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Kinks in Sun's Waves Unraveled
Kinks in Sun's Waves Unraveled
28 Mar 2001
(Source: Jet Propulsion Laboratory)

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Kinks in the Sun's magnetic field have puzzled scientists since they first started studying the solar wind, and now researchers at NASA's Jet Propulsion Laboratory, Pasadena, Calif., have found the reason: they are caused by the evolution of a type of magnetic wave called Alfven waves.

Scientists measured sudden changes in the Sun's magnetic field with the magnetometer instrument on the Ulysses spacecraft, which is orbiting the Sun's poles at a distance between Jupiter and Mars. Ulysses has been studying the Sun since 1990 and has just finished studying the south pole of the Sun at solar maximum, a time of great activity.

"Over the poles of the Sun, we saw abrupt decreases in the magnetic field," said JPL's Dr. Bruce Tsurutani, a co- investigator on the magnetometer instrument on Ulysses. "We did not know what they were, because we had never seen anything like it before. Now we know that the disturbance is caused by Alfven waves."

Scientists expected to find that either the field magnitude remained the same, though the angle changed, or that the magnitude changed, with no fields threading across the structure, said Tsurutani. Instead, they found that the ends of Alfven waves always have both rotational and tangential characteristics.

Like the movements of a plucked guitar string, Alfven waves travel down the magnetic fields that emanate from the Sun. Disturbances in the Sun's magnetic field, which is embedded in the solar wind, travel through space to eventually cause auroras on Earth. The high-energy particles from the solar wind become trapped in the Earth's magnetic field and come down into the atmosphere near the Earth's north and south magnetic poles. The highly-charged particles then collide with oxygen and nitrogen in Earth's atmosphere and emit light, forming the aurora.

Tsurutani also studied polar plumes, long trails from the base of the Sun. The plumes form in the Sun's polar regions, the upper and lower 30-degree latitude regions, and where these plumes occur, the magnetic field isn't kinked, but instead forms long, thin, straight tubes. This means that the Alfven waves don't operate in these regions, though scientists don't yet know why.

"Ulysses was able to find that the Sun's polar plumes stretch out past the orbit of Mars and maybe farther," said Tsurutani. "What's fascinating is how these plumes can be so thin and so long at the same time." A plume could be 100 times wider than it is long. The European Space Agency's Solar and Heliospheric Observatory (SOHO) noted these polar plumes in 1996.

Alfven waves are named for Hannes Alfven, a Swede who in1942 discovered the waves, for which he was later awarded the Nobel Prize.

Tsurutani discussed his findings this week at the European Geophysical Society's 26th annual meeting, joined by his colleagues on the study, Dr. Carlos Galvan, Dr. John Arballo, Dr. Regina Sakurai and Dr. Daniel Winterhalter, from the Space Plasma Physics Element at JPL, Dr. Bimla Buti University of New Delhi and Dr. Gurbax Lakhina, director of the Mumbai Geomagnetic Observatory, Bombay, India.

Ulysses, launched in 1990, is a joint venture of NASA and the European Space Agency. JPL manages Ulysses for NASA's Office of Space Science, Washington, D.C. More information on the Ulysses mission is available at the JPL Ulysses website: http://ulysses.jpl.nasa.gov/ and ESA's Ulysses website, http://helio.estec.esa.nl/ulysses/. JPL is managed by the California Institute of Technology in Pasadena for NASA.

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Last Updated: 5 Jun 2001