Five Spacecraft Join to Solve an Auroral Puzzle

TERRADAILY

The configuration of spacecraft and the Earth when the breakthrough was made. On 18 March 2003, NASA's IMAGE was closer to the Earth and observing an aurora that contained a dayside proton auroral spot (bottom left). At the same time, ESA's Cluster quartet then passed overhead returning proton data (top left graph), showing a magnetic reconnection was taking place and that protons were leaking through Earth's magnetic shield. These protons were then being funneled into Earth's atmosphere along magnetic field lines to form the spot." Image credit: Geophysical Research Letters

Washington - May 22, 2003
Five spacecraft have made a remarkable set of observations, leading to a breakthrough in understanding the origin of a peculiar and puzzling type of aurora. Seen as bright spots in Earth's atmosphere and called "dayside proton auroral spots," they are now known to occur when fractures appear in the Earth's magnetic field, allowing particles emitted from the Sun to pass through and collide with molecules in our atmosphere.

On March 18, 2002, a jet of energetic solar protons collided with the Earth's atmosphere and created a bright "spot" seen by NASA's IMAGE spacecraft, just as the European Space Agency's (ESA) four Cluster spacecraft passed overhead and straight through the proton jet.

This is the first time that a precise and direct connection between the proton jet and bright spot has been made, and it results from the simultaneous observations by Cluster and IMAGE.

The results of the study are published May 21 in Geophysical Research Letters, a journal of the American Geophysical Union, in a paper by Tai Phan of the University of California in Berkeley and 24 international colleagues.

Earth's magnetic field acts as a shield, protecting the planet from the constant stream of tiny particles ejected by the Sun, known as the solar wind. The solar wind itself is a stream of hydrogen atoms, separated into their constituent protons and electrons.

When electrons find routes into our atmosphere, they collide with and "excite" the atoms in the air. When these excited atoms release their energy, it is emitted as light, creating the glowing "curtains" we see as the aurora borealis in the far north and aurora australis in the far south. Dayside proton auroral spots are caused by protons "stealing" electrons from the atoms in our atmosphere.

An extensive analysis of the Cluster results has now shown that the region was experiencing a turbulent event known as "magnetic reconnection." Such a phenomenon takes place when the Earth's usually impenetrable magnetic field fractures and has to find a new stable configuration. Until the field mends itself, solar protons leak through the gap and jet into Earth's atmosphere, creating the dayside proton aurora.

Philippe Escoubet, ESA's Cluster Project Scientist, comments, "Thanks to Cluster's observations, scientists can directly and firmly link for the first time a dayside proton auroral spot and a magnetic reconnection event."

Tai Phan, leader of the investigation, now looks forward to a new way of studying the Earth's protective shield. He says, "This result has opened up a new area of research.

We can now watch dayside proton aurorae and use those observations to know where and how the cracks in the magnetic field are formed and how long the cracks remain open. That makes it a powerful tool to study the entry of the solar wind into the Earth's magnetosphere."

Proton auroras were globally imaged for the first time by NASA's IMAGE (Imager for Magnetopause-to-Aurora Global Exploration) spacecraft, which revealed the presence of dayside proton auroral spots.

ESA's Cluster is a collection of four spacecraft, launched on two Russian rockets during the summer of 2000. They fly in formation around the Earth, relaying the most detailed information ever about how the solar wind affects the planet.

The principal investigators for the instruments in the current study were Henri Reme of CESR/Toulouse, France (Cluster Proton Detectors), Andre Balogh of Imperial College, London, United Kingdom (Cluster Magnetic Field Instrument), and Stephen Mende of University of California, Berkeley (IMAGE/FUV).

"Simultaneous Cluster and IMAGE Observations of Cusp Reconnection and Auroral Spot for Northward IMF" Citation: T. Phan, H. U. Frey, S. Frey, L. Peticolas, S. Fuselier, C. Carlson, H. Reme, J.-M. Bosqued, A. Balogh, M. Dunlop, L. Kistler, C. Mouikis, I. Dandouras, J.-A. Sauvaud, S. Mende, J. McFadden, G. Parks, E. Moebius, B. Klecker, G. Paschmann, M. Fujimoto, S. Petrinec, M. F. Marcucci, A. Korth, and R. Lundin, Simultaneous Cluster and IMAGE observations of cusp reconnection and auroral proton spot for northward IMF, Geophys. Res. Lett., 30(10), 1509, doi:10.1029/2003GL016885, 2003.

IRON AND ICE

Chaos Explains Origin Of New Moons

Bristol - May 19, 2003
The ability to understand how small bodies such as moons switch from orbiting the Sun to orbiting a planet has long remained one of the outstanding problems of planetary science. A paper published in Nature on 15 May shows how this problem has been resolved using chaos theory, enabling scientists to predict where astronomers might search for new moons orbiting the giant planets.

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