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Sun in MDI

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Solar Physics

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Space Weather

 

The Sun is the source of the light and heat that enables life to survive on Earth. It is also the source of the 'solar wind', that travels at hundreds of kilometres per second, containing high energy particles and plasma. Fortunately the Earth is surrounded by an atmosphere and radiation belts that, in conjunction with the Earth's strong magnetic field, shield us from the these harmful particles.

Visually we can see the interaction of the solar wind with the Earth's magnetosphere as auroras at the north and south poles. Electrically we observe disruption to power lines and communication when the Earth's magnetic field is shaken by the solar wind

Solar storms, increased output of plasma and high energy particles such as X-rays, can cause extreme disruption to satellites as electrical charges can develop to the point of discharge. Communications via ionospheric reflection is disrupted during large solar storms as the various ionospheric layers absorb the increased radiation levels.

The following links provide excellent information resources relating to the Sun's interaction to man's environment, Earth.

 

Space Weather A good primer on space weather basics arrowredbutt.jpg (1274 bytes)
SEC's Space Weather Now National weather service's space weather web site arrowredbutt.jpg (1274 bytes)
Current Solar Forecast NOAA daily update arrowredbutt.jpg (1274 bytes)
Real-Time Magnetopause and Bow Shock Model Dynamic modelling of the Earth's bow shock and magnetopause arrowredbutt.jpg (1274 bytes)
Estimated Auroral Activity from NOAA/TIROS Auroral Activity Extrapolated from NOAA TIROS satellite sensors arrowredbutt.jpg (1274 bytes)