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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 />

Multi-frequency radar studies of PMSE: statistical properties, microphysical results <strong>an</strong>d<br />

electron densities<br />

Li Qi<strong>an</strong>g , Rapp Markus<br />

<strong>Leibniz</strong>-<strong>Institut</strong>e of Atmospheric Physics at the Rostock University, Kühlungsborn, Germ<strong>an</strong>y<br />

It is now common belief that polar mesosphere summer echoes (PMSE) originate from<br />

turbulence-induced scatter in combination with a large Schmidt number due to the presence of<br />

charged ice particles. It provides us opportunity to achieve deep insight of PMSE to apply this<br />

theory on simult<strong>an</strong>eous observations of PMSE at two well separated frequencies. In this<br />

study, we first present the statistical properties of PMSE obtained from simult<strong>an</strong>eous<br />

observations with the EISCAT Svalbard radar <strong>an</strong>d the SOUSY Svalbard radar (collocated<br />

near Longyearbern (78 o N, 16 o E), with frequencies of 500 <strong>an</strong>d 53.5 MHz, respectively) in June<br />

2006 <strong>an</strong>d also with the EISCAT VHF <strong>an</strong>d UHF radars (collocated near Tromso (69 o N, 19 o E),<br />

with frequencies of 224 <strong>an</strong>d 930 MHz, respectively) from the years 2003 through 2007.<br />

According to the above mentioned theory, the ratio of the volume reflectivities of PMSE<br />

simult<strong>an</strong>eously observed at two frequencies c<strong>an</strong> be used to calculate the Schmidt number <strong>an</strong>d<br />

hence the radii of the charged ice particles involved. The resulting particle radii display<br />

excellent agreement with expectations from microphysical models <strong>an</strong>d independent<br />

observations of microphysical ice parameters using optical techniques. Finally, we use UHFradar<br />

measurements of incoherent scatter in the presence of VHF PMSE to study the electron<br />

density dependence of PMSE. Statistical distributions of the ratio |ZA|NA/ne will be presented<br />

(where ZA is the average aerosol charge, NA the aerosol number density, <strong>an</strong>d ne the free<br />

electron number density) revealing that in the majority of cases |ZA|NA/ne

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