Difference between revisions of "Solar wind"

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The '''solar wind''' is the continuous stream of energetic and ionized particles from the [[Sun]] that extends far into interplanetary space following the interplanetary magnetic field (IMF). The ''solar wind'' strongly interacts with magnetic fields of the planets and will often manifest itself as [[aurora|aurorae]] in the upper atmospheres of planets with magnetic fields. In the case of Mars, with a weak (often considered to be non-existent) global magnetic field, solar wind particles have greater penetration into the atmosphere creating a hazard to any future [[hill-side concept|human settlements]] on the surface. The ''solar wind'' is often associated with [[Coronal Mass Ejections]] (CMEs), [[solar flares]] and coronal holes.  
 
The '''solar wind''' is the continuous stream of energetic and ionized particles from the [[Sun]] that extends far into interplanetary space following the interplanetary magnetic field (IMF). The ''solar wind'' strongly interacts with magnetic fields of the planets and will often manifest itself as [[aurora|aurorae]] in the upper atmospheres of planets with magnetic fields. In the case of Mars, with a weak (often considered to be non-existent) global magnetic field, solar wind particles have greater penetration into the atmosphere creating a hazard to any future [[hill-side concept|human settlements]] on the surface. The ''solar wind'' is often associated with [[Coronal Mass Ejections]] (CMEs), [[solar flares]] and coronal holes.  
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[[Category:Space Weather]]
 
[[Category:Space Weather]]

Revision as of 19:54, 11 October 2007

The solar wind is the continuous stream of energetic and ionized particles from the Sun that extends far into interplanetary space following the interplanetary magnetic field (IMF). The solar wind strongly interacts with magnetic fields of the planets and will often manifest itself as aurorae in the upper atmospheres of planets with magnetic fields. In the case of Mars, with a weak (often considered to be non-existent) global magnetic field, solar wind particles have greater penetration into the atmosphere creating a hazard to any future human settlements on the surface. The solar wind is often associated with Coronal Mass Ejections (CMEs), solar flares and coronal holes.

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