GROUND-BASED PHOTOMETRIC OBSERVATIONS OF THE MAGNETOSPHERIC DAYSIDE CLEFT

被引:15
|
作者
Peterson, R. N. [1 ]
Shepherd, G. G. [1 ]
机构
[1] York Univ, Ctr Res Expt Space Sci, Toronto, ON M3J 1P3, Canada
关键词
D O I
10.1029/GL001i006p00231
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
A ground-based meridian-scanning photometer was operated at Cape Parry, N.W.T., Canada (70 degrees N, 125 degrees W geographic) in November and December, 1973, to observe the atomic oxygen emissions at 6300 angstrom and 5577 angstrom, and the H-beta emission at 4861 angstrom. A 6300 angstrom behaviour pattern that could be identified with the dayside cleft was observed during a quiet afternoon and during a magnetically disturbed period. During quiet times a 1 kR 6300 angstrom feature was observed at 78 degrees invariant latitude while during a modest disturbance the intensity increased to 4 kR and the feature moved to 73 invariant. This confirmed that the 6300 angstrom signature is readily identifiable from the ground, and that Cape Parry is one of the few relatively accessible Northern hemisphere sites where the optical cleft emissions can be observed from the ground.
引用
收藏
页码:231 / 234
页数:4
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