Solar wind output at a 50 year low, indicates new data

Washington, September 24 : Data from the Ulysses spacecraft, a joint NASA-European Space Agency mission, has shown that the sun has reduced its output of solar wind to the lowest levels in 50 years.

The sun's solar wind plasma is a stream of charged particles ejected from the sun's upper atmosphere.

The solar wind interacts with every planet in our solar system. It also defines the border between our solar system and interstellar space.

This border, called the heliopause, is a bubble-shaped boundary surrounding our solar system where the solar wind's strength is no longer great enough to push back the wind of other stars.

The region around the heliopause also acts as a shield for our solar system, warding off a significant portion of the cosmic rays outside the galaxy.

The data from the Ulysses spacecraft suggests that the sun's current state could reduce the natural shielding that envelops our solar system.

"The sun's million mile-per-hour solar wind inflates a protective bubble, or heliosphere, around the solar system. It influences how things work here on Earth and even out at the boundary of our solar system where it meets the galaxy," said Dave McComas, Ulysses' solar wind instrument principal investigator and senior executive director at the Southwest Research Institute in San Antonio, Texas.

"Ulysses data indicate the solar wind's global pressure is the lowest we have seen since the beginning of the space age," he added.

According to Ed Smith, NASA's Ulysses project scientist at the Jet Propulsion Laboratory in Pasadena, California, "Galactic cosmic rays carry with them radiation from other parts of our galaxy."

"With the solar wind at an all-time low, there is an excellent chance the heliosphere will diminish in size and strength. If that occurs, more galactic cosmic rays will make it into the inner part of our solar system," he added.

In 2007, Ulysses made its third rapid scan of the solar wind and magnetic field from the sun's south to North Pole.

When the results were compared with observations from the previous solar cycle, the strength of the solar wind pressure and the magnetic field embedded in the solar wind were found to have decreased by 20 percent.

The field strength near the spacecraft has decreased by 36 percent.

"The sun cycles between periods of great activity and lesser activity," Smith said. "Right now, we are in a period of minimal activity that has stretched on longer than anyone anticipated," he added.

ANI