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Thermal perturbation of the sun (Document No: 19820009155)
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Twigg, L. W. Endal, A. S. |
| Copyright Year | 1981 |
| Description | An investigation of thermal perturbations of the solar convective zone via changes in the mixing length parameter were carried out, with a view toward understanding the possible solar radius and luminosity changes cited in the literature. The results show that: (a) a single perturbation of alpha is probably not the cause of the solar radius change and (b) the parameter W = d lambda nR./d lambda nL. can not be characterized by a single value, as implied in recent work. |
| File Size | 191489 |
| Page Count | 6 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19820009155 |
| Archival Resource Key | ark:/13960/t3c010v32 |
| Language | English |
| Publisher Date | 1981-12-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Solar Diameter Solar Activity Luminosity Variations Solar Constant Magnetic Disturbances Mathematical Models Perturbation Convection Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
