protons that pack less of a punch than larger, more predictable bouts of space weather.

"It is like trying to predict a gust of wind in a specific place at a specific time," said Fabio Giannini of the European Space Agency (ESA). "It appears that the Earth's magnetic field can concentrate these low-energy particles."

Next page: Naked cameras

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