Quasi-Periodic Auroras in the Post-Noon Sector and their Relationship to the High Time Resolution Mode HF Radar

Y. MURATA.1), N. SATO2), H. YAMAGISHI2), A. S. YUKIMATU2), M. KIKUCHI2), K. MAKITA3) T. OGAWA4), H. YANG5) R. LIU5) A. D. M. WALKER6) and M. LESTER7)
1 Graduate University for Advanced Studies, Japan
2National Institute of Polar Research, Japan
3Takushoku University, Japan
4Nagoya University, Japan
5Polar Research Institute of China, China.
6University of Natal, South Africa.
7University of Leicester, UK.

Zhongshan Station in Antarctica is located at 74.49°S in invariant geomagnetic latitude and MLT=UT+1.3hr. All-sky TV camera and meridian-scanning photometer at Zhongshan gives us an opportunity to observe quasi-periodic optical aurora in the vicinity of the cusp/cleft region on the post-noon sector. The field of view of the Syowa East HF radar covers over Zhongshan, so that it is possible to investigate the spatial and temporal signatures of quasi-periodic optical aurora and HF radar aurora. We report here a case study of simultaneous observations of quasi-periodic optical aurora, HF radar backscatter power, Doppler velocity and ground based magnetogram, acquired on August 3, 1997. The Syowa East radar has been operating on a high time resolution mode and all-sky camera and photometers were running at Zhongshan under clear sky. Quasi-periodic optical aurora with period of ~1-min and ~10- min has been identified during ~1200-1400 UT. Fine structure of the aurora showed an east-west aligned band/arc type discrete aurora, and the luminosity position moved poleward quasi-periodically. The HF radar backscatter powers and magnetic variations showed one to one correlations with the 10-min quasi-periodic variations of optical aurora. The magnetic pulsations observed at Zhongshan and Syowa in Antarctica and IMAGE magnetometer array in the northern hemisphere revealed typical field line resonance characteristics; the latitudinal dependence of amplitude and polarization parameters.

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