1) aurora line
极光线
2) Aurora
极光
1.
Review of space-based FUV aurora/airglow observations;
星载远紫外极光/气辉探测发展综述
2.
A multiple wavelength monochromatic all-sky CCD imagers system has been deployed in this station, which monitors aurora phenomena on 427.
0nm)单色极光全天空CCD成像观测系统,并于2003年12月11日-2004年2月25日极夜期开展了首次极光越冬观测,获得了1200多小时的连续观测数据。
3.
To detect wind field in the upper atmosphere passive methods was used with imaging interferometer technique the main source is O(Ⅰ,Ⅱ) forbidden aurora.
利用干涉成像光谱技术被动探测上层大气风场所使用的光源主要是氧禁戒线极光。
3) aurora kinases
极光激酶
1.
Due to the continuously deepening research on aurora kinases recently, the key functions of aurora kinases in cell mitosis and tumorigenesis have been gradually revealed.
极光激酶(aurora kinases)是负责调控细胞有丝分裂的一类重要的丝氨酸/苏氨酸激酶。
4) Auroral belt
极光带
5) Postnoon aurora
午后极光
1.
Based on auroral observations of a multi channels scanning photometer at Zhongshan Station, Antarctica and solar wind parameters data obtained by WIND Satellite at the upstream of the bow shock in 1997 and 1998, the dependence of the high latitude postnoon auroral intensity upon the solar wind parameters are studied quantitatively.
研究表明 ,午后极光 6 3 0 。
2.
It is examined that postnoon aurora observed at Zhongshan station (invariant latitude 74.
５Ｓ，ＭＬＴ＝ ＵＴ＋ ２）利用全天空极光摄像机和三波段极光扫描光度计观测到的午后极光进行了分析，发现宁静日午后极光的形态随磁地方时变化。
6) Auroral intensity
极光强度
1.
Based on auroral observations of a multi channels scanning photometer at Zhongshan Station, Antarctica and solar wind parameters data obtained by WIND Satellite at the upstream of the bow shock in 1997 and 1998, the dependence of the high latitude postnoon auroral intensity upon the solar wind parameters are studied quantitatively.
本文利用 1 997年和 1 998年南极中山站多通道扫描光度计的地面观测数据和 WIND卫星在弓激波上游对太阳风参数的观测数据 ,对午后高纬极光强度与太阳风等离子体密度、动压以及太阳风速度之间的相关性进行了定量研究。
参考词条
补充资料：北极光
在北极地区，天空经常被绚丽的绿色、紫色和金色反射光照亮。这些就是北方的极光(北极光)。尽管在英语中“极光”有“黎明之光”的含义，但这些异常的光现象不是由于黎明引起，而是因为大气层受到太阳发射出的带电粒子的冲击而引起大规模放电所造成的。
说明：补充资料仅用于学习参考，请勿用于其它任何用途。