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Cluster Tunes Into Radio Earth

Artist's conception of the black aurora and its associated electric currents, as observed by the four Cluster spacecraft. Courtesy of the European Space Agency.
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  • Greenbelt - Dec 10, 2001
    Researchers have known for three decades that the Earth is a potent radio transmitter, but they were never able to pinpoint where the noise was coming from. By using data from the four spacecraft of the European Space Agency's Cluster mission, NASA-funded scientists have now precisely located the source of that radio noise along magnetic field lines several thousand miles above bright regions in Earth's northern lights.

    Dr. Robert Mutel, Dr. Donald Gurnett, and colleagues from the University of Iowa have used simultaneous measurements from the quartet of spacecraft to pinpoint the location in space where auroral kilometric radiation (AKR) is emitted. AKR is a form of radio wave with a frequency just below the AM radio band (about 540-550 kilohertz).

    AKR is generated by the movement of high-energy particles through Earth's magnetic field (or magnetosphere) in connection with auroras (the northern and southern lights).

    In preliminary findings, Mutel and colleagues have noted that the most intense AKR emissions seem to occur above the bright spots in the auroral ovals around Earth's polar regions, where high-energy particles slam into the upper atmosphere and create the northern lights.

    Mutel presents his results on December 10 at the Fall Meeting of the American Geophysical Union in San Francisco during a joint press conference with colleagues from ESA.

    Using the Wideband (WBD) Plasma Wave Instruments that they built for Cluster, along with a modified form of the astronomical technique known as very-long baseline interferometry, Mutel and colleagues have been able to detect bursts of radio waves being emitted by electrons sliding down Earth's magnetic field lines toward the auroral zones.

    Researchers proposed in the 1970s that AKR was likely originating about 7,000 to 8,000 miles (11,000 to 13,000 km) above Earth's surface in the magnetosphere, but until now they were not able to make the measurements to confirm the theory.

    "It is only by using independent, simultaneous measurements from multiple spacecraft that we are able to make these sorts of observations," said Dr. Melvyn Goldstein, NASA's project scientist for the Cluster mission. "This research is exactly the sort of thing we were hoping to do with the Cluster mission."

    Though AKR is not detectable from the Earth's surface - the ionosphere blocks most radio waves from space at those frequencies - it is the most important and intense naturally occurring radio emission from Earth. Sounding like sporadic bursts of high-pitched whistles and squawks, AKR is emitted by Earth about one-third to one-half of every day at a signal strength as high as one billion Watts.

    The most potent commercial radio signals on Earth are only 100,000 Watts, meaning that AKR would drown out much of our AM radio signals were it not for the ionosphere (a tenuous layer of electrified gas at the boundary between Earth's atmosphere and space).

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    First Image and Spectrum of a Dark Matter Object
    Paris (ESA) Dec 5, 2001
    Astronomers have observed a Dark Matter object directly for the first time. Images and spectra of a MACHO microlens - a nearby dwarf star that gravitationally focuses light from a star in another galaxy - were taken by the NASA/ESA Hubble Space Telescope and the European Southern Observatory's Very Large Telescope. The result is a strong confirmation of the theory that a large fraction of Dark Matter exists as small, faint stars in galaxies such as our Milky Way.

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