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Helioseismology from the South Pole The 1984/85 campaign

Published online by Cambridge University Press:  03 August 2017

B. Gelly ,
E. Fossat ,
G. Grec  and
M. Pomerantz
B. Gelly
Affiliation:
Département d'Astrophysique de l'I.M.S.P., Universite de NICE, Parc Valrose, F-06034 NICE-CEDEX
E. Fossat
Affiliation:
Département d'Astrophysique de l'I.M.S.P., Universite de NICE, Parc Valrose, F-06034 NICE-CEDEX
G. Grec
Affiliation:
Département d'Astrophysique de l'I.M.S.P., Universite de NICE, Parc Valrose, F-06034 NICE-CEDEX
M. Pomerantz
Affiliation:
Département d'Astrophysique de l'I.M.S.P., Universite de NICE, Parc Valrose, F-06034 NICE-CEDEX

Abstract

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More than 700 hours of full disk line of sight solar velocity have been recorded at the Geographic South Pole between late november 1984 and early february 1985. This paper presents very briefly some preliminary result of the analysis of this data.

Type
Chapter 1: Observations of Solar Oscillations
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 21 - 23
Copyright
Copyright © Reidel 1988 

References

Grec, G.; Fossat, E. and Pomerantz, M. 1983, Solar Phys. 82, 55 Google Scholar
Woodard, M. and Hudson, H. 1983, Nature, 305, 589 Google Scholar
Woodard, H. and Noyes, R.B. 1985, Seismology of the Sun and the Distant Stars, p303, Reidel, Gough, D. O., ed.Google Scholar