Why explore the magnetosphere? One compelling reason is that doing so helps us understand phenomena in the more distant universe, in particular the intricate web of plasma phenomena, magnetic fields and particle acceleration.|
But there also exists a practical angle: in a world increasingly dependent on electricity and electronics, the "space weather" outside the atmosphere can have serious effects, in particular on human communications.
Currently more than 200 communication satellites circle the Earth in synchronous orbit. A large magnetic storm can greatly increase the number of fast ions and electrons which hit those satellites; such ions and electrons are similar to the ones emitted by radioactive substances and can create serious problems.
The simplest effect is an electric charge on the satellite, usually negative, raising its voltage to hundreds or even thousands of volts. Charging by itself has little effect on the satellite's operation, although on a scientific satellite it would seriously distort observations (if the satellite is charged to, say, -500 volts, electrons with less energy than 500 electron-volts are repelled and cannot be detected). However, if different parts of the satellite are charged to different voltages, the current between them can cause damage.
Particles with higher energy can permanently degrade solar cells. Also, high-energy particles can penetrate the circuitry and cause either damage or false signals which lead to unintended responses by the satellite. All these have occured in the past.|
Another effect of magnetic storms (and to lesser extent, of substorms) is a greater intensity of the electric currents circulating between Earth and distant space. As already noted, these currents are associated with the polar aurora, and they flow from space into the auroral zone or the other way around. In big storms, not only is the magnetic disturbance more intense, but it also spreads further equatorwards, into more densely populated areas. For instance, in the picture on the right, taken from space during a storm in March 1989, aurora blankets the northern states of the US as well as southern Canada
This disturbance also induces extra currents in the wires of the electrical power grid, creating a temporary overload. Serious overloads of this type can trigger circuit breakers and thus cause widespread "power blackouts," and on occasion they have even destroyed power transformers.|
For these reasons, conditions at the Sun, in interplanetary space and in the magnetosphere are closely watched. The Space Environment Center in Boulder, Colorado, maintained by of the National Oceanic and Atmospheric Administration (NOAA), has a Space Weather Operation facility which constantly tracks the "weather" in space.
This is done in several ways. NOAA satellites of the GOES series, in synchronous orbit, observe the local radiation environment and also monitor the Sun's x-rays, which come from the corona and increase at active times. Telescopes on Earth observe the Sun through special filters and in special wavelength (e.g. x-rays), all of which highlight active features. For a view of NOAA's "space weather report," click here; another such report, from the University of Michigan, is linked here.
In an interesting development, the recent SOHO spacecraft, currently at the L1 Lagrangian point, allows scientists to detect (by special processing of its images) coronal mass ejections, not just in a sideways view but even when they are headed straight for Earth. A CME noted in this way on January 6, 1997, arrived as predicted on the 10th-11th and caused a widespread disturbance. Another such event occured April 7-11, 1997.
Of course, the sideways view of CMEs contains additional information, and NASA's planned solar missions include STEREO (Solar Terrestrial Relations Observatory), with a pair of well-separated solar observatories, to get a stereoscopic view of such eruptions. One spacecraft would orbit near Earth, the other would be stationed elsewhere in the Earth's orbit around the Sun, capturing a sideways view of solar eruptions. So far there is unfortunately no sure way of predicting whether the direction of the magnetic field carried by an erupting solar plasma would slant northwards or southwards, an important factor in predicting "space weather." Closer to Earth, spacecraft near the L1 point such as SOHO and WIND, and since August 1997 also ACE, intercept shocks and plasma clouds up to one hour before their arrival at Earth and serve as early warning stations.
An obvious question is whether the high energy particles produced by such events constitute a hazard not just for spacecraft but also for astronauts. So far no astronauts have been seriously exposed, not even those on the Russian space station "Mir" whose inclined orbit extends to fairly high latitudes, closer to the auroral zone than the planned orbit of the International Space Station planned by NASA. Nothing in space can be guaranteed, however, and re-entry modules for quick escape into the protecting atmosphere have been studied.
On Sunspots, Solar Eruptions, and the big storm of 13 March 1989
Tutorial exposition on Space Weather, from the Rice University web site
"Storms in Space: A Fictionalized Account of 'The Big One'," John W. Freeman, Jr., Eos, Transaction of American Geophysical Union 6 September, 1994.
"Geomagnetic Storm Forecasts and the Power Industry," by John G. Kappenman, Lawrence J. Zanetti and William A. Radasky,Eos, Transaction of American Geophysical Union 28 January, 1997.
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Last updated March 13, 1999