Converts FITS magnetic tape files into NDFs.
[]
. The file specifiers indicate which files from the
tape are to be processed. For example: [2]
indicates the second file on the tape. [4-6]
indicates files 4 to 6. [5-]
indicates file 5 to the last file on the tape. [1,3-5,7-]
indicates files
1,3,4,5, and 7 to the end of the tape. If no file specifiers are given, all files on the tape will be
processed. *
, which will be replaced by the
corresponding FITS tape file number. If OF is not specified, mtf2ndf*.fits
will be used
and deleted. (See also "
Notes"
). "*"
. <fits2ndf_pars>
tcsh
script which calls an ADAM A-task. Convert startup sets alias
mtfits2ndf
to ‘tcsh mtfits2ndf.tcsh
’, and tcsh
must be on the user’s PATH. /dev/nst0
to an NDF called f256
. The FITS blocking factor of the tape is 10. As a result of
the parameters passed to FITS2NDF, the data type of the NDF’s data array matches that of the FITS
primary data array, a FITS extension is created in f256
, and FITS sub-files are propagated to NDF
extensions. /dev/nst0
(with a blocking factor of 1) to FITS disk files named ral256_*.fit
, where *
is
replaced by each tape file number. The FITS files will be converted to NDFs named ral256_*
and retained. NASA Office of Standards and Technology, 1997, A User’s Guide for the Flexible Image Transport System (FITS), Version 4.0.
NASA Office of Standards and Technology, 1999, Definition of the Flexible Image Transport System (FITS).