Abstract
By means of a coronagraph and a visual skyphotometer which is based upon coronagraph principles, the intensity of the solar aureole in the interval 4’–66’ from the sun limb has been studied. The results show that there is a good correlation between the type of prevailing air mass and the characteristics of the measured intensity. The intensity variation with time and height is studied and discussed.
DOI: https://doi.org/10.3402/tellusa.v20i1.9918 | Journal eISSN: 3035-9554
Language: English
Page range: 55 - 64
Submitted on: Oct 5, 1966
Published on: Jan 1, 1968
Published by: Stockholm University Press
In partnership with: Paradigm Publishing Services
© 1968 Bo Rydgren, published by Stockholm University Press
This work is licensed under the Creative Commons Attribution 4.0 License.
