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The Upper Atmosphere

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This research is supported by the National Science Foundation.

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Zeman Lab

T he Imaging Radar Interferometer at Zeman Laboratory is located on the grounds of the Cornell Botanic Garden at a site once used for the development of hardware destined for the Arecibo Radio Observatory in Puerto Rico.

The radar is used to observe meter-scale field-aligned plasma density irregularities in the E region ionosphere over the Great Lakes region. The irregularities inhabit so-called sporadic E ionization layers made mainly from metallic ions. Similar irregularities are observed widely at middle latitudes where they occur in long bands spaced by tens of kilometers and propagating predominately to the southwest in the northern hemisphere. The bands are thought to be associated with neutral dynamic instability in the mesosphere/ lower thermosphere although various plasma instabilities may also be involved. Sporadic E layers and the attendant irregularities also occur at higher latitudes approaching the ionospheric trough but have received less attention until now.

The sporadic E-layer irregularities are connected by magnetic field lines with F-region irregularities associated with so-called midlatitude spread F. The field of view of the Zeman radar is overlooked by the Millstone Hill Observatory in Westford, Massachusetts, which can detect midlatitude spread F using incoherent scatter radar techniques. In addition, a coherent scatter radar located in Clemson, South Carolina, the twin of the Zeman radar, can detect F-region field-alligned irregularities via coherent scatter. Together with other instrumentation nearby, the radars will be used for a comprehensive investigation of instabilities and irregularities at the edge of the midlatitude ionosphere.

A key feature of the Zeman and Clemson radars is their implementation of radar imaging techniques. Radar imaging provides a volumetric view of the scatterers under investigation. The images have a cadence of approximately once every three seconds, a range resolution of 1.5 km, and an angular resolution of approximately 0.5 degrees. Doppler spectra are imaged as well. The radars provide unambiguous information about the spatial, temporal, and dynamic structure of the underlying waves and instabilities.

Representative data

UT Date CSR RTI images images images MHO data Alpena ionogram
Jul. 16 2020 r200716.pdf s200716.mp4 0145 UT
Jul. 19 2020 r200719.pdf 0022 UT
Aug. 5 2020 r200805.pdf s200805.mp4 0130 UT
Aug. 11 2020 r200811.pdf s200811a.mp4 s200811b.mp4 s200811c.mp4 0052 UT

Gallery

Here are some images from the radar field site.