Press Release

Ulysses spacecraft observes surprising reach of solar activity

By SpaceRef Editor
August 9, 2001
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Once every 11 years, the sun’s magnetic field flips over. During the
commotion that accompanies these field reversals, large solar flares send
great geysers of hot gas and huge quantities of charged particles erupting
from the surface and streaming into space during a period called “solar
maximum.”

New data collected by University of Chicago scientists via the Ulysses space
probe shows that there is no escaping the pervasive influence of these
potentially harmful charged particles, not even at the seldom-visited high
solar latitudes.

“What we found, which I think nobody really expected, is the widespread
distribution of particles accelerated following a single solar flare
basically all the way through the heliosphere,” the region of space dominated
by the sun, said Bruce McKibben, a physicist at the University’s Enrico Fermi
Institute.

Solar flares — sudden local brightenings on the sun’s surface — usually
produce X-rays and radio emissions as well as charged particles and gas
eruptions. “The energetic particles following a flare can sometimes increase
the radiation intensity in space to harmful levels, and increased radiation
can linger in the vicinity of Earth in the inner heliosophere for days,
weeks, or even as much as a month after a large flare,” McKibben explained.

Scientists had expected to find that the sun’s magnetic field lines, which
are stretched out into space by the solar wind, would keep charged particles
originating in solar flares near the equator confined to a fairly narrow
band near their origination point. Instead, these particles have mysteriously
migrated to high solar latitudes in a matter of just three or four days,
making radiation levels almost the same over the poles as at the equator.

It thus appears that even at polar latitudes, where only Ulysses has gone
before, spacecraft can be exposed to almost the same solar energetic
particle environment as spacecraft on the plane of the ecliptic, where the
Earth and the planets follow their orbits around the sun. McKibben will
present a paper that describes the rapid and pervasive dissemination of
solar particles Aug. 9 at the 27th International Cosmic Ray Conference in
Hamburg, Germany. The paper will draw on observations from all of the
instruments that are part of the Cosmic and Solar Particles Investigation
(COSPIN) consortium.

McKibben leads the high-energy charged-particle experiment on Ulysses
provided by the COSPIN consortium. The consortium consists of scientific
groups from five nations, each of which provided a detector system covering
specific aspects of the high-energy particle radiation in space. The Pioneer
6 and 7 spacecraft had previously detected evidence of the widespread
distribution of charged particles from the sun in the late 1960s and early
1970s. But the data then were limited to spacecraft orbiting the sun in the
ecliptic plane near the sun’s equator.

“We’ve now extended that into the third dimension,” McKibben said.

Exactly how solar particles travel so rapidly across the magnetic fields of
interplanetary space remains a mystery, McKibben said. “There’s clearly some
mechanism that moves them across magnetic fields much faster than we have
any reason to believe they should. There are ideas but none of them seem
completely adequate, at least to me, and I’m puzzled.”

Last year the sun entered a solar maximum, which scientists expect will last
for up to three or four years. Charged particles released by the sun are
the chief danger during periods of high solar activity, said Cliff Lopate,
another Fermi Institute physicist.

“When the sun becomes active, it can release enormous numbers of charged
particles in extremely brief periods of time,” Lopate said. “Because there
are so many of them, the particles can damage both electronic and biological
systems in space.”

The Earth’s magnetic field shields the International Space Station fairly
well against the sun’s radiation, but “solar maximum would be a bad time
to go to Mars,” McKibben said. “It appears that you can get significant
enhancements in radiation exposure anywhere in the solar system following
an event anywhere on the sun.”

The sun’s severe radiation zone extends as far out as the orbit of Jupiter,
“so there’s not very much protection in going away from the sun, either,”
McKibben said.

University of Chicago News Office

5801 South Ellis Avenue – Room 200

Chicago, Illinois 60637-1473

(773) 702-8360 Fax: (773) 702-8324

Contact:

Steve Koppes, (773) 702-8366, s-koppes@uchicago.edu

SpaceRef staff editor.