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scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

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STP12 Abstracts<br />

Berlin, 12 - 16 July <strong>2010</strong><br />

SCOSTEP Symposium <strong>2010</strong><br />

Short term variability of the high <strong>an</strong>d mid latitude ionosphere as a result of coupling<br />

between the solar wind <strong>an</strong>d magnetosphere<br />

Lester Mark , Mil<strong>an</strong> Stephen<br />

University of Leicester<br />

Ionospheric variability occurs on a r<strong>an</strong>ge of time scales from days to years <strong>an</strong>d probably<br />

centuries. In this talk we focus on the variability which is introduced by the coupling between<br />

the solar wind <strong>an</strong>d magnetosphere. This coupling introduces variability on time scales of<br />

hours, due to magnetospheric substorms, <strong>an</strong>d days, due to magnetic storms. The ch<strong>an</strong>ges in<br />

the ionosphere are due to enh<strong>an</strong>ced energy deposition into the ionosphere in the form of<br />

particle precipitation which results in heating of the plasma <strong>an</strong>d also enh<strong>an</strong>ced electric field<br />

resulting in Joule heating of the plasma. At high latitudes the ch<strong>an</strong>ges in the ionospheric<br />

plasma result from the enh<strong>an</strong>ced ionisation from particle precipitation, which c<strong>an</strong> lead to<br />

enh<strong>an</strong>ced absorption of radio waves should the particles penetrate to altitudes of 100 km <strong>an</strong>d<br />

less. Joule heating on the other h<strong>an</strong>d leads to enh<strong>an</strong>ced temperatures in the ionosphere<br />

resulting in enh<strong>an</strong>ced ion loss from either ion upflow or from enh<strong>an</strong>ced recombination. This<br />

tends to occur at altitude above about 250 km. At mid-latitudes the variability during<br />

substorms may be more related to the propagation of atmospheric gravity waves stimulated by<br />

the heating at cusp latitudes or auroral latitudes on the nightisde. These waves propagate to<br />

mid <strong>an</strong>d low latitudes resulting in variation in the ionospheric plasma density on time scales<br />

of hours. Mid-latitude variations due to storms are extremely complex due to tr<strong>an</strong>sport of<br />

plasma due to winds. In this presentation we shall concentrate on observations of the<br />

ionosphere made by the Super Dual Auroral Radar Network (SuperDARN) which extends<br />

from the poles to about 40 degrees of latitude in both hemispheres. These radars provide<br />

information on the electric fields responsible for Joule heating, ionospheric plasma<br />

distributions, in particular enh<strong>an</strong>ced absorption <strong>an</strong>d ch<strong>an</strong>ges in the F region peak density, <strong>an</strong>d<br />

gravity waves. With the continued extension to mid latitudes particularly in the Americ<strong>an</strong><br />

sector, these radars now provide critical information on the ionospheric variability on the<br />

short term.

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