Observational constraints on the solar opacity profile
โ Scribed by F.L. Villante
- Publisher
- Elsevier Science
- Year
- 2011
- Tongue
- English
- Weight
- 215 KB
- Volume
- 217
- Category
- Article
- ISSN
- 0920-5632
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
Observations of the intensity distribution near the solar limb at 2.43 and 22.5/t, show the absence of limb brightening to within 1 or 2 arc sec of the limb. Observations at 1.2 mm indicate limb brightening at this wavelength. These results are compared with the Utrecht Reference Photosphere and wit
The observed large rates of spinning down after glitches in some radio pulsars have been previously explained in terms of a long-term spin-up behavior of a superfluid part of the crust of neutron stars. We argue that the suggested mechanism is not viable; being inconsistent with the basic requiremen