High time resolution PFISR and optical observations of naturally enhanced ion acoustic lines

被引:15
|
作者
Michell, R. G. [1 ]
Lynch, K. A. [1 ]
Heinselman, C. J. [2 ]
Stenbaek-Nielsen, H. C. [3 ]
机构
[1] Dartmouth Coll, Dept Phys & Astron, Hanover, NH 03755 USA
[2] SRI Int, Menlo Pk, CA 94025 USA
[3] Univ Alaska Fairbanks, Inst Geophys, Fairbanks, AK 99775 USA
关键词
Ionosphere; Plasma waves and instabilities; Wave-particle interactions; Magnetospheric physics; Auroral phenomena; FIELD-ALIGNED CURRENTS; RADAR OBSERVATIONS; AURORAL IONOSPHERE; EISCAT SVALBARD; ALFVEN WAVES; PLASMA; INSTABILITIES; ENERGIZATION; ACCELERATION; FLUCTUATIONS;
D O I
10.5194/angeo-27-1457-2009
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Observations of naturally enhanced ion acoustic lines (NEIALs) taken with the Poker Flat Incoherent Scatter Radar (PFISR) using a mode with very high time resolution are presented. The auroral event took place over Poker Flat, Alaska on 8 February 2007 at 09: 35 UT (similar to 22:00 MLT), and the radar data are complemented by common-volume high-resolution auroral imaging. The NEIALs occurred during only one of the standard 15-s integration periods. The raw data of this time show very intermittent NEIALs which occur only during a few very short time intervals (<= 1s) within the 15-s period. The time sampling of the raw data, similar to 19 ms on average, allows study of the time development of the NEIALs, though there are indications that even finer time resolution would be of interest. The analysis is based on the assumption that the NEIAL returns are the result of Bragg scattering from ion-acoustic waves that have been enhanced significantly above thermal levels. The spectra of the raw data indicate that although the up-and down-shifted shoulders can both become enhanced at the same time, (within 19 ms), they are most often enhanced individually. The overall power in the up-and down-shifted shoulders is approximately equal throughout the event, with the exception of one time, when very large up-shifted power was observed with no corresponding down-shifted power. This indicates that during the 480 mu s pulse, the strongly enhanced ion-acoustic waves were only traveling downward and not upward. The exact time that the NEIALs occurred was when the radar beam was on the boundary of a fast-moving (similar to 10 km/s), bright auroral structure, as seen in the high resolution auroral imaging of the magnetic zenith. When viewed with high time resolution, the occurrence of NEIALs is associated with rapid changes in auroral luminosity within the radar field of view due to fast-moving auroral fine structures.
引用
收藏
页码:1457 / 1467
页数:11
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