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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 />

Equatorial-to-Middle Latitude Ionospheric Irregularities: Studies Using ROCSAT Data<br />

Su Shin-Yi 1 , Chao Chi-Kw<strong>an</strong> 1 , Liu Chao-H<strong>an</strong> 2<br />

1 National Central University, 2 Academia Sinica<br />

Equatorial-to-middle latitude topside ionospheric ion density variations observed by<br />

ROCSAT-1 at the 600-km altitude have been studied to construct the global/seasonal/localtime<br />

distributions of the equatorial plasma depletion (plasma bubble) occurrence rates, <strong>an</strong>d the<br />

low-to-middle latitude plasma enh<strong>an</strong>cement (plasma blob) occurrence rates from 1999 to<br />

2004 when the solar activities were mo<strong>der</strong>ate to high. The occurrence distributions of the two<br />

contrasting density irregularity structures indicate some complementary pattern in the<br />

latitudinal distribution. The seasonal/longitudinal (s/l) distributions of the equatorial density<br />

depletions have been studied extensively in the past <strong>an</strong>d the causes of such distributions have<br />

been proposed due to (1) the magnetic declination <strong>an</strong>gle to affect the longitudinal gradient of<br />

the ionospheric conductivity across the sunset terminator, (2) the geographic location of the<br />

dip equator to affect the ionospheric seasonal density variation, <strong>an</strong>d (3) the strength of the<br />

geomagnetic field at the dip equator to drive the over-all electrodynamics. In contrast, the<br />

study of the low-to-middle latitude density enh<strong>an</strong>cements has just been started <strong>an</strong>d the<br />

occurrence distribution only indicates that the maximum occurrence rates appear during the<br />

June solstice in both northern <strong>an</strong>d southern hemispheres. Some occurrence dependence is<br />

noticed at longitude of large magnetic declination region, but the causal relationship between<br />

the equatorial density depletion <strong>an</strong>d the density enh<strong>an</strong>cement irregularities needs further<br />

investigation. Details of the global/seasonal/local-time distributions between the two different<br />

density irregularities are compared <strong>an</strong>d the causes of the plasma enh<strong>an</strong>cement irregularity<br />

structures are discussed.

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