Moving To The Rhythm Of The Sun

Friday, August 17, 2007

Ulysses This artist's impression shows the ESA/NASA Ulysses spacecraft. Launched in 1990, the European-built spacecraft visits both polar regions once every 6.2 years as it circles the Sun in an orbit that is almost perpendicular to the ecliptic, the plane in which Earth and the planets move. Credits: ESA

Using highly sophisticated statistical techniques, Thomson and colleagues have discovered these same, distinct tones emitted by the Sun, in seismic data here on Earth. They have also found that Earth’s magnetic field and atmosphere, and even voltages induced on ocean cables, are all taking part in this cosmic sing-along.

Although these tones are all around us, it would not be possible for us to hear them, even if we listened very closely. Their pitch is too low for the human ear, typically 100-5000 microHertz (1 microHertz corresponds to 1 vibration every 278 hours). This is more than 12 octaves below the lowest note audible to humans. For comparison, the note to which orchestras tune their instruments (A above Middle C on a piano) corresponds to 440 Hertz.

According to Thomson, data from Ulysses provided an important clue as to how these sounds generated deep inside the Sun reach the Earth.

The same techniques applied to the terrestrial data sets were first used on measurements of energetic particle fluxes and interplanetary magnetic fields recorded on board Ulysses.

Surprisingly, rather than being random in nature, the fluctuations in the data were made up of many discrete frequencies or tones, similar to the terrestrial data. These tones also corresponded well to those that theorists predict, should be generated by pressure and gravity waves in the Sun.

Some of these so-called solar oscillations had been observed optically using instruments on SOHO, and by dedicated networks of telescopes on the Earth. They are caused by pressure waves in the Sun, and are referred to as p-modes. The deeper sounds associated with the Sun’s gravity waves (g-modes) are far more elusive.

Just as seismologists on Earth use sound waves to probe the interior of our world, solar scientists would like to use g-modes to probe the core of the Sun, if only they could detect them. G-modes have been undetectable optically, so Thomson and colleagues’ evidence for them in interplanetary data was both unexpected and hard to explain at first.

They examined a wide range of data sets covering natural phenomena and technological systems in fields as diverse as telecommunications and seismology and continued to find new evidence of discrete tones with characteristics of solar oscillations in what was previously considered background “noise”. This added to the puzzle posed by the Ulysses findings.

Thomson believes that the key to the problem is magnetism. He suggests that the g-mode vibrations are picked up by the magnetic field at the Sun’s surface. Part of this magnetic field is then carried away from Sun into interplanetary space by solar wind, where it can be detected by space probes like Ulysses.

The magnetic field of the solar wind in turn interacts with the Earth’s magnetic field and causes it to vibrate in sympathy, retaining the characteristic g-mode signals. The motions of the geomagnetic field then couple into the solid Earth to produce small, but easily detectable, responses as Earth, with many of its technological systems, moves to the rhythm of the Sun.

Source: ESA