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contributor authorStrong, Keith T.
contributor authorSchmelz, Joan T.
contributor authorSaba, Julia L. R.
contributor authorKucera, Therese A.
date accessioned2017-06-09T16:46:46Z
date available2017-06-09T16:46:46Z
date issued2017
identifier issn0003-0007
identifier otherams-73907.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4216073
description abstracthe Sun is often racked by short-term violent events such as flares and coronal mass ejections (CMEs) but these two phenomena are often confused. Both are caused by the release of energy due to the reconnection of stressed and unstable magnetic fields. Flares bathe the solar system in electromagnetic radiation from gamma-rays to radio emissions. CMEs throw billions of tonnes of solar plasma into interplanetary space at velocities of over 1,000 km s-1. Flares can occur without significant ejecta being spewed out from the Sun into the Solar System. CMEs can occur without a significant flare being detected. The most violent and dangerous events occur when a large flare is accompanied by a major eruption. These violent events are much more common near solar maximum but can occur at any time during the solar cycle, so we are rarely completely immune to their effects. Various types of solar activity can lead to problems with electrical grids, navigation systems, and communications, and can present a hazard to astronauts, as will be discussed in future papers in this series.
publisherAmerican Meteorological Society
titleUnderstanding Space Weather: The Violent Sun
typeJournal Paper
journal volume098
journal issue011
journal titleBulletin of the American Meteorological Society
identifier doi10.1175/BAMS-D-16-0191.1
journal fristpage2387
journal lastpage2396
treeBulletin of the American Meteorological Society:;2017:;volume( 098 ):;issue: 011
contenttypeFulltext


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