Bibcode
Palle, P. L.
Bibliographical reference
(Helioseismology from space; Proceedings of the Interdisciplinary Scientific Commission E Meeting (ME.7) of the COSPAR 28th Plenary Meeting, The Hague, Netherlands, June 25-July 6, 1990. A91-34076 13-92) Advances in Space Research (ISSN 0273-1177), vol. 11, no. 4, 1991, p. 29-38.
Advertised on:
1991
Citations
0
Refereed citations
0
Description
The characteristics of the three different principal data sets that have
been extensively analyzed in a search for g-modes (Tenerife, ACRIM, and
Stanford) are reviewed, and the results claimed from the analysis are
examined. It is noted that discrepancies betwen observers suggest that,
though they have probably been detected, the solar g-modes have not yet
been measured or classified. There is general agreement about the
existence of signals, embedded in noise, in the low-frequency range
where g-modes are expected to occur. The situation appears to be quite
different from that for p-modes (e.g., lower frequencies and poorer
SNR). It is concluded that, given the planned SOHO helioseismology
experiments and earth-based networks of helioseismological instruments,
there is real hope for success in the future.