Sundogs in Antarctica南极的幻日
The parhelia or "sun dogs" are more readily visible in the cold of the antarctic and artic regions. 极地和南极地区的寒冷气候使日晕更加容易被观察到。
![]() ![]() Photos by Dr. Richard Sadleir. Used by permission. All rights reserved. 由理查德·萨德利博士拍摄。经许可使用。版权所有。
"I also noticed something I had not seen in previous sun haloes, perhaps because this was in perfect conditions. The light ring of the halo was very intense on the sun side of the halo and then faded outwards. " 我也注意到一个我以前在日晕中没有见过的现象,也许是因为这次条件非常理想。日晕的光环在日侧非常明亮,然后向外逐渐变弱。
"After the whole phenomena faded, the cloud of ice crystals actually fell around us for a short time. They were elongated crystals about 8 to 12 mm long. I remember them as falling vertically (the air was absolutely still)." 现象消失后,冰晶云在我们周围短暂地飘落。这些冰晶呈细长形状,长度约为8到12毫米。我记得它们是垂直下落的(当时空气完全静止)。
The coloration of the sundogs arises from dispersion in the ice crystals, which act as 60° prisms to separate the colors of sunlight. The prism calculation using n=1.306 for red and n=1.317 for blue gives angles of 21.54° and 22.37° for red and blue respectively. The inner edge of the halo is sharp and appears reddened - the angle of minimum deviation for red is less and you see it from crystals closer to the Sun or Moon direction. The out edge of the halo is blue in appearance but less saturated because other wavelengths can refract at that angle.
sundogs 的颜色是由冰晶中的色散造成的,这些冰晶像 60° 的棱镜一样,将阳光的颜色分开。使用红光折射率 n=1.306 和蓝光折射率 n=1.317 进行棱镜计算,得到红光和蓝光的折射角分别为 21.54° 和 22.37°。光环的内边缘是清晰的,并且呈现红色——红光的最小偏转角较小,因此你看到它来自更接近太阳或月亮方向的冰晶。光环的外边缘看起来是蓝色的,但饱和度较低,因为其他波长的光可以在该角度发生折射。 |
Index Halo formation Atmospheric optics concepts References Greenler Schaaf 索引 群星形成 大气光学概念 参考文献 Greenler Schaaf | ||||||
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