Abstract
The variation of the cosmic ray intensity during a magnetic storm has been ascribed to the electrically polarized beam of particles from the sun. The loss of particles due to the total reflection in the electric field has been calculated. For comparison with observations, however, the change of intensity I per surface element dS, solid angle dΩ, and energy interval dW should be considered.
DOI: https://doi.org/10.3402/tellusa.v6i3.8737 | Journal eISSN: 3035-9554
Language: English
Page range: 260 - 260
Published on: Jan 1, 1954
Published by: Stockholm University Press
In partnership with: Paradigm Publishing Services
© 1954 S. Lundquist, published by Stockholm University Press
This work is licensed under the Creative Commons Attribution 4.0 License.