Performance and early results from the GOLF instrument flown on the SOHO mission

被引:90
作者
Gabriel, AH [1 ]
Charra, J
Grec, G
Robillot, JM
Cortes, TR
Turck-Chieze, S
Ulrich, R
Basu, S
Baudin, F
Bertello, L
Boumier, P
Charra, M
Christensen-Dalsgaard, J
Decaudin, M
Dzitko, H
Foglizzo, T
Fossat, E
Garcia, RA
Herreros, JM
Lazrek, M
Palle, PL
Petrou, N
Renaud, C
Regulo, C
机构
[1] Univ Paris 11, CNRS, Inst Astrophys Spatiale, F-91405 Orsay, France
[2] CNRS, Lab Cassini, Observ Cote Azur, URA 1362, F-06304 Nice, France
[3] Univ Bordeaux 1, Observat, F-33270 Floirac, France
[4] Inst Astrofis Canarias, Tenerife 38205, Spain
[5] CE Saclay, DSM, DAPNIA, Serv Astrophys, F-91191 Gif Sur Yvette, France
[6] Univ Calif Los Angeles, Dept Astron, Los Angeles, CA 90024 USA
[7] Danmarks Grundforskningsfond, Teoretisk Astrofys Ctr, Aarhus, Denmark
[8] Natl Opt Astron Observ, Natl Solar Observ, Tucson, AZ 85726 USA
[9] Inst Fys Astron, DK-8000 Aarhus, Denmark
[10] Univ Nice, CNRS, Dept Astrophys, URA 709, F-06034 Nice, France
[11] CNR, CNCPRST, Rabat, Morocco
关键词
D O I
10.1023/A:1004911408285
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
GOLF in-flight commissioning and calibration was carried out during the first four months, most of which represented the cruise phase of SOHO towards its final L1 orbit. The initial performance of GOLF is shown to be within the design specification, for the entire instrument as well as for the separate sub-systems. Malfunctioning of the polarising mechanisms after 3 to 4 months operation has led to the adoption of an unplanned operating sequence in which these mechanisms are no longer used. This mode, which measures only the blue wing of the solar sodium lines, detracts little from the detection and frequency measurements of global oscillations, but does make more difficult the absolute velocity calibration, which is currently of the order of 20%. Data continuity in the new mode is extremely high and the instrument is producing exceptionally noise-free p-mode spectra, The data set is particularly well suited to the study of effects due to the excitation mechanism of the modes, leading to temporal variations in their amplitudes. The g modes have not yet been detected in this limited data set. In the present mode of operation, there are no indications of any degradation which would limit the use of GOLF for up to 6 years or more.
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收藏
页码:207 / 226
页数:20
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