OBSERVATION OF ELECTROMAGNETIC OXYGEN CYCLOTRON WAVES IN A FLICKERING AURORA

被引:26
|
作者
LUND, EJ
LABELLE, J
TORBERT, RB
LIOU, K
PERIA, W
KLETZING, CA
KELLEY, MC
BAKER, SD
PRIMDAHL, F
STENBAEKNIELSEN, HC
RANTA, A
HAERENDEL, G
FREY, HU
机构
[1] UNIV NEW HAMPSHIRE,DEPT PHYS,DURHAM,NH 03824
[2] UNIV NEW HAMPSHIRE,CTR SPACE SCI,DURHAM,NH 03824
[3] CORNELL UNIV,CTR ENGN & THEORY,ITHACA,NY 14853
[4] TECH UNIV DENMARK,DEPT ELECTROPHYS,DK-2800 LYNGBY,DENMARK
[5] UNIV ALASKA,INST GEOPHYS,FAIRBANKS,AK 99775
[6] GEOPHYS OBSERV,SF-99600 SODANKYLA,FINLAND
[7] MAX PLANCK INST EXTRATERR PHYS,D-85740 GARCHING,GERMANY
关键词
D O I
10.1029/95GL02409
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Instruments on the Auroral Turbulence rocket detected several intervals of weak electromagnetic oscillations at frequencies of 6-13 He in a strongly flickering auroral are. These oscillations have amplitudes of up to delta B similar to 3 nT and delta E similar to 4 mV/m and have downward field-aligned Poynting fluxes of up to similar to 10(-5) W/m(2). Fluctuations in the parallel electron flux at about 9 Hz were observed in association with the strongest of these oscillations. Simultaneous groundbased optical data show that the are was flickering at frequencies of 8-15 He. The observed frequencies would match the oxygen-cyclotron frequency at similar to 4500 km altitude. In one wave/particle event the apparent lag of the waves behind the modulated electrons implies a modulation source altitude of 2500-5000 km. We interpret these waves as electromagnetic ion cyclotron waves originating in the auroral acceleration region.
引用
收藏
页码:2465 / 2468
页数:4
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