Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-17T16:26:08.176Z Has data issue: false hasContentIssue false
  • English
  • Français

Temperature Fluctuations and Convective Modes in the Solar Photosphere

Published online by Cambridge University Press:  25 April 2016

P. R. Wilson
P. R. Wilson*
Affiliation:
Department of Applied Mathematics, University of Sydney
Get access Rights & Permissions [Opens in a new window]

Extract

Recently I have carried out a two-dimensional radiative-transfer analysis of the data given by Edmonds on centrelimb relative rms intensity fluctuations in terms of horizontal temperature fluctuations in the solar photosphere. Edmonds himself attempted an analysis of his data and found a ΔTrms which increased monotonically from about 300°K at unit mean optical depth (i.e. at a given physical depth) to 500°K at optical depth 3.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 5 , March 1969 , pp. 195 - 196
Copyright
Copyright © Astronomical Society of Australia 1969

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Edmonds, F. N., Ap. J. Suppl., 6, 367 (1962).CrossRefGoogle Scholar
2 Edmonds, F. N., Ap. J., 139, 1358 (1964).CrossRefGoogle Scholar
3 Wilson, P. R., Solar Phys., in press (1969).Google Scholar
4 Townsend, A. A., Quart, J. Roy. Met. Soc., 90, 248 (1964).Google Scholar
5 Herring, J. R., J. Atmos, Sci., 20, 325 (1963).Google Scholar