Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-27T05:45:43.299Z Has data issue: false hasContentIssue false
  • English
  • Français

III. Solar Rotation

Published online by Cambridge University Press:  25 April 2016

Robert F. Howard

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The study of solar rotation using the Doppler effect in solar spectrum lines continues to be an active and fruitful area of research. Duvall (1982) has confirmed a slower rotation rate for the photosphere than for sunspots, which bears on an earlier controversy regarding this point between the Stanford Solar Observatory and some other observatories. The issue is not settled, however.

Type
Research Article
Information
Transactions of the International Astronomical Union , Volume 19 , Issue 1 , 1985 , pp. 100 - 103
Copyright
Copyright © Reidel 1985

References

Abarbanell, C. and Wühl, H. 1981, Solar Phys., 70, 197.Google Scholar
Arevalo, M.J. et al. 1982, Astron. and Astrophys,, 111, 266.Google Scholar
Balthasar, H. and Schbssler, M. 1982, Solar Phys., 87, 23.Google Scholar
Balthasar, H. 1983, Solar Phys., 84, 371.Google Scholar
Cram, L.E., Durney, B.R. and Guenther, D.B. 1983, Ap. J., 267, 442.Google Scholar
Dicke, R.H. 1982, Solar Phys., 78, 3.Google Scholar
Duvall, T.L. Jr. 1982, Solar Phys., 76, 137.Google Scholar
Gilman, P.A. and Howard, R. 1984, Ap. J., 283, 285.Google Scholar
Godoli, G. and Mazzucconi, F. 1983, Solar Phys., 83, 339.Google Scholar
Howard, R. et al. 1983, Solar Phys., 87, 195.Google Scholar
Howard, R., Gilman, P.A. and Gilman, P.I. 1984, Ap. J., 283, 373.Google Scholar
Koch, A., Wbhl, H. and Schrbter, E.H. 1981, Solar Phys., 71, 295.Google Scholar
Kopecky, M. 1982, Bull. Astron. Inst. Czech., 33, 285.Google Scholar
Kubicela, A. and Karabin, M. 1983, Solar Phys., 84, 389.Google Scholar
Kuveler, G. and Wühl, H. 1983, Astron. and Astrophys,, 123, 29.Google Scholar
LaBonte, B.J. and Howard, R. 1982, Solar Phys., 75, 161.Google Scholar
Landman, D.A. and Takushi, J.T. 1981, Solar Phys., 73, 379.Google Scholar
Libbrecht, K. 1984, Ph.D. Thesis: Princeton University.Google Scholar
Livingston, W. and Duvall, T.L. Jr. 1979, Solar Phys, 61, 219.Google Scholar
Lustig, G. 1982, Astron. and Astrophys,, 106, 151.Google Scholar
Lustig, G. 1983, Astron. and Astrophys,, 125, 355.Google Scholar
Newton, H.W. and Nunn, M.L. 1951, M.N.R.A.S., 111, 413.Google Scholar
Perez-Garde, M. et al. 1981, Astron. and Astrophys, 93, 67.Google Scholar
Rovithis, P. 1982, Astrophysics and Space Science, 88, 5.Google Scholar
Snider, J.L. 1983, solar Phys., 84, 377.Google Scholar
Snodgrass, H.B. 1983, Ap. J., in press.Google Scholar
Ternullo, M., Zappala, R.A., and Zuccarello, F. 1981, Solar Phys., 74, 111.Google Scholar
Tuominen, J., Tuominen, I., and Kyrblbinen, J. 1983, M.N.R.A.S., 205, 69.Google Scholar
Yallop, B.D., Hohenkerk, C., Murdin, L. and Clark, D.H. 1982, Quart. J.R.A.S., 23, 213.Google Scholar