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[Untitled]

Authors :
Theodore D. Tarbell
M. Rubin
Edward J. Rhodes
R. Howe
C. De Forest
Joergen Christensen-Dalsgaard
C. J. Wolfson
Thomas L. Duvall
Sarbani Basu
J. L. R. Saba
Douglas Gough
P. M. Giles
D. Mathur
Werner Däppen
M. Morrison
A. Burnette
Alan M. Title
R. Nigam
P. N. Milford
Takashi Sekii
R. I. Bush
S. D. Williams
Alexander G. Kosovichev
L. Bacon
Juri Toomre
K. Leibrand
I. Zayer
J. Aloise
Michael Thompson
K. Scott
Philip H. Scherrer
Jesper Schou
J. T. Hoeksema
R. S. Bogart
Source :
Solar Physics. 170:43-61
Publication Year :
1997
Publisher :
Springer Science and Business Media LLC, 1997.

Abstract

The medium-l program of the Michelson Doppler Imager instrument on board SOHO provides continuous observations of oscillation modes of angular degree, l, from 0 to ∼ 300. The data for the program are partly processed on board because only about 3% of MDI observations can be transmitted continuously to the ground. The on-board data processing, the main component of which is Gaussian-weighted binning, has been optimized to reduce the negative influence of spatial aliasing of the high-degree oscillation modes. The data processing is completed in a data analysis pipeline at the SOI Stanford Support Center to determine the mean multiplet frequencies and splitting coefficients.

Details

ISSN :
00380938
Volume :
170
Database :
OpenAIRE
Journal :
Solar Physics
Accession number :
edsair.doi...........b7e54e543a99f507c2d515be58baae96
Full Text :
https://doi.org/10.1023/a:1004949311268