DAWN ENHANCEMENT OF AURORAL EMISSION

Author:

Lytle E. A.,Hunten D. M.

Abstract

The 0–0 band at 3914 Å was observed once per minute with a scanning spectrometer as sunlight illuminated the upper atmosphere on the morning of September 5, 1958. It is reasonable to assume that the density of [Formula: see text] ions was maintained constant during this time, and that the observed rise of intensity was due to resonance scattering of sunlight. The ions were found to be distributed between 180 and 320 km with peak at 250; density here was 12 × 104 ions/cm3. There was some evidence for another layer at 120 km. Rotational temperatures measured while the main layer was fully illuminated agreed well and gave an average of 1060 ± 100 °K.

Publisher

Canadian Science Publishing

Subject

General Physics and Astronomy

Cited by 21 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Morphology of evening sector aurorae in λ557.7-nm Doppler temperatures;Geophysical Research Letters;2005

2. Sunlit aurora and the N2+ ion: a personal perspective;Planetary and Space Science;2003-11

3. Physics of the Aurora and Airglow;1995

4. Physics of the Optical Emissions;Physics and Chemistry in Space;1971

5. Tropospheric scattering of twilight N2+ emission;Planetary and Space Science;1968-05

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