Spacecraft discovers solar winds weakening

This could cause the Sun's heliosphere to shrink in size and strength.Provided by the Jet Propulsion Laboratory, Pasadena, California
By | Published: September 24, 2008 | Last updated on May 18, 2023
Sun's heliosphere
This artist’s impression shows the Sun’s heliosphere.
NASA/Goddard Space Flight Center Conceptual Image Lab
September 24, 2008
Data from the Ulysses spacecraft, a joint NASA-European Space Agency mission, show the Sun has reduced its output of solar wind to the lowest levels since accurate readings became available. 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,” says Dave McComas, Ulysses’ solar wind instrument principal investigator and senior executive director at the Southwest Research Institute in San Antonio. “Ulysses data indicate the solar wind’s global pressure is the lowest we have seen since the beginning of the space age.”

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.

“Galactic cosmic rays carry with them radiation from other parts of our galaxy,” says Ed Smith, NASA’s Ulysses project scientist at the Jet Propulsion Laboratory in Pasadena, California. “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.”

Galactic cosmic rays are of great interest to NASA. Cosmic rays are linked to engineering decisions for unmanned interplanetary spacecraft and exposure limits for astronauts traveling beyond low-Earth orbit.

In 2007, Ulysses made its third rapid scan of the solar wind and magnetic field from the Sun’s south pole to the 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 was 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 says. “Right now, we are in a period of minimal activity that has stretched on longer than anyone anticipated.”

Ulysses was the first mission to survey the space environment over the Sun’s poles. Data from Ulysses have forever changed the way scientists view our star and its effects. The venerable spacecraft has lasted more than 17 years, or almost four times its expected mission lifetime.

The Ulysses solar wind findings were published in a recent edition of Geophysical Research Letters.

The Ulysses spacecraft was carried into Earth orbit aboard space shuttle Discovery on October 6, 1990. From Earth orbit it was propelled toward Jupiter, passing the planet on February 8, 1992. Jupiter’s immense gravity bent the spacecraft’s flight path downward and away from the plane of the planets’ orbits. This placed Ulysses into a final orbit around the Sun that would take it over the north and south poles.