Coronal Radiation and Ionospheric Variations during the Solar Eclipse, July 9, 1945
Abstract
From the ionospheric observations made by O. Rydbeck and from the coronal observations made by the author it is deduced that the source of the solar ultra-violet light, producing the E-layer, lies in the innermost part of the corona in the regions of highest intensity of the 5303-radiation. Very strong support to this conclusion is given by the fact that in these regions the temperature of the corona reaches its highest values.
- Publication:
-
Terrestrial Magnetism and Atmospheric Electricity
- Pub Date:
- 1947
- DOI:
- 10.1029/TE052i003p00333
- Bibcode:
- 1947TeMAE..52..333W