Accurate Determination of the Solar Photospheric Radius
| dc.creator | Brown, T. M. | |
| dc.creator | Christensen-Dalsgaard, J. | |
| dc.date | 1998-03-11 | |
| dc.date.accessioned | 2026-07-07T11:46:09Z | |
| dc.date.available | 2026-07-07T11:46:09Z | |
| dc.description | The Solar Diameter Monitor measured the duration of solar meridian transits during the 6 years 1981 to 1987, spanning the declining half of solar cycle 21. We have combined these photoelectric measurements with models of the solar limb-darkening function, deriving a mean value for the solar near-equatorial radius of 695.508 +- .026 Mm. Annual averages of the radius are identical within the measurement error of +- .037 Mm. | |
| dc.description | 6 pages, 2 figures Submitted to Astrophys. J. Lett., March 9 1998 Uses AASTeX Macro package aas2pp4 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9803131 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9803131 | |
| dc.identifier | Astrophys.J.500:L195-L198,1998 | |
| dc.identifier | doi:10.1086/311416 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/202124 | |
| dc.subject | Astrophysics | |
| dc.title | Accurate Determination of the Solar Photospheric Radius | |
| dc.type | text |