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Line Profiles and Rotational Splitting of Individual P-Modes

Published online by Cambridge University Press:  08 February 2017

V.G. Gavryusev  and
E.A. Gavryuseva
V.G. Gavryusev
Affiliation:
CAISMI CNR, Largo E. Fermi 5, 50125, Florence, Italy
E.A. Gavryuseva
Affiliation:
Osservatorio Astronomico di Capodimonte, via Moiariello 16, I-80131, Naples, Italy, Institute for Nuclear Research RAN, Moscow, Russia

Extract

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We used GONG time series for ℓ = 0,1,2,3 from June 10, 1995 to January 7, 1997, 578 days in total. The duty cycle varies significantly during this period of time but on average it is sufficiently high, and the remaining gaps are irregular. Because of this we do not see daily side lobes in the spectra obtained.

Type
III. Large-Scale Structure of the Sun
Information
Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 153 - 156
Copyright
Copyright © Kluwer 1998 

References

Gavryusev, V.G., Gavryuseva, E.A., 1996, A&A, 310, 651 Google Scholar
Gavryusev, V.G., Gavryuseva, E.A., 1997, submitted to ApJ Google Scholar