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George Mason U. professor finds direction of local interstellar magnetic field (Forwarded)
Media Relations
George Mason University Media Contact: Tara Laskowski, 703-993-8815 05/11/2007 MASON PROFESSOR FINDS DIRECTION OF MAGNETIC FIELD Merav Opher's model suggests that our solar system's shape is asymmetric FAIRFAX, Va. -- Merav Opher, assistant professor of physics and astronomy at George Mason University, and her colleagues Ed Stone of the California Institute of Technology and Tamas Gombosi from the University of Michigan recently published a paper in Science magazine that suggests the direction of the local interstellar magnetic field, located just outside of our solar system. The paper, "The Orientation of the Local Interstellar Magnetic Field," uses data sets gathered from the Voyager spacecrafts, which recently crossed the termination shock at the edge of the solar system after having been launched in 1977. Up to now, scientists have believed that the magnetic field outside of our solar system was parallel to the galactic plane. But Opher, Stone and Gombosi used two data sets to conclude that the magnetic field is actually 60-90 degrees perpendicular to the plane. Their data also strongly suggests that the solar system is asymmetric. While scientists thought the northern and southern hemispheres would be similar, Opher's team has found that the southern hemisphere is more compressed due to the pull of the magnetic field. Even the eastern and western hemispheres don't look the same, giving our solar system more of a bullet shape. "Scientists have often looked at the larger scale magnetic fields of the galaxy. The work we are doing is on a much smaller scale, looking just beyond our solar system. It is like looking at our backyard and opposed to looking at the country," says Opher. "For the first time we know what the local magnetic field looks like, and astronomers will be very excited about this." Opher is the only female scientist -- and by far one of the youngest scientists -- working to calculate the flow of particles and magnetic fields at the edge of the solar system. Many millions of miles past Pluto, the solar wind of our sun begins to lose its dominance when it comes into contact with the interstellar wind from the rest of our galaxy. Scientists consider the place where the two winds meet -- called the heliopause -- as the edge of our solar system. Opher analyzed radio emissions from the heliopause and the streaming direction of ions from the termination shock, which is the area where the million-mile-per-hour solar wind slows to about 250,000 miles per hour. Their work suggests that the field orientation of the local magnetic field differs from that of a larger scale interstellar magnetic field thought to parallel the galactic plane. This conclusion will have an enormous impact on the way physicists and astronomers measure the physics and properties of the areas beyond our solar system. About George Mason University George Mason University, located in the heart of Northern Virginia's technology corridor near Washington, D.C., is an innovative, entrepreneurial institution with national distinction in a range of academic fields. With strong undergraduate and graduate degree programs in engineering, information technology, biotechnology and health care, Mason prepares its alumni to succeed in the workforce and meet the needs of the region and the world. Mason professors conduct groundbreaking research in areas such as cancer, climate change, information technology and the biosciences, and Mason's Center for the Arts brings world-renowned artists, musicians and actors to its stage. Its School of Law is recognized by U.S. News and World Report as one of the top 50 law schools in the United States. |
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