Scientists map previously undetected particles from edge of solar system

Washington, July 3 : Scientists have mapped the energized particles where the hot solar wind slams into the cold interstellar medium, which were undetected till now, using images captured by NASA's sun-focused Solar Terrestrial Relations Observatory (STEREO) twin spacecraft.

The two STEREO spacecraft were launched in 2006 into Earth's orbit around the sun to obtain stereo pictures of the sun's surface and measure magnetic fields and ion fluxes associated with solar explosions.

From June to October 2007, sensors aboard both STEREO spacecraft detected energetic neutral atoms originating from the same spot in the sky, where the sun plunges through the interstellar medium.

According to Dr. Robert Lin, professor of physics at the University of California, Berkeley and lead for the suprathermal electron sensor aboard the STEREO spacecraft, mapping the region by means of neutral, or uncharged, atoms instead of light heralds a new kind of astronomy using neutral atoms.

"You can't get a global picture of this region, one of the last unexplored regions of the heliosphere, through normal telescopes," said Lin.

The heliosphere is a bubble in space produced by the solar wind. It stretches from the sun to beyond the orbit of Pluto.

The solar wind streams off the Sun in all directions at great speeds.

Once beyond the orbit of Pluto, this supersonic wind must slow down to meet the gases in the interstellar medium. As the solar wind slows, it changes direction to form a comet-like tail behind the sun.

This subsonic flow region is called the heliosheath.

The results clear up a discrepancy in the amount of energy dumped into space by the decelerating solar wind.

The solar wind was detected when Voyager 2 entered the heliosheath.

Researchers determined that the newly discovered population of ions in the heliosheath contains about 70 percent of the dissipated energy from the solar wind, exactly the amount unaccounted for by Voyager 2's instruments.

The Berkeley team concluded that these energetic neutral atoms were originally ions heated up in the termination shock area that lost their charge to cold atoms in the interstellar medium and, no longer hindered by magnetic fields, flowed back toward the sun and into the sensors aboard STEREO.

"This is the first mapping of energetic neutral particles from the edge of the heliosphere," said Lin.

According to Lin, the neutral atoms are probably hydrogen, which comprise most of the particles in the local interstellar medium.

NASA plans to launch the Interstellar Boundary Explorer, or IBEX, later this year to more thoroughly map the boundary of the solar system.

ANI