Compton effect and solar spectral lines
β Scribed by P. Maltby
- Publisher
- Springer Netherlands
- Year
- 1977
- Tongue
- English
- Weight
- 145 KB
- Volume
- 47
- Category
- Article
- ISSN
- 0004-640X
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Progressive Alfv6n waves set the atoms in oscillatory motion. The radiation will be absorbed (emitted) at a Doppler-shifted wavelength; the Doppler shift is determined by the velocity given to the atoms by the wave. The effect of the waves on the line profile, integrated over one period, is given fo
A photographic Fabry-Perot interferometer was used to measure the breadth and wavelength of the Fexlv spectral line at 5303 β’ in the solar corona, during the eclipse of 7 March, 1970, in Mexico. The observations were consistent with a possible large-scale vortex structure in a bright streamer, in wh