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dc.contributor.authorMaggiolo R.
dc.date2015
dc.date.accessioned2016-10-12T12:17:16Z
dc.date.available2016-10-12T12:17:16Z
dc.identifier.isbn9781118978719
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/4449
dc.descriptionThe auroral ionosphere is a region of intense energy precipitation. Its most noteworthy effects are the intense luminous emissions observed in the auroral oval. Less visible but of primary importance for magnetospheric dynamics, this energy precipitation results in an intense outflow of ionospheric ions. In this chapter, we provide an overview of the whole chain of processes associated with auroral ion outflow. We discuss the processes that energize ionospheric ions, from the topside ionosphere to the more distant magnetospheric regions, and the effect of auroral ionospheric outflow on the magnetospheric dynamics. We will also present recent observations of auroral ion outflow. They provide a detailed picture of its large-scale spatial distribution, its dependence on solar and geomagnetic activity, its temporal dynamics, and its connection with auroral emissions. © 2016 by the American Geophysical Union. All rights reserved.
dc.languageeng
dc.publisherJohn Wiley & Sons, Hoboken, NJ, USA
dc.relation.ispartofseriesGeophysical Monograph Series
dc.titleAuroral Arcs and Ion Outflow
dc.typeBook chapter
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeacceleration mechanisms
dc.subject.freeauroral arc morphology
dc.subject.freeauroral arcs
dc.subject.freeion outflow
dc.subject.freeionospheric dynamics
dc.subject.freemagnetospheric dynamics
dc.subject.freespatial distribution
dc.source.titleAuroral Dynamics and Space Weather
dc.source.volume215
dc.source.page39-58
Orfeo.peerreviewedNo
dc.identifier.doi10.1002/9781118978719.ch4
dc.identifier.scopus2-s2.0-84977438858
dc.source.editorZhang, Y
dc.source.editorPaxton, L.J.


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