Zeman Lab Radar

The 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 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


UT Date CSR RTI images images images MHO data Ionogram
Jun. 1 2021 r210601.pdf s210601a.mp4 0130 UT
Jun. 14 2021 r210614.pdf s210614.mp4 0130 UT
Jun. 19 2021 r210619.pdf 0130 UT
Jun. 28 2021 r210628.pdf s210628b.mp4 s210628c.mp4 0200 UT
Jun. 29 2021 r210629.pdf s210629.mp4 0200 UT
Jun. 30 2021 r210630.pdf s210630a.mp4 s210630b.mp4 0300 UT
Jul. 2 2021 r210702.pdf s210702a.mp4 s210702b.mp4 ne2021-07-01.png 0200 UT
Jul. 7 2021 r210707.pdf s210707.mp4 0300 UT
Jul. 23 2021 r210723.pdf s210723.mp4 0300 UT
Jul. 30 2021 r210730.pdf s210730.mp4 ne2021-07-29.png 0030 UT
Jul. 31 2021 r210731.pdf s210731.mp4 0100 UT
Aug. 5 2021 r210805.pdf s210805.mp4 0130 UT
Sep. 1 2021 r210901.pdf s210901a.mp4 s210901b.mp4 0100 UT


UT Date CSR RTI images images images MHO data Ionogram
Jun. 12 2022 r220612.pdf s220612.mp4 0215 UT
Jun. 13 2022 r220613.pdf s220613.mp4 0200 UT
Jun. 14 2022 r220614.pdf s220614.mp4 0200 UT
Jul. 7 2022 r220707.pdf 0300 UT
Jul. 8 2022 r220708.pdf
Aug. 15 2022 r220815.pdf s220815a.mp4 s220815b.mp4 0000 UT


UT Date CSR RTI images images images MHO data Ionogram
May 29, 2023 r230529.pdf s230529.mp4 0300 UT
Jul. 9, 2023 r230709.pdf s230709.mp4 0300 UT
Jul. 10, 2023 r230710.pdf 0300 UT
Jul. 19, 2023 r230719.pdf 0300 UT
Jul. 30, 2023 r230730.pdf 0330 UT
Jul. 31, 2023 r230731.pdf s230731.mp4 0100 UT


UT Date CSR RTI images images images MHO data Ionogram
May 11, 2024 r240511.pdf s240511.mp4
June 26, 2024 r240626.pdf s240626_1.mp4 s240626_2.mp4
June 27, 2024 r240627.pdf s240627_1.mp4 s240627_2.mp4
July 10, 2024 r240710.pdf
Oct. 11, 2024 r241011.pdf s241011_1.mp4 s241011_2.mp4

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