The purpose of a Instrument parameter file is to set default values
for that instrument. These files are described in the GSAS manual
(p158 in the 1990 version, p176 in the 1994 version).
Below are two files, one for a CW neutron instrument and one for a
synchrotron instrument. I will try to explain what I know.
BANK      It is possible to describe several different instrument
          configurations in a single file and then select the appropriate
          bank number. In most CW cases this is not needed.
          Data for bank 1 is prefixed by "INS  1..." Data for bank 2
          would be "INS  2..."
The HTYPE statement describes the type of data.
	The first letter is P for powder S for single xtal
	The second letter is N or X for neutron or X-ray
        The third letter is T for TOF or C for CW
        I forget what the 4th letter is for, I think it means ready for use.
The ICONS entry (for CW) describes wavelength1, wavelength2, zero and POLA
	(change these values in the overall parameters-instrument
         constants menu)
The "I HEAD" entry can have any text
The "I ITYP" entry describes an incident spectrum correction needed
           for energy dispersive but not CW instruments.
	Put 0 as the 1st number and
	your maximum 2theta range for the second two numbers
	the 4th does not matter.
"INS  1 IRAD"   specifies a x-ray radiation type. Use 3 for CuKa radiation.
The "INS  1PRCFnn" defines the default profile parameters where the
                   first set specified is the default.
   on the first card ("INS  1PRCF1" or "INS  1PRCF2") the entries are
	profile#, # of parameters, cut-off
   the remaining cards are the profile parameters for that profile function
   (U, V, W,...)
The best way to set these is to complete a refinement on a standard with
pretty sharp peaks and then copy the values from the .EXP file (see below).
Change the prefix "HAPn" to "INS ". With good data and a reasonable structure,
you can start a refinement with pretty rotten starting values and then fit
them. Start by fitting W only... You probably won't be able to refine V with a
conventional instrument.
in .EXP file:
HAP1 1PRCF      2   12   0.00500    0YYYNYNNNNNNNNNNNNNNN
HAP1 1PRCF 1   0.205738E+03  -0.160655E+03   0.117736E+03   0.000000E+00
HAP1 1PRCF 2   0.103780E+02   0.000000E+00   0.500000E+01   0.000000E+00
HAP1 1PRCF 3   0.000000E+00   0.000000E+00   0.000000E+00   0.000000E+00
CW Neutron instrument parameter file:
-------------------------------------
INS   BANK      1
INS   HTYPE   PNCR
INS  1 ICONS   1.54020   0.00000   0.04000         0
INS  1I HEAD   NIST BT-1 instrument
INS  1I ITYP    0    5.0000  168.0000         1
INS  1PRCF1     1    6   0.00500
INS  1PRCF11   0.179000E+03  -0.301000E+03   0.181000E+03   0.500000E+01
INS  1PRCF12   0.000000E+00   0.000000E+00
INS  1PRCF2     2   12   0.00500
INS  1PRCF21   0.179000E+03  -0.301000E+03   0.181000E+03   0.000000E+01
INS  1PRCF22   0.000000E+00   0.000000E+00   5.000000E+00   0.000000E+00
INS  1PRCF23   0.000000E+00   0.000000E+00   0.000000E+00   0.000000E+00
Synchrotron Neutron instrument parameter file:
----------------------------------------------
INS   BANK      1
INS   DTYPE   STND
INS   HTYPE   PXCR
INS  1 ICONS  1.540510  0.000000       0.0         0
INS  1 IRAD     0
INS  1I HEAD  DUMMY INCIDENT SPECTRUM for x7a
INS  1I ITYP    0    0.0000  150.0000
INS  1PRCF1     2   12      0.01
INS  1PRCF11   0.000000E+00   0.000000E+00   0.800000E+02   0.000000E+00
INS  1PRCF12   0.000000E+00   0.000000E+00   0.000000E+00   0.000000E+00
INS  1PRCF13   0.000000E+00   0.000000E+00   0.000000E+00   0.000000E+00
Hope this helps,
Brian
-- ***************************************************************************Brian H. Toby Reactor Radiation Division E151/235Brian.Toby@NIST.gov National Institute of Standards & Technologyvoice: 301-975-4297 FAX: 301-921-9847 Gaithersburg, MD 20899***************************************************************************