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Improving Space Weather Forecasting By Detecting Active Regions On The Far Side Of The Sun

Date:
April 18, 2000
Source:
American Geophysical Union
Summary:
Scientists have devised a method to detect sunspots on the far side of the Sun, before they rotate toward Earth, potentially causing communications disruptions. They do so by detecting the alpha lyman radiation sunspots produce.

WASHINGTON - Scientists have taken a major step forward in their quest to predict space weather, a term covering various events originating on the Sun that can seriously affect communications and electric power transmission lines on Earth and even modify the orbit of satellites. These solar events are expected to increase this year as the Sun approaches solar maximum in its 11-year cycle of sunspot activity.

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One source of space weather is in fact the sudden increase in sunspot activity, which can potentially change the orbit of satellites. This is caused by increased ultraviolet radiation, which heats Earth's upper atmosphere and changes its density. Large objects like the International Space Station could thereby be moved into new orbits, where they might collide with space debris, whose orbits would also be changing. While all of these orbits can be calculated and satellites maneuvered out of danger, it would clearly help for scientists to have maximum advance knowledge of severe space weather.

Writing in the May 1 issue of Geophysical Research Letters, published by the American Geophysical Union, Jean-Loup Bertaux and colleagues at the Aeronomy Service (Service d'Aeronomie) of France's National Center for Scientific Research (Centre National de la Recherche Scientifique, CNRS) and the Finnish Meteorological Institute (FMI) report a method they have devised of detecting active regions, or sunspots, on the far side of the Sun, before they rotate to its Earthward side. Since the Sun's rotational period is 27 days, this can allow up to two weeks' advance warning of strong solar winds.

The technique, described in the GRL paper, is to make use of Lyman alpha radiation, a spectroscopic line in hydrogen atoms floating freely in space. Although the Sun constantly emits Lyman alpha radiation, its active regions can be thought of as projectors, beaming this radiation in stronger and more concentrated streams. Hydrogen atoms in space then function as screens illuminated in their ultraviolet spectrum by the Lyman alpha radiation.

Lyman alpha is detected by the SWAN (Solar Wind ANisotropies) instrument aboard the SOHO (SOlar Heliospheric Observatory) satellite, which maintains an apparently fixed position between the Earth and the Sun. SWAN scans the whole sky and is thus able to detect strongly illuminated regions of hydrogen atoms in space beyond the far side of the Sun. By tracking the movement of these strongly illuminated regions, scientists can in effect see around the corner and predict when the sunspots producing strong radiation streams will rotate around and face toward the Earth. This will provide more time to take corrective action in advance of heavy solar weather they may produce.

SOHO is a joint mission of ESA and NASA, stationed at 1.5 million kilometers (930,000 miles) from the Earth, near the so-called Lagrange point L1, where the gravity of Earth and Sun balance each other.


Story Source:

The above story is based on materials provided by American Geophysical Union. Note: Materials may be edited for content and length.


Cite This Page:

American Geophysical Union. "Improving Space Weather Forecasting By Detecting Active Regions On The Far Side Of The Sun." ScienceDaily. ScienceDaily, 18 April 2000. <www.sciencedaily.com/releases/2000/04/000417104750.htm>.
American Geophysical Union. (2000, April 18). Improving Space Weather Forecasting By Detecting Active Regions On The Far Side Of The Sun. ScienceDaily. Retrieved January 30, 2015 from www.sciencedaily.com/releases/2000/04/000417104750.htm
American Geophysical Union. "Improving Space Weather Forecasting By Detecting Active Regions On The Far Side Of The Sun." ScienceDaily. www.sciencedaily.com/releases/2000/04/000417104750.htm (accessed January 30, 2015).

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