Solar gravitational redshift
β Scribed by James C. Lopresto; Robert D. Chapman; Elizabeth A. Sturgis
- Publisher
- Springer
- Year
- 1980
- Tongue
- English
- Weight
- 203 KB
- Volume
- 66
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
β¦ Synopsis
Wavelengths of solar spectrum lines should be shifted toward the red by the Sun's gravitational field as predicted by metric theories of gravity according to the principle of equivalence. Photographic wavelengths of 738 solar Fe I lines and their corresponding laboratory wavelengths have been studied. The measured solar wavelength minus the laboratory wavelength (AAobserved) averaged for the strong lines agrees well with the theoretically predicted shift (AAtheoretieal). Studies show that the departures depend on line strength. No dependence of the departures on wavelength was found within the existing data.
By studying strong lines over a wide spectral range, velocity shifts caused by the complex motions in the solar atmosphere seem to affect the results in a minimal fashion.
π SIMILAR VOLUMES
## Abstract Intergalactic gravitational radiation fields with wavelengths in the range of 1 to 10^3^ Megaparsecs have remarkable observational effects if the energy density of the fields becomes comparable to the equivalent βcriticalβ cosmological matter density Οo = 3__H__~0~^2^. In this case the