========================================================================== J/A+A/390/717 Solar Velocities of the Sun in 1989-99 (IRIS++) (Salabert+, 2002) The following files can be converted to FITS (extension .fit .fgz or .fiZ) v*.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/390/717 ==========================================================================
drwxr-xr-x 19 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:58 [TAR file] -rw-r--r-- 1 cats archive 465 Oct 24 2002 .message -r--r--r-- 1 cats archive 6950 Oct 24 2002 ReadMe -rw-r--r-- 1 cats archive 213 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2047 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 1693017 May 30 2002 v89f.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 3317496 May 30 2002 v90f.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 3823834 May 30 2002 v91f.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 3787643 May 30 2002 v92f.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1706274 Jul 18 2002 v93f.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 4054386 May 30 2002 v94f.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 4214675 May 30 2002 v95f.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 4082954 May 30 2002 v96f.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 4318829 May 30 2002 v97f.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 4225997 May 30 2002 v98f.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 3235454 May 30 2002 v99f.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/390/717 Solar Velocities of the Sun in 1989-99 (IRIS++) (Salabert+, 2002) ================================================================================ IRIS++ database: Merging of IRIS + Mark-1 + LOWL Salabert D., Fossat E., Gelly B., Tomczyk S., Palle P.L., Jimenez-Reyes S.J., Cacciani A., Corbard T., Ehgamberdiev S., Grec G., Hoeksema J.T., Kholikov S., Lazrek M., Schmider F.X. <Astron. Astrophys. 390, 717 (2002)> =2002A&A...390..717S ================================================================================ ADC_Keywords: Sun ; Radial velocities Keywords: Sun: instruments - Sun: signal analysis - Sun: database - Sun: helioseismology Abstract: The IRIS (International Research of Interior of the Sun) network has been operated continuously since July 1st 1989. To date, it has acquired more than a complete solar cycle of full-disk helioseismic data which has been used to constrain the structure and rotation of the deep solar interior. However, the duty cycle of the network data has never reached initial expectations. To improve this situation, several cooperations have been developed with teams collecting observations with similar instruments. This paper demonstrates that we are able to merge data from these different instruments in a consistent manner resulting in a very significant improvement in network duty cycle over more than one solar cycle initiating what we call the IRIS++ network. Description: The precise measurement of the solar seismic properties requires year long measurements as uninterrupted as possible. The cooperation between several groups managing instruments all around the world has produced the one solar cycle long IRIS++ data bank. Integrated radial velocities from mid-1989 up to end-1999 measured by the ground-based IRIS++ network are presented. The full-disc integration gives access to low degree p-modes (l=0, 1, 2 & 3).
© UDS/CNRS