Solar flux and seasonal variations of the mesopause temperatures at 51°N

Y. Sahai , D.H. Giers , L.L. Cogger , P.R. Fagundes , G.P. Garbe
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引用次数: 18

Abstract

Observations of the OH (8-3) band airglow emission, using a multichannel tilting filter type photometer, have been carried out at Calgary (51°N, 114°W), Canada, since 1981. In this paper recent measurements of the nocturnal, seasonal and solar flux variations of the mesopause temperature, obtained from the rotational temperature of the OH (8-3) band observations, are presented. The data presented span the ascending phase of the present solar cycle viz. 1987–1988 (low solar activity) and 1990 (high solar activity). Good correlations (r = 0.73) between the OH (8-3) band rotational temperature and the 10.7 cm solar flux were observed. The mean temperature for the period investigated was about 210 K. The seasonally averaged nocturnal variations show only small irregular excursions, possibly associated with solar tides and the passage of gravity waves in the mesopause region. However, the observed rotational temperatures show considerable night-to-night changes.

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太阳通量与51°N中层顶温度的季节变化
自1981年以来,在加拿大卡尔加里(51°N, 114°W)使用多通道倾斜滤光片式光度计对OH(8-3)波段气辉光发射进行了观测。本文介绍了最近从OH(8-3)波段的旋转温度观测中获得的夜间、季节和太阳通量变化的测量结果。所提供的资料跨越当前太阳周期的上升阶段,即1987-1988年(太阳活动低)和1990年(太阳活动高)。OH(8-3)波段旋转温度与10.7 cm太阳通量具有良好的相关性(r = 0.73)。研究期间的平均温度约为210 K。季节平均夜间变化显示只有小的不规则的偏移,可能与太阳潮汐和重力波在中层顶区域的通过有关。然而,观测到的旋转温度显示出相当大的夜间变化。
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