Space-time structure of auroral radio absorption events observed with the imaging riometer at South Pole

Details Space-time structure of auroral radio absorption events observed with the imaging riometer at South Pole Space-time structure of auroral radio absorption events observed with the imaging riometer at South Pole

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991rasc...26..925h&link_type=abstract

Radio Science (ISSN 0048-6604), vol. 26, July-Aug. 1991, p. 925-930.

Computer Science

Auroral Absorption, Ionospheric Propagation, Riometers, Earth Magnetosphere, Imaging Techniques, Polar Regions

Scientific paper

An imaging riometer system comprising 49 independent beams has been operating at South Pole station since January 1988. A study of intense, short-duration events from the premidnight sector has defined their typical shape as elliptical, with axial ratio 2.3 oriented along the local L shell. The space-time evolution shows rapid intensifications of the moving absorption patches.

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