Index of /~sylvain/tables/2005

 Name                    Last modified       Size  Description

 Parent Directory        04-Jan-2008 10:29      -  
 2088d.gong.dat          04-Mar-2004 11:05   3.4M  
 2088d.gong.txt          15-Dec-2004 16:21   3.7M  
 2088d.mdi.dat           29-Jan-2004 13:16   3.6M  
 2088d.mdi.txt           15-Dec-2004 16:21   3.8M  
 728d.segment1.gong.dat  06-Mar-2004 10:59   3.3M  
 728d.segment1.gong.txt  15-Dec-2004 16:21   3.5M  
 728d.segment1.mdi.dat   17-Mar-2004 12:15   3.5M  
 728d.segment1.mdi.txt   15-Dec-2004 16:21   3.7M  
 728d.segment2.gong.dat  08-Mar-2004 12:09   3.3M  
 728d.segment2.gong.txt  15-Dec-2004 16:21   3.5M  
 728d.segment2.mdi.dat   22-Mar-2004 09:50   3.4M  
 728d.segment2.mdi.txt   15-Dec-2004 16:21   3.6M  
 728d.segment3.gong.dat  10-Mar-2004 10:18   3.3M  
 728d.segment3.gong.txt  15-Dec-2004 16:21   3.6M  
 728d.segment3.mdi.dat   22-Mar-2004 09:55   3.4M  
 728d.segment3.mdi.txt   15-Dec-2004 16:21   3.6M  
 728d.segment4.gong.dat  12-Mar-2004 12:59   3.3M  
 728d.segment4.gong.txt  15-Dec-2004 16:21   3.6M  
 728d.segment4.mdi.dat   23-Mar-2004 14:58   3.5M  
 728d.segment4.mdi.txt   15-Dec-2004 16:22   3.7M  
 728d.segment5.gong.dat  25-Mar-2004 16:01   3.2M  
 728d.segment5.gong.txt  15-Dec-2004 16:22   3.5M  
 728d.segment5.mdi.dat   25-Mar-2004 15:59   3.5M  
 728d.segment5.mdi.txt   15-Dec-2004 16:22   3.7M  

Mar  7 2007 

  Additional segments have been since fitted, and the rejection criteria for
the fitted modes has been reviewed and set to be less stringent.

  Look at ../2007/README

Dec 15 2004

  I've generated *.txt files, these are ASCII files too, but:

   - have a 5 lines 'header' 

  and

   - are formatted using a fixed format (5(I3,X),12(E19.12,X))

For additional details and reference, look at

  S.G. Korzennik, A Mode-Fitting Methodology Optimized for Very Long
  Helioseismic Time Series, ApJ, 626:585--615, June 2005.
  [2005ApJ...626..585K]

or the preprint available at:

  http://www-sgk.harvard.edu:8080/~sylvain/preprints/yaopbm.ps.Z
  http://www-sgk.harvard.edu:8080/~sylvain/preprints/yaopbm.pdf

May 14 2004 

  The tables resulting from fitting MDI & GONG times series, for 1 <= L <= 25,
  are in the files:

    2088d.gong.dat: results from fitting GONG 2088-day-long time series
    2088d.mdi.dat:  results from fitting MDI  2088-day-long time series

    728d.segmentN.gong.dat: results from fitting GONG 728-day-long time series
                            for segment N, where N = 1...5
    728d.segmentN.mdi.dat:  results from fitting MDI  728-day-long time series
                            for segment N, where N = 1...5

File format:

  ASCII table, with first 4 lines being a 'header', which is followed by the
  data in 17 columns:

 Column  1: N         radial order
         2: L         sph harm degree
         3: M         azimuthal order
         4: NMTP      no of multitapers used to estimate the power spectrum
         5: KEPT      flag, =1 if this multiplets is inside 3-sigma when
                      fitting all m values to a Clebsh-Gordan expansion,
                      otherwise =0 
         6: BETA      horiz-to-vert ratio used to compute leakage matrix
         7: FWHM      full width at half max (independant of m)
         8: ALPHA     asymmetry              (independant of m)
         9: FREQ      frequency
        10: AMP       power amplitude        (arbitrary units)
        11: BGD       background power level (arbitrary units)
        12: SFWHM     error bar on full width at half max
        13: SALPHA    error bar on asymmetry
        14: SFREQ     error bar on frequency
        15: SAMP      error bar on power amplitude
        16: SBGD      error bar on background power level
        17: FITRMS    RMS(model-observations)