Ballooning for Cosmic Rays
Astronomers have long thought that supernovas are
the source of cosmic rays, but there's a troubling discrepancy
between theory and measurements. An ongoing balloon flight over
Antarctica could shed new light on the mystery.
January 12, 2001 -- Hold out your hand for 10 seconds. A dozen electrons and muons just zipped unfelt through your palm. The ghostly particles are what scientists call "secondary cosmic rays" -- subatomic debris from collisions between molecules high in Earth's atmosphere and high-energy cosmic rays from outer space.
Cosmic rays are atomic nuclei and electrons that streak through the Galaxy at nearly the speed of light. The Milky Way is permeated with them. Fortunately, our planet's magnetosphere and atmosphere protects us from most cosmic rays. Even so, the most powerful ones, which can carry a billion times more energy than particles created inside atomic accelerators on Earth, produce large showers of secondary particles in the atmosphere that can reach our planet's surface. [more]
Above: Supernova explosions, like the one that created the expanding Crab Nebula (pictured), may be the source of galactic cosmic rays.
Where do cosmic rays come from? Scientists have been trying to answer that question since 1912, when Victor Hess discovered the mysterious particles during a high altitude balloon flight over Europe. Galactic cosmic rays shower our planet from all directions. There's no definite source astronomers can pinpoint, although there is a popular candidate.
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"It takes an awful lot of power to maintain the galactic population of cosmic rays," says Adams. "Cosmic rays that lose their energy or leak out of the Galaxy have to be replenished. Supernovae can do the job, but only if one goes off every 50 years or so." The actual supernova rate is unknown. Observers estimate that one supernova explodes somewhere in the Galaxy every 10 to 100 years -- just enough to satisfy the energy needs of cosmic rays.
But there could be a problem with the supernova theory, says Adams.
"A supernova blast blows a bubble in the interstellar medium that grows until the shock wave runs out of energy," he explained. "They can accelerate particles up to some point, about 1014electron volts (eV) per nucleon, but not beyond that. Below an energy of 1014 eV, all of the different cosmic ray species -- protons, helium nuclei, etc. -- should have the same kind of energy spectrum: a power law with index around -2.7."
A "power law" spectrum is one that looks like a straight line on a piece of log-log graph paper. In the energy range ~1010 eV to 1014 eV, the supernova theory of cosmic ray acceleration predicts that the power law spectrum of protons should have the same slope as the power law spectra of heavier nuclei (about -2.7).
The problem is when scientists compare the energy spectra of protons and helium nuclei, the two don't resemble one another as much as they should. Both are power laws, as expected, but "existing data indicate a possible spectral index difference between protons and helium of about 0.1," says Eun-Suk Seo, a cosmic ray researcher at the University of Maryland. "The [slope of the] proton spectrum is close to -2.7, but the energy spectra of helium and heavier nuclei seem to be flatter. The difference is small and it might not be statistically significant." If there is a genuine discrepancy, she added, it could signal trouble for supernova models of cosmic ray acceleration.
To find out if the supernova theory is indeed in peril, a team of scientists led by John Wefel ( Louisiana State University) and Eun-Suk Seo, and aided by personnel from the National Science Balloon Facility, launched a helium-filled balloon from McMurdo, Antarctica on Dec. 28, 2000. The payload, which is now 120,000 feet above Earth's surface, includes a NASA-funded cosmic ray spectrometer known by its builders as the Advanced Thin Ionization Calorimeter or "ATIC" for short.
"ATIC is sensitive to cosmic rays with energies between ~1010eV and 1014eV," says Wefel. By covering such a wide range of energies with a single modern spectrometer, the team hopes to measure the proton and helium cosmic ray spectra with better precision than ever before.National Science Balloon Facility. The ATIC experiment lifted off on its circumpolar trip to measure Galactic cosmic rays on Dec. 28, 2000.
"The higher energy cosmic rays are rare," he continued. "For example, each day ATIC collects no more than ~10 cosmic rays with energies exceeding 1013 eV. That's why we have to fly the balloon for such a long time, to gather enough particles for a statistically significant result." By the time ATIC lands on January 12th or 13th, the spectrometer will have been in the stratosphere counting cosmic rays for nearly two full weeks.
The long flight time, more than any other reason, is why the researchers chose to fly the balloon over Antarctica. "We would be happy to fly this payload over North America," says Adams. "The problem is that we need the spectrometer to be aloft for a long time. Antarctica has two advantages: It's international territory, so we don't need to apply for lots of overflight permissions, and the Antarctic Vortex (a circulating weather system around the south pole) keeps the balloon confined to airspace over the continent."
"If there is a difference between the proton and the helium spectra -- and that's not certain, by the way -- it won't necessarily kill the supernova model," continued Wefel. "But a discrepancy would cause problems." Theorists may have to consider the progress of supernova shock fronts in greater detail. "Every supernova explosion is an individual work of art," says Adams. "We use mathematical models that assume the explosions are spherical, but they are not. Within the blast wave itself you can see irregularities. There are bright knots, for example, where shock waves run into interstellar clouds. In crowded groups of massive stars ('OB associations') where supernovae can occur in quick succession, blast waves collide with other blast waves." It can get a little messy! Modeling such details might affect any necessary reconciliation between the theory and the data.
Above: The ATIC balloon payload. Click on the image to find out how the Advanced Thin Ionization Calorimeter works.
And what if the supernova model can't be rescued? "There are other possibilities," says Wefel, "but not a lot of good ones. We'll really have to look hard to find something other than supernovae that can meet the cosmic ray energy requirement."
The analysis team led by Eun-Suk Seo is eager to sift through ATIC's data files after the balloon lands. The new particle counts, which the experimenters hope will be the most accurate to date in ATIC's energy range, could shed new light on the decades-old mystery of cosmic rays.
Visit the ATIC home page for status
reports about the ongoing balloon flight. Participants
in the ATIC project include Louisiana State University, the University
of Maryland, NASA, the Naval Research Laboratory, Southern University
(Baton Rouge), the National Science Foundation, and collaborators
from Germany, Korea and Russia.
ATIC video -a collection of movies about the ATIC project
Cosmic Ray Classroom Activities -from the ATIC team at LSU
Cosmic Rays, what are they? - from NASA Goddard's "Imagine the Universe"
NASA's Scientific Ballooning Program - supported the launch, flight and recovery of ATIC.
Supernovae and Supernova Remnants - a tutorial from Harvard's Chandra Science Center "X-ray Astronomy Field Guide"
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