Sabatino Sofia
Affiliations: | Astronomy | Yale University, New Haven, CT |
Area:
stellar structure and evolutionWebsite:
http://www.astro.yale.edu/sofia/Google:
"Sabatino Sofia"Bio:
http://ycaa.yale.edu/people/sabatino-sofia
http://adsabs.harvard.edu/abs/1966PhDT.........5S
http://articles.adsabs.harvard.edu//full/1966ApJ...145...84S/0000099.000.html
Mean distance: (not calculated yet)
Parents
Sign in to add mentorJames Hardin Hunter | grad student | 1966 | Yale | |
Ludwig Friedrich Oster | grad student | 1966 | Yale | |
(The Origin of Condensations in Planetary Nebulae.) |
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Publications
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Sofia S, Fox P. (1994) Solar variability and climate: an editorial essay Climatic Change. 27: 249-257 |
Lydon TJ, Fox PA, Sofia S. (1993) Improved solar models constructed with a formulation of convection for stellar structure and evolution calculations without the mixing-length theory approximations The Astrophysical Journal. 403 |
Gatewood G, Castelaz M, Persinger T, et al. (1989) A Map-based Determination of the Nature of Beta Delphini The Astrophysical Journal. 342: 1085-1090 |
Sofia UJ, Bruhweiler FC, Sofia S. (1989) Ultraviolet variability of the solar analogue star Alpha Centauri A Journal of Geophysical Research. 94: 9117-9124 |
Sofia S, Endal AS. (1987) The Solar-Stellar Connection - Solar Studies Publications of the Astronomical Society of the Pacific. 99: 1241-1247 |
Schatten KH, Miller N, Sofia S, et al. (1985) The importance of improved facular observations in understanding solar constant variations The Astrophysical Journal. 294: 689-696 |
Sofia S, Chiu HY, Maier E, et al. (1984) Solar disk sextant. Applied Optics. 23: 1235 |
Chiu HY, Maier E, Schatten KH, et al. (1984) Solar disk sextant optical configuration. Applied Optics. 23: 1230 |
Schatten KH, Miller N, Sofia S, et al. (1982) Solar irradiance modulation by active regions from 1969 through 1980 Geophysical Research Letters. 9: 49-51 |
Sofia S, Chan KL. (1982) Quick matching technique to study the relationship between solar radius and luminosity variations Solar Physics. 76: 145-153 |